Kvant
Kvant 1971, No. 5

Kvant 1971, No. 5 · Pages

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Popular science physics and mathematics
quantum
5
1971
magazine
Academy
Sciences of the USSR
and the Academy of Pedagogical
Sciences of the USSR

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3

In the room:

P. L. Chebyshev (1821—1894)
1
About Bertrand’s postulate
4
Potential Energy Graphs
8
Hippocrates’ moons
17
Math circle
Physics helps geometry
22
Laboratory “Quenta”
Impossible objects
26
Photographing impossible objects
27
Problem “Quenta”
Tasks
30
Solutions to problems M31-M33;
F43, F48-F52
32
Applicant’s workshop
What is here - are we losing or is it here!
40
Entrance written exam
in mathematics at the faculty
computational mathematics
and cybernetics of Moscow State University in 1970
42
Entrance written exam
in mathematics at MIPT in 1970
46
Problems using Newton’s laws
50
Information
Moscow Mathematical…
58
Answers, directions, solutions
60
Collector’s Corner
3rd cover page
N. N. Kolesnikov
M. I. Bashmakov
R. G. Mints
V. N. Berezin
B. Yu. Kodan
L. Penrose,
R. Penrose
V. I. Bakhmin
I. N. Bernitsa,
A. B. Zelevinsky,
A. G. Kushinrenko,
I. Sh. Slobodetsky
V. A. Petrov
Sh. A. Alimov,
F. P. Vasiliev,
V. P. Modenov
A. P. Savin,
B.V. Fedosov
Yu. V. Zaychikov
A. G. Terushkin

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The scientific interests of P. L. Chebyshev are distinguished by their great diversity and breadth. He left behind extensive research in the field of mathematical analysis, especially in the theory of approximation of functions by polynomials, in intercalculus, number theory, probability theory, geometry, ballistics, theory of mechanisms and other fields of knowledge.

In each of these areas of science, Pafnuty Lvovich obtained functional results, developed new ideas and methods that determined the development of these branches of mathematics and mechanics for many years and retained their significance to this day.

At the same time, it gives rise to Chebyshev’s ability to obtain excellent scientific results using simple, elementary means.

Another important feature of P. L. Chebyshev’s scientific activity is his constant interest in practical issues, the desire to connect theoretical problems of mathematics with the needs of natural and technical, practical activities of people. In the light of modern trends in the development of science, the programmatic setting of scientific activity by P. L. Chebyshev seems extremely practical: “The practical activity of man is extremely diverse, and in order to satisfy all its requirements, there are not enough sciences and many different methods. But of these, especially important are those that are necessary to solve various modifications of the same problem, common to all practical human activity: how to allocate one’s means to achieve the greatest possible benefit” (P. L. Chebyshev, Socinnia, vol. II, St. Petersburg, 1907, p. 239).

It should be noted that for Pafnutya Lvovich himself, his interest in practice turned out to be extremely fruitful, since many of his mathematical discoveries were made while solving applied problems. For example, the study of the hinge mechanism, known as the “Watt parallelogram,” led him to the creation of the basic theory of the best approximation of functions by polynomials, which has now turned into a widely developed mathematical field of great applied importance. In terms of the richness of mathematical ideas, the significance of the results obtained and the study of their acquisition, the work of P. L. Chebyshev “The Theory of Mechanisms Known as a Parallelogram” (1854) is outstanding. In this method, Chebyshev introduces and solves the famous problem: “Given a continuous function f(x); among all polynomials P(x) of degree n, find one such that in a given interval the maximum value of the difference |f(x) - P(x)| it was possible to do less." If the function itself is a polynomial of degree n+1, then the problem posed is equivalent to finding a polynomial of the same degree, with the same coefficient for the leading term, which deviates less from zero on the interval under consideration. This is how the famous “Chebyshev complete nomes” arose - polynomials that “deviate least away from zero” in the interval [−1, +1]: T_n(x) = \frac{1}{2^{n-1}} \cos(n \arccos x). (These expressions are polynomials in x of degree n. The coefficients of the highest degree of these polynomials are equal to one.) Chebyshev also studied the approximation of functions after a variety of functions and trionometric polynomials. (A rational function is the ratio of two polynomials, and a trionometric polynomial is a polynomial of sin x and cos’x.)

In probability theory, Chebyshev managed to obtain a number of important results using extremely simple means. Many results and conclusions were only named, not completed, but all of Chebyshev’s work in this area was the basis on which the Russian school of probability theory developed. Rigorous proofs of polynomials, the least

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Chebyshev, and their further development was carried out by his students, academicians A. M. Lyapunov and A. A. Markov.

P. L. Chebyshev’s research in number theory was of outstanding importance for science. For the first time since Euclid, with surprisingly witty and surprisingly elementary reasoning, he obtained the most important results in the problem of the distribution of prime numbers in the works “On Determining the Number of Prime Numbers Not Exceeding a Given Value” and “On Prime Numbers.” P. L. Chebyshev proved that the function x(x)−xx(x) - x of simply numbers not exceeding them xx satisfies the inequality

0,92<π(x)ln⁡xx<1,06∗0,92 < \frac{\pi(x)\ln x}{x} < 1,06^*

for sufficiently large xx. This inequality was then somewhat studied by the English mathematician Sylvester, and the French mathematician Hadamard strictly proved that

lim⁡x→∞[π(x):xln⁡x]=1\lim_{x \to \infty} \left[ \pi(x): \frac{x}{\ln x} \right] = 1

or asymptotically π(x)∼x/ln⁡x\pi(x) \sim x/\ln x.

Here Chebyshev proved the statement (the so-called Bertrand postulate), which is that between xx and 2x(x≥2)2x(x \geq 2) there is always at least one prime number **).

Classic results were also obtained by Chebyshev in the field of mathematical analysis.

One of the sciences that Pafnuty Lvovich was interested in throughout his life was the theory of mechanisms and machines, and Chebyshev was engaged not only in theoretical research in this area, but also paid more attention to the direct design of mechanisms.

Long before the Soviet Lunokhod 1 continued the first route

ln⁡x−log⁡ax по основанию e,\ln x - \log_a x \text{ по основанию } e,

where e=lim⁡n→∞(1+1n)ne = \lim_{n \to \infty} \left(1 + \frac{1}{n}\right)^n.

**) For the method by which Chebyshev obtained his remarkable results, see pp. 4-7.

Sou on the lunar surface, science fiction and scientists considered various options for machines that would exist for some walking mechanism. P. L. Chebyshev developed a version of a plantigrade machine that imitates the movement of an animal when walking.

The enormous influence of P. L. Chebyshev on the development of mathematics in our country is not limited to his personal achievements. His works, exceptionally rich in new ideas and methods, gave a powerful impetus to the development of diverse branches of mathematics and mechanics; in addition, he personally posed important tasks and problems for young scientists. On his direct advice, A. M. Lyapunov began research on the theory of the figuration of rotating life, where he obtained classical results that are of paramount importance for mechanics and cosmogony.

The great mathematician and mechanic P. L. Chebyshev was a leading man of his time. So, for example, together with two other academician mathematicians - V. G. Imshenetsky and V. Ya. Bunyakovsky - he proposed to the physics and mathematics department of the St. Petersburg Academy to elect a wonderful Russian living spirit - Sofya Vasilievna Kovalevskaya **) as a corresponding member of the Academy.

Chebyshev paid a lot of attention to issues of public education, taking an active part in the Academic Committee of the Ministry of Education.

The scientist’s works, his scientific, pedagogical and educational activities, and the famous St. Petersburg mathematical school he founded played an exceptionally large role in the development of accounting mathematics and mechanics. In 1944, the USSR Academy of Sciences established the P. L. Chebyshev Prize for the best research in the field of mathematics and the theory of mechanisms and machines.

**) S.V. Kovalevskaya was elected on November 7, 1889.

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ABOUT BERTRAND’S POSTULATE

M. I. Bashmakov

Among the 69 works of Pafnuty Lvovich Chebyshev, two works played a particularly important role in the development of number theory. These works: “On determining the number of prime numbers not exceeding a given value” and “On prime numbers,” written by him in his youth, are related to the most difficult question in number theory: the distribution of prime numbers.

In the second of these works, inequalities are indicated that make it possible to fairly accurately estimate the number of prime numbers in a given segment of the natural series and, in particular, the following fact is proven: between xx and 2x2x (where x>1x>1) there is always at least one prime number. This statement was made by the famous French mathematician Bertrand, who tested it within the existing tables of prime numbers, but was unable to prove it and accepted it as a construct.

We will trace Chebyshev’s main ideas that led him to these estimates, and then propose a series of problems whose solutions allow readers (familiar enough with the properties of logarithms) to reconstruct Ukazyv’s proof of Bertrand’s construction and obtain inequalities for the number of prime numbers not exceeding a given value.

The reader may wonder what does logarithm have to do with prime numbers? This is the merit of Chebyshev, that he pointed out how to use the general functions of analysis - roots, logarithms - in the study of problems about integers. If we want to find out whether there is at least one prime number on the interval from nn to 2n2n, then we can proceed as follows:

  1. come up with some function y=f(x)y=f(x) of the real argument xx that would not change its value while xx runs through the segment between neighboring prime numbers, and would take on a larger value when passing through a prime number;

  2. prove inequalities for the relative function ff, which would help to estimate the growth rate quite accurately.

For a function chosen in this way, the difference f(2n)−f(n)f(2n) - f(n) will be a positive number if and only if the function ff returns when moving from nn to 2n2n, that is, if there is at least one prime number between nn and 2n2n.

The first condition is easy to satisfy. We can consider the following function: let us denote by π(x)\pi(x) the number of prime numbers not exceeding xx.

For example, π(1)=0\pi(1) = 0 (one is not considered a prime number), π(3)=2\pi(3) = 2, π(9)=4\pi(9) = 4, π(9,5)=4\pi(9,5) = 4, π(10,9)=4\pi(10,9) = 4, π(11)=5\pi(11) = 5, etc.

Of course, if we could prove that

π(2x)−π(x)>0,\pi(2x) - \pi(x) > 0,

we would have proved Bertrand to act, since

π(2x)−π(x)\pi(2x) - \pi(x)

just denotes the number of prime numbers contained between xx and 2x2x.

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GRAPHICS
POTENTIAL
ENERGY

R. G. MINZ

How to find out whether body movement is limited and to what extent? Do equilibrium positions exist, and if so, are they stable or unstable?

In this article we will show that such questions are easy to answer if the potential energy of the body is known. We’ll discuss when it makes sense to talk about potential energy and how to calculate its magnitude at each point.

If we talk about potential energy, it means that we want to study the motion of a body, more precisely, of material points *), based on the law of conservation of mechanical energy.

This law states that for a closed system of material points (bodies) the quantities

E=T+U.E = T + U.

(1)

Sum

T=m1v122+m2v222+⋯+mnvn22T = \frac{m_1 v_1^2}{2} + \frac{m_2 v_2^2}{2} + \dots + \frac{m_n v_n^2}{2}

is called the kinetic energy of the system, and UU is the potential energy of the interaction of the body. Kinetic energy in formula (1) reflects the body’s own motion, and potential energy, which depends on the distances between bodies, their mutual influence on each other.

In what follows, for simplicity, we will consider the movement only

*) As usual, by a material point we mean a body whose own dimensions in this problem are negligible.

one of the material points *), assuming that all the others are at rest. In such cases, we usually talk about the motion of a particle in an external strong field, and formula (1) takes the form

E=mv22+U.E = \frac{mv^2}{2} + U.

(2)

Speaking about the movement of a particle in an external field, we will consider the influence of stationary parts on moving ones, and all systems of parts as a whole are closed. There is, however, a subtlety to this. Let us trace it visually using the example of two materials of points with masses mm and MM. Let a particle of mass MM dig around at some moment. Let us find out under what conditions it continues to remain motionless, that is, it will be possible to talk about the movement of a particle of mass mm in an external field. Let’s use the law of conservation of momentum

*) The problem of the movement of a large number of telecommunications interacting with each other is extremely complex. Until now, they had only been able to solve the problem of two bodies in a general form.

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nia (after all, our system of bodies is closed): Mv⃗+mv⃗1=mv⃗0M\vec{v} + m\vec{v}_1 = m\vec{v}_0. (Here v⃗0\vec{v}_0 is the initial speed of a particle with mass mm, v1v_1 is its speed after some time and vv is the speed acquired by particles with mass MM.)

Hence v⃗=mM(v⃗0−v⃗1)\vec{v} = \frac{m}{M} (\vec{v}_0 - \vec{v}_1). If v⃗1≠v⃗0\vec{v}_1 \neq \vec{v}_0, then v⃗=0\vec{v} = 0 only when M→∞M \to \infty Physical this means that m≪Mm \ll M. Thus, the external field is the result of the action of heavy stationary particles on light ones. Let us recall two typical examples of an external field: a satellite in the Earth’s gravitational field, an electron in the field of a nucleus. In each of these examples, of course, condition m≪Mm \ll M is satisfied.

If the total energy EE of the particle is given, then correspondence (2) imposes restrictions on in which region of space the particle can be located. Indeed, after all, the kinetic energy Ekin=mv22E_{\text{kin}} = \frac{mv^2}{2} allows on the basis of 2mEkin\sqrt{\frac{2}{m}} E_{\text{kin}} to be minimal!), and from the law of conservation of energy it follows that

mv22=E−U.\frac{mv^2}{2} = E - U.

Thus, E≥UE \geq U; we have obtained a criterion for determining the region in which movement with total energy EE is possible. At points where E=UE = U, kinetic energy, and therefore speed, vanishes.

Let us consider as an example the movement of a body along a straight line (axis xx). Then the potential energy depends only on the position on this line: U=U(x)U = U(x). In this case, our criterion is very convenient to apply graphically. Let us draw a straight line U(x)=EU(x) = E on the horizontal potential energy graph. Wherever the potential energy graph passes below the straight line, E>UE > U and movement is possible. At the points of intersection, speed

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Fig. 2. The body, moving to the left, approaches the point x1x_1, where its speed is zero. One cannot accumulate at this point, since a force acts on it (see the sled rule on page 12). Therefore, it will continue to move to the right, increasing speed.

Knowing the potential energy, it is easy to determine the speed of the particle at each point. Since mv22=E−U\frac{mv^2}{2} = E - U, then v=±2m[E−U]v = \pm \sqrt{\frac{2}{m} [E - U]}.

Two signs of speed correspond to two possible directions of movement along the xx axis. figure 2 graphically shows the dependence of the particle velocity on its position for the case when the energy and potential energy correspond to figure 1a. The direction of movement is indicated on the graph by an arrow.

So, we see that with the help of potential energy graphs we can simply and clearly find out where the possibility of movement is, what type of trajectories it has and how the speed of a body depends on its position. When clarifying these questions, we needed to know the behavior of potential energy as a function of coordinates “in general,” that is, how it behaves along the entire trajectory.

Let’s now see what is associated with the rate of change of potential energy, that is, the quantity

ΔUΔx=U(x2)−U(x1)x2−x1,\frac{\Delta U}{\Delta x} = \frac{U(x_2) - U(x_1)}{x_2 - x_1},

where Δx=x2−x1\Delta x = x_2 - x_1 is very small

According to the law of conservation of mechanical energy

ΔU=U(x2)−U(x1)=mv122−mv222=m2(v1+v2)(v1−v2)\Delta U = U(x_2) - U(x_1) = \frac{mv_1^2}{2} - \frac{mv_2^2}{2} = \frac{m}{2} (v_1 + v_2) (v_1 - v_2)

where v1v_1 is the speed of the body at point x1x_1, and v2v_2 is its speed at point x2x_2. In a small area Δx\Delta x the force acting on the body can be considered constant. Movement under the influence of a constant force, which means FF, equal to acceleration, and acceleration a=F/ma = F/m. In this case, v2−v1=aΔt=FmΔtv_2 - v_1 = a \Delta t = \frac{F}{m} \Delta t (Δt\Delta t is the time of movement), and v1+v22\frac{v_1 + v_2}{2} is equal to the average speed v1+v22=vcp=ΔxΔt\frac{v_1 + v_2}{2} = v_{cp} = \frac{\Delta x}{\Delta t}. Let’s substitute these expressions into formula (4):

ΔU=mΔxΔt(−FmΔt)=−FΔx.\Delta U = m \frac{\Delta x}{\Delta t} \left( -\frac{F}{m} \Delta t \right) = -F \Delta x.

From here

ΔUΔx=−F.\frac{\Delta U}{\Delta x} = -F.

Formula (5) can also be obtained otherwise, taking into account that with uniform motion only the potential energy of the body changes and its change is equal to the work of the force acting on the body.

Let us find out the geometric meaning of formula (5). Let us be given a potential energy graph. It is clear that the smaller the value of x2−x1x_2 - x_1, the more accurately the rate of change of potential energy coincides with the tangent of the tangent to the potential energy curve (Fig. 3). Action

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Indeed, tgα1=ab=U(x2)−U(x1)x2−x1tg\alpha_1 = \frac{a}{b} = \frac{U(x_2) - U(x_1)}{x_2 - x_1}, and the smaller x2−x1x_2 - x_1, the more accurately the angle α1\alpha_1 is equal to the angle α\alpha. Thus, we come to the conclusion that the tangent of the tangent to the potential energy graph, taken with the opposite sign, coincides with the force acting on the body. This means that the more the potential energy increases, the greater the magnitude of the force and vice versa.

After formula (5) has acquired a clear geometric meaning, it is easy, for example, to find out whether equilibrium positions exist and what they are. We call the equilibrium position the point at which a body can remain for as long as possible, provided, of course, that it initially has zero speed. When is this possible? A change in speed is characterized by acceleration: if it is zero, then the speed of the body is unchanged. Acceleration is proportional to the force acting on the body. This means that equilibrium positions are those points where the force vanishes.

Let’s look again at the potential energy graph. As we have already seen, the force acting on a body is equal to the tangent of the tangent to the potential energy curve taken with the opposite sign. If this angle is zero, then the force is zero. Thus, on the potential energy graph, the equilibrium positions correspond to those points at which
Fig. 4

Fig. 5a,6

whose tangent is parallel to the abscissa axis. It is obvious, for example, that equilibrium positions are maxima and minima of potential energy (Fig. 4).

Equilibrium positions can be stable and unstable. What do you mean? Let us slightly deviate the body from its equilibrium position. If at the same time the force acting on the body returns it back, then the equilibrium is called stable; if not, then it is unstable.

Let us examine for stability the equilibrium position corresponding to the minimum on the potential energy curve (point AA on Fig. 4). Let the body move from point AA to the right. In the new position A1A_1 (Fig. 5 a), the tangent of the tangent angle is positive, and the force is negative, that is, directed in the direction opposite to the displacement and returns the body to

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point AA. If you should merge to the left of point AA, then in this position (A2A_2 on Fig. 5 a) the tangent of the tangent angle is negative, the force is positive, that is, directed to point AA and forces the body to return to its original position. Thus, the equilibrium position at the minimum potential energy is stable. Similarly, we can consider the stability of the equilibrium position if the potential energy is maximum (Fig. 5 b).

So, we see that from the potential energy curve we can find the magnitude of the force acting on the body, and it is easy to determine where the equilibrium positions are and what they are. In this sense, the potential energy graph can be compared to an ice slide from where it descends to the Sankh. In those places where the hill is round, the sled accelerates quickly; on a gentle descent, it accelerates more slowly. The top of the slide and the depressions in it are the equilibrium positions. After all, if you put a sled there, they will stay there. In this case, the top is the position of unstable equilibrium, and the valley is stable.

Now, perhaps, let’s talk about how to calculate the value of potential energy. To do this, let us return again to formula (5) and rewrite it in the form

U(x2)−U(x1)=−F⋅(x2−x1).U(x_2) - U(x_1) = -F \cdot (x_2 - x_1).

Recall that the length Δx=x2−x1\Delta x = x_2 - x_1

Fig. 6

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The energy of the body is equal to the area taken with the opposite sign *) under the graph of the dependence of the action of force on the body on the coordinates **). Then its graph is a straight line parallel to the x-axis. The area under it is equal to F⋅(x−x0)F \cdot (x - x_0), from where we obtain for the difference in potential energies

U(x)−U(x0)=−F⋅(x−x0)U(x) - U(x_0) = -F \cdot (x - x_0)

(Fig. 7a, b).

Using correspondence (8) we obtain

mv22−mv022=F⋅(x−x0).\frac{mv^2}{2} - \frac{mv_0^2}{2} = F \cdot (x - x_0).

mv22−Fx=mv022−Fx0,\frac{mv^2}{2} - Fx = \frac{mv_0^2}{2} - Fx_0,

that is, potential energy U=−FxU = -Fx. However, this is not the only possibility; with the same reason we could write such an equality

mv22−Fx+C=mv022−Fx0+C,\frac{mv^2}{2} - Fx + C = \frac{mv_0^2}{2} - Fx_0 + C,

where CC is a constant number. But then the potential energy is U=−Fx+CU = -Fx + C. Thus, we see that the potential energy is determined exactly up to an arbitrary constant. This can be explained by the very law of conservation of mechanical energy. After all, if we say that the quantities E=mv22+UE = \frac{mv^2}{2} + U are conserved, then E′=mv22+U+CE' = \frac{mv^2}{2} + U + C is also conserved, where CC is some constant. But in this case U′=U+CU' = U + C. This means that potential energy can only be determined to an accuracy of an arbitrary constant, which is always chosen from messages of convenience *). Of course, such uncertainty of potential energy does not in any way affect the conclusions we have drawn about the characteristics of motion in a given field, the presence of equilibrium positions in it, and the dependence of the body’s speed on the coordinate. You can easily verify this; you only need to simultaneously change the potential energy by values ​​CC and change the total energy of the body by the same amount. The fact is that to fully describe the movement of a body, it is necessary to specify its position and speed at some moment

*) It should be noted that if the force is negative, then the corresponding participation should be assigned a minus sign.

*) A field in which the force acting on the body is constant everywhere is called homogeneous. Homogeneous, for example, is the gravitational field near the Earth’s surface F=mgF = mg and the electric field inside a flat capacitor.

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Fig. 8

time, thereby we will know
mv022\frac{mv_0^2}{2} and U(x0)U(x_0) Polyana energy
E=mv022+U(x0)E = \frac{mv_0^2}{2} + U(x_0) By adding some constant value to UU, the energy of EE will increase by exactly the same amount.

Let us now consider the motion of the cube outside in the absence of friction (Fig. 8) and calculate what the potential energy is in this case. According to Hooke’s law, the force acting on the cube is equal to F=−kxF = -kx, where kk is the stiffness of the spring xx is its deformation. In this case, the graph of the force is straight, the tangent of the angle of inclination of which to the axis xx equals kk (Fig. 9a)

The potential energy difference U(x1)−U(x0)U(x_1) - U(x_0) is equal to the area of ​​the trapezoid ABCDABCD protected on Fig. 9a, the height of which is BC=x1−x0BC = x_1 - x_0. and we get the main AB+CD2=kx0+kx12\frac{AB + CD}{2} = \frac{kx_0 + kx_1}{2}. Using the formula for the area of ​​a trapezoid, we find that U(x1)−U(x0)=(x1−x0)(kx0+kx1)2=k(x12−x02)2=kx122−kx022U(x_1) - U(x_0) = \frac{(x_1 - x_0)(kx_0 + kx_1)}{2} = \frac{k(x_1^2 - x_0^2)}{2} = \frac{kx_1^2}{2} - \frac{kx_0^2}{2}.

As a result, for U(x)U(x) we obtain the following expression: U(x)=kx22U(x) = \frac{kx^2}{2}

*) Similar to the case of a homogeneous field with constant CC, we chose here so that U(0)=0U(0) = 0.

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cases (F=const.F=−kxF = \text{const.} \quad F = -kx) it is impossible to calculate this area without knowledge of integral calculus. If we find it, then it turns out that for a force changing according to the law F=αr2F = \frac{\alpha}{r^2}, the potential energy

U=αrU = \frac{\alpha}{r}

Please note that in formula (10) we have chosen the constant CC so that the potential energy vanishes at infinity. Why is this convenient and when? Let us remember that potential energy characterizes the action of bodies on each other—interaction; if at infinity the force becomes zero, then the further the bodies are separated from each other, the weaker their mutual influence. This is precisely why the choice of constant in our and similar (F(∞)=0F(\infty) = 0) cases is accordingly.

From formula (10) it follows that the type of potential energy significantly depends on the sign of α\alpha (see Fig. 106). If α>0\alpha > 0, then the force is F=αr2>0F = \frac{\alpha}{r^2} > 0, and we are dealing with repulsion (like charges, α=q1q2>0\alpha = q_1 q_2 > 0). If α<0\alpha < 0, then the force is F=−∣α∣r2<0F = -\frac{|\alpha|}{r^2} < 0, which corresponds to attraction (opposite charges, α=−q1∣q2∣\alpha = -q_1 |q_2|). Here, please, it is worth returning once again to the analogy with a sled going down an ice slide. Notice that if you put a sled on a slide that has a potential energy interwash profile, they point in the direction of the force. Such a set of rules makes it possible to immediately determine whether attraction or repulsion is taking place. Indeed, if the sank is shown to the point r=0r = 0 (for example, the lower curve at Fig. 106), then attraction takes place, if on the contrary (for example, the upper curve), then repulsion occurs.

The same rule allows us to qualitatively construct the type of potential

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Stifling. At large distances, attraction quickly kills, and recoil when approaching, starting from a certain distance, returns very sharply. The described picture of the interaction of atoms corresponds to the potential energy graph. Shown-

16

nyy on figure 11 Make sure of this, use the analogy with an ice slide. Point r=r0r=r_0 corresponds to the position of stable equilibrium, and therefore r0r_0 is equal to the distance between atoms in the molecule.

In conclusion, let us summarize some results. We have seen that from the potential energy graph we can find out a number of essential characteristics of movement (the number of different trajectories depending on the energy, whether the movement is limited or not, whether there are equilibrium positions and whether they are stable or unstable). Each of them, as it turned out, has a simple geometric meaning. It is also easy to determine the magnitude and direction of the force acting on the body (“the sled rule”). We have shown that the area under the force graph, taken with the opposite sign, is equal to the potential energy of the body. This makes it possible in some cases to directly calculate potential energy. This makes solving various problems much easier.

And finally, we have seen how the qualitative form of potential energy allows us to understand what exists and give an answer to it.

Now try to solve the following problems yourself.

Exercises

  1. Find out the area of ​​possible movement when
    E<U0E<U_0 and E>U0E>U_0.
    if the potential energy has the form shown in Fig. 12.

  2. Find equilibrium positions along the potential energy curve (Fig. 13) and find out their stability.

Draw a graph of force versus coordinate.

  1. Show geometrically that when the potential energy changes by a constant value CC, the force acting on the body at each point does not change.

  2. A cube with side aa of density ρ1\rho_1 floats on the surface of a liquid whose density is ρ2\rho_2. Draw graphs of the force acting on the cube and the potential energy depending on the depth of the piercing.

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HOLES
HIPPOCRATES

In the fifth century BC, that is, almost two and a half thousand years ago, a scientist lived in Greece, named Hippocrates of Chios. It was Hippocrates who made the first known attempt to create the “Elements” of geometry. Unfortunately, this book has not reached us.

According to one legend, the unlucky merchant Hippocrates was limited to his ancestors and went to Athens to desire them. Here he met sages who spent their time mainly solving geometric problems. Having not found justice for the robbers, Hippocrates consoled himself with the fact that he surpassed the most skilled sages in geometry. . .

Hippocrates tried to square the circle, in other words, to construct a circle equal in size to a given square using a compass and ruler. And although he, naturally, did not succeed, he managed to construct several figures, which were pieces of a plane, limited by two circles, and nevertheless equal in size to a square.

In the history of geometry, the name of Hippocrates is associated with figures of a special type, the so-called lune. A lunula (in other words, a crescent) can be defined as follows: on a chord of an arbitrary circle, a semicircle is constructed externally, the ends of which coincide with the ends of the chord. Figure bounded by a smaller arc

the circumference of a given circle and the drawn semicircle is the hole.

On figure 1, four holes are also painted in the desired color. Hippocrates noted that their total area is equal to the area of ​​a square, colored blue here. Indeed, the sum of the areas of the semicircles built on the sides of this square is equal to the area of ​​the circle in which the square is inscribed. If you remove the purple-colored segments from the semicircles, then you will be left with four holes; if you remove them from the large circle, then the status remains a square.

Fig. 1.
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Fig. 2.

Figure 2 illustrates another theorem of Hippocrates. It turns out that the area of ​​a trapezoid inscribed in a circle with a center at point O is equal to the sum of the areas of the orange holes and the orange semicircle (all three holes are equal in construction, the semicircle is equal to the semicircles from which the holes are formed). This theorem is proven in the same way as the previous statement.

At figure 3 there is a figure also compiled by Hippocrates. The two sides and the smaller base of the trapezoid are equal to 1, the larger base is equal to 3\sqrt{3}. The lower arc of the figure, protected on figure by black lines and which is naturally called a generalized lone arc, touches the diagonal of the trapezoid. It turns out that the area of ​​the inscribed trapezoid and the lune are equal (prove this by the areas of the lune. The proof of this fact is easy to obtain if you use the Pythagorean theorem. By the way, this figure has another amazing property. The lune has the same width. More precisely, the diameters of the circles most inscribed in them are each equal to half the difference between the sum of the legs and the hypotenuse of the triangle shown in the same figure.

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the sides of the triangle TT still serve as the metric.

Since the symmetric segments are equal in size, it is now sufficient to prove (see Fig. 6 f) that the sum of the areas of the quadrilaterals R1,R2R_1, R_2 and R3R_3 without the area of ​​the triangle LL is equal to twice the area of ​​the triangle TT.

Triangles LL and L′L' are symmetrical about side cc. Let us now reflect the triangles PP and QQ first relative to the side cc. We get triangles P′P' and Q′Q'. Then reflect triangle P′P' relative to side bb, and triangle Q′Q' relative to side aa. A figure is formed from two triangles T1T_1 and T2T_2.

Both of these triangles are symmetrical

Fig. 62.

SS′=π\frac{S}{S'} = \pi

Fig. 7

Fig. 8a, b, c.

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Physics
helps
geometry

B. Yu. Kogan

When studying physics, of course, mathematics is used. But it turns out that the other way around is also true: physics benefits mathematics. Here are some examples of how the concept of center of gravity can be used in geometry.

  1. Theorem on medians of a triangle. Let us place material points of equal mass at the vertices of the triangle (Fig. 1). The center of gravity of the system of points A and B is located at point K - the middle of the segment AB. This means that the center of gravity of the system of points A, B and C lies on the median of the SC. Reasoning in a similar way, we will come to the conclusion that this center of gravity lies on the median AL and on the median BM. But the system of points A, B and C has only one center of gravity. Therefore, the medians of a triangle intersect at one point.

Further, since point C has mass m, and point K “represents” a system of points A and B, having mass 2m, then KS is half the size of SC. Therefore, the point of intersection of the medians divides each of them in a ratio of 2:1.

  1. Theorem on the midlines of a quadrilateral. Let us place material points of the same mass (Fig. 2) at the vertices of the quadrilateral ABCD. Since the center of gravity of the system of points A

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or about points A and D, we will come to the conclusion that the center of gravity of the system of points A, B, C and D lies at the intersection of the mean lines KM and LN. Further, since the system of points A and B has the same mass as the system of points C and D, then KS = SM. Reasoning in a similar way, we find that LS=SN. Consequently, the midlines of the quadrilateral, intersecting, are divided in half.

Note that our reasoning does not use the fact that points A, B, C and D lie in the same plane. This means that the proven theorem is also true for a spatial quadrilateral. (It follows from this that the midlines of such a quadrilateral necessarily intersect.)

  1. Generalization of the previous theorem. Consider an arbitrary quadrilateral ABCD (Fig. 3). Let us place material points at its vertices: at vertex A - masses m, at vertex B - masses αm, at vertex D - masses βm and at vertex C - masses αβm, where α and β are arbitrary positive numbers. Then the center of gravity of the system of points A, B, C and D will lie at the intersection of straight lines KM and LN, where K is the center of gravity of the system of points A and B, M is the center of gravity of the system of points C and D, L is the center of gravity of the system of points B and C, and N is the center of gravity of the system of points A and D. Further, since lengthwise arbitrary correspond to weights, then

AKKB=αmm=α,DMMC=αβmβm=α,\frac{AK}{KB} = \frac{\alpha m}{m} = \alpha, \quad \frac{DM}{MC} = \frac{\alpha \beta m}{\beta m} = \alpha,

NSSL=αm+αβmm+βm=α,BLLC=αβmαm=β,\frac{NS}{SL} = \frac{\alpha m + \alpha \beta m}{m + \beta m} = \alpha, \quad \frac{BL}{LC} = \frac{\alpha \beta m}{\alpha m} = \beta,

ANND=βmm=β,\frac{AN}{ND} = \frac{\beta m}{m} = \beta,

KSSM=αβm+βmαm+m=β.\frac{KS}{SM} = \frac{\alpha \beta m + \beta m}{\alpha m + m} = \beta.

Therefore, if the sides of this quadrilateral are divided so that

AKKB=DMMC=α,BLLC=ANND=β,\frac{AK}{KB} = \frac{DM}{MC} = \alpha, \quad \frac{BL}{LC} = \frac{AN}{ND} = \beta,

then the segments NL and KM will separate in that

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For example, on figure 4 each “vertical” segment is divided into three identical sections, and each “horizontal” segment is divided into four identical sections *).

  1. Finding matches. Using the concept of the center of gravity, problems of the following type can be easily solved. On the sides of the triangle ABCABC there are points KK and LL (Fig. 5). Given that AKKB=12\frac{AK}{KB} = \frac{1}{2} and BLLC=35\frac{BL}{LC} = \frac{3}{5}, find the ratios of ASSL\frac{AS}{SL} and CSSK\frac{CS}{SK}.

Solution. Let us place material points at the vertices A,B,CA, B, C so that the correspondence holds
mBmA=ABKB=12,mCmB=BLLC=35,\frac{m_B}{m_A} = \frac{AB}{KB} = \frac{1}{2}, \quad \frac{m_C}{m_B} = \frac{BL}{LC} = \frac{3}{5},
for example, let’s put
mA=10m,mB=5m,mC=3m.m_A = 10m, \quad m_B = 5m, \quad m_C = 3m.
Then the center of gravity of the system of points AA and BB will lie at point KK, and the center of gravity of the system of points BB and CC will lie at point LL. Consequently, the center of gravity of the system of points A,BA, B and CC lies on the straight line CKCK and at the same time on the straight line ALAL, that is, it is located at the intersection point SS. From here it is easy to find that
ASSL=mB+mCmA=5m+3m10m=45,\frac{AS}{SL} = \frac{m_B + m_C}{m_A} = \frac{5m + 3m}{10m} = \frac{4}{5},
CSSK=mA+mBmC=10m+5m3m=51.\frac{CS}{SK} = \frac{m_A + m_B}{m_C} = \frac{10m + 5m}{3m} = \frac{5}{1}.
Exercise

  1. Each vertex of the tetrahedron is connected to the intersection point of the medians of the opposite face. Prove that the four resulting segments intersect at one point.
  2. In triangle ABCABC the median AKAK is drawn. The line connecting the vertex CC with the midpoint of the median intersects the side ABAB at the point LL. Find the ratio AL:LBAL:LB.
  3. In the triangle ABCABC shown at figure 6,
    AKAB=BLBC=CMCA=13.\frac{AK}{AB} = \frac{BL}{BC} = \frac{CM}{CA} = \frac{1}{3}.
    What part of the area of ​​triangle ABCABC is the sum of the areas of the protected triangles?
    *) This theorem is also true for a non-planar quadrilateral.

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Impossible objects

L. Penrose, R. Penrose

The impression of three-dimensional objects can be conveyed using flat images. This can be used to create a contradictory impression.

figure non-existent structures are described here. Each part is perceived as an image of a three-dimensional three-dimensional object, but the entire figure, due to the incorrect connection of these parts, appears to be a ghost object.

An example of such a construction is shown in figure 1. Each part is a block of rectangular cross-section, but the lines in figure are connected so that the object depicted does not exist in reality. As the eye follows the edge of the block, the apparent distance from the object to the object being observed changes.

figure 2 shows a structure, each part of which is a series of steps. However, the parts of this are connected to each other in such a way that the picture as a whole is incompatible: the steps are constantly rising.

The illusion of non-existent structures can also be caused by unknown objects. To do this, they must be designed in a special way and photographed at a certain angle. An example of such a photographer is shown in figure 3. Here the action of an existing model gives the same impression as the image of an unknown staircase (Fig. 2). This is because the rightmost step when photographing is close to the camera and higher than the step that appears to be located directly above it.

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Fig. 3. Impossible cube model.

open-loop three-dimensional model (Fig. 2). If you look at such a model with one eye and find the desired point, you can see how the two disconnected sides of the model will fit together. By photographing the model from this position, you will get a photograph of the impossible Penrose trigon.

This example is also used to obtain an image of an impossible cube. If you make a cage like the one shown in figure 3, then, positioning it so that the back edges of the cage cover the slits in the front ones, you will see an impossible cube: the back edges of the cage will seem to be pushed forward. (A photograph can also be obtained from this position.) The physiologist Gibson, using this idea, came up with a number of interesting illusions in which he used rectangular cardboard with slits in some of them, so that the most distant of the rectangular ones would appear to be located in the foreground. On figure4 the two sets of squares, although seemingly identical, are arranged differently in space, and in the third row the jack is actually close to the six, and the cards are therefore the same size. Such a photograph can be obtained by making appropriate slits in a nearby card and in the middle rectangular column, through which you can see the more distant six (Fig. 5).

Another series of the same kind of optical illusions can be obtained using the so-called artificial Ames room, the geometry of which is shown in figure 6. This room is made somewhat unusually. The floor in it is inclined and rises to the right of the observer, the rear wall moves away as one moves to the left, the windows on this wall are of different sizes and are shaped like a trapezoid. However, if you look into such a room from a certain point, it looks completely ordinary: the floor of each

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Fig. 5. A device that allowed you to observe the illusion that you see on figure 4.

square, the back wall is perpendicular to the direction of view, and the windows are rectangular and identical. Ames made one of these rooms large enough for people to stay in it. The result was an amazing effect: when the viewer looks at people walking along this room, he observes unusual changes in their sizes. Depending on where a person goes, he seems to be either growing or faltering.

A small model of such a room allows you to see a person’s hands or face through the windows of the back wall. As in a large room, hands or faces appear large or small depending on whether they appear in the windows to the right or to the left. We are so accustomed to rooms of a general shape that in the Ames room we perceive even highly distorted objects as real. Perception of an image is a psychological process. In this case, the attitude of the abuser to the subject of abuse and even his condition at the moment is important. It is interesting that familiar faces are perceived as completely normal in Ames’s room, while the geometry of the room always becomes noticeable to the observer.

Of course, building a large Ames room yourself is quite difficult. But it is apparently possible to make a small model. By placing interior items, you can get some pretty effective photos if you want. Why not try it?

Fig. 6. Geometry of the twisted Ames room.

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Tasks

M81. An arbitrary point PP is taken inside the square A1A2A3A4A_1 A_2 A_3 A_4. From vertex A1A_1 a perpendicular is dropped to line A2PA_2 P, from vertex A2A_2 - to A3PA_3 P, from A3A_3 - to A4PA_4 P, from A4A_4 - to A1PA_1 P. Prove that all four perpendiculars (or their extensions) intersect at one point.

A. N. Vilenkin

M82. There are several identical automatic vehicles on the ring road. It is known that if all the gasoline available in these automatic vehicles were poured into one, then this car would be able to drive along the entire ring road and return to its original place. Prove that at least one of the cars standing on the road can compress all the stakes, taking gasoline from the rest of the cars along the way.

M83. Prove that the numbers 1, 2, …, nn for any nn cannot be divided into two groups so that the product of numbers in one group is equal to the product of numbers in the other.

M84. Let AA be the base of the perpendicular dropped from the center of the given circle onto the given straight line ll.

On this line two more points BB and CC are taken so that

AB=AC.AB = AC.

Two arbitrary secants are drawn through the points BB and CC, one of which intersects the circle at points PP and QQ, the second - at points MM and NN. Let lines PMPM and QNQN intersect line ll at points RR and SS. Prove that

AR=AS.AR = AS.

This problem (or some of its variants) is sometimes called the “butterfly problem”; the origin of this name is clear from figure 1.

M85. Prove that if a1,a2,...,ama_1, a_2, ..., a_m are pairwise distinct natural numbers, none of which is divisible by the square of an integer greater than one, and b1,b2,...,bmb_1, b_2, ..., b_m are integers other than zero, then

b1a1+b2a2+…+bmam≠0.b_1 \sqrt{a_1} + b_2 \sqrt{a_2} + \ldots + b_m \sqrt{a_m} \neq 0.

L. N. Vaserstein

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F93. In the side wall of a vessel filled with a liquid with a refractive index nn, a hole of small radius rr continues. A horizontal thin beam of light is directed along the axis of the hole from the vessel. To what level hh above the hole must the liquid flow out so that the light ray emerges from the jet without ever experiencing internal reflection?

Neglect the change in the cross section of the jet, and assume the refractive index of the liquid to be sufficiently large.

I. F. Ginzburg

F94. A cycle is performed over one gram-molecule of an ideal gas (a closed process consisting of two isochores and two isobars (Fig. 2)). The temperatures at points 1 and 3 are T1T_1 and T3T_3, respectively. Determine the work done by the gas per cycle if it is known that points 2 and 4 lie on the same isotherm.

F95. The surface of the river forms an inclined plane. Can a body float freely along a river at a speed exceeding the speed of the current or the maximum speed of the current?

F96. Two identical balls connected by thread. Find the rise height of this system if one of the balls is thrown upward with a speed of vv.

A. Drozdov

F97. A coil of insulated wire is bent in the shape of a figure eight, the bulb of which has a radius of r1=1r_1 = 1 cm and r2=3r_2 = 3 cm. The coil is in a magnetic field with induction B=104B = 10^4 ec, perpendicular to the plane of the coil.

The wire insulation is designed for a voltage of 10 e. Will insulation breakdown occur if the magnetic field is suddenly turned off? Field switch-off time 10−310^{-3} sec.

L. G. Aslamaov

Fig. 2.

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Solutions

In this issue we publish solutions to problems M31–M33

M31

A square sheet of paper is cut straight into two parts. One of the resulting parts is again cut into two parts, and this is done many times. What is the smallest number of cuts that need to be made so that the resulting parts turn out to be exactly twenty-decagons?

With each cut, the total number of pieces of paper increases by 1 (since one piece disappears and two new ones appear), so after nn cuts there will be (n+1)(n+1) pieces of paper.

Let us now calculate what the total number of vertices in all pieces together can be after nn cuts. With each cut, the total number of vertices increases either by 2 (if you cut through the vertices), or by 3 (if you cut through the vertex and side), or by 4 (if you cut through 2 sides). Since at first there were 4 vertices, then after nn cuts there will be no more than 4n+44n+4 vertices in all pieces together.

Let’s assume that after NN cuts there are 100 dacagons. Since in this case the total number of pieces obtained will be N+1N+1, then, in addition to these decadagons, there will be another N+1−100N+1-100 pieces. Each of these pieces will have at least three vertices, so the total number of vertices in all pieces will be at least 100⋅20+(N−99)⋅3100\cdot 20+(N-99)\cdot 3. As was proven earlier, this number is no more than 4N+44N+4. Means,

4N+4≥100⋅20+(N−99)⋅3=3N+1703,4N+4 \geq 100\cdot 20+(N-99)\cdot 3 = 3N+1703,

whence N≥1699N \geq 1699.

So, we have proven that it is impossible to get 100 bidecagons by making fewer than 1699 cuts. This is the main and most difficult part of the proof.

Let us now show how you can get 100 bidecagons by making 1699 cuts. Here is one way: cut the square into 100 rectangles (99 cuts) and turn each rectangle into a 20-sided triangle in 16 cuts, cutting off triangles from the corners (1600 cuts). There will be 1699 cuts in total.

Answer. Can get 100 decanagons by making 1699 cuts, and by making fewer cuts, 100 dedecagons.

In the same way, you can find out what is the smallest number of cuts you need to make to get exactly kk l-gons.

The exact solution to this problem was sent by D. Grigoriev from Leningrad and V. Livits from Zaporozhye.

I. N. Bernistey

M32

In all cells of the table 100×100100 \times 100 is a plane. It is allowed to simultaneously change the signs in all cells of one row or one column. Is it possible, by continuing the operations several times, to obtain a table with exactly 1970 minutes?

Let us change the sign xix_i times in the iith row, and yky_k times in the kkth column. Then in the cell located at the intersection of the iith row and kkth column, the sign will change xi+ykx_i+y_k times. Consequently, this cell will contain a minutec if and only if xi+ykx_i+y_k is odd. Thus, about

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The exact number of minuses in the resulting table depends only on the parity of the numbers xix_i and yky_k; on figure 1, ​​zeros are placed together with even numbers, and ones are placed together with odd numbers. Let xx be the number of odd numbers among xix_i; yy is the number of odd numbers yky_k (on figure x=5,y=4x = 5, y = 4). Then, as is easy to calculate, the total number of minuses in the table will be equal to

x(100−y)+(100−x)y=100x+100y−2xy,x(100-y)+(100-x)y = 100x+100y-2xy,

where x,yx, y are integers.

Now let’s return to our problem and prove that the answer is negative, i.e. it is impossible to get 1970 minuses. Let’s assume that we managed to get 1970 minuses. Then 1970=100x+100y−2xy1970 = 100x+100y-2xy, from where

xy−50x−50y+2500=1515.xy - 50x - 50y + 2500 = 1515.

Factoring the left-hand side, we get

(x−50)(y−50)=1515=15⋅101.(x-50)(y-50) = 1515 = 15 \cdot 101.

We have

−50≤x−50≤50,−50≤y−50≤50.-50 \leq x-50 \leq 50, -50 \leq y-50 \leq 50.

Since 101 is a prime number, then either x−50x-50 or y−50y-50 is divisible by 101 (after all, their product is divisible by 101). But from the previous inequalities it then follows that either x−50x-50 or y−50y-50 is equal to 0. So, we have a contradiction that proves that exactly 1970 minutes of obtaining the impossible.

The correct solution was sent by D. Grigoriev.

A. V. Zelevinsky

M33

There is a natural number n>1000n > 1000. Let’s take the remainders from dividing the number 2n2^n by the numbers 1, 2, 3,…, nn and find the sum of these remainders. Prove that this sum is greater than 2n2^n.

Let us denote the sum of remainders from dividing 2n2^n by the numbers 1, 2,…, nn by SnS_n. We will succeed in the statement of the problem and prove that for n>1000n > 1000 Sn>3,5nS_n > 3,5n. Along the way, we will prove the same method as

Sn>n2(log⁡2n−4)S_n > \frac{n}{2} (\log_2 n - 4)

for any nn.

We follow mainly the decision of D. Grigoriev from Leningrad. The solution is based on a very simple consideration: 2n2^n is not divisible by an odd integer other than 1, which means that the remainder of division of 2n2^n by such a number is not less than 1. From here it is easy to deduce that for any odd k>1k > 1 the remainder of division of 2n2^n by 2lk2^l k is not less than 2l2^l. Indeed, let the remainder of the division of 2n−l2^{n-l} by kk be equal to rr, that is, 2n−l=mk+r2^{n-l} = mk + r, where 0≤r<k0 \leq r < k, then 2n=m(2lk)+2lr2^n = m(2^l k) + 2^l r, where 0≤2lr<2lk0 \leq 2^l r < 2^l k, that is, the remainder of the division of 2n2^n by 2lk2^l k is equal to 2lr2^l r, and since r≠0r \neq 0, then this remainder is not less than 2l2^l.

It follows that in any case

Sn≥1⋅(количество не превышших n чисел вида 2k+1,k>1)+2⋅(количество не превышших n чисел вида 2(2k+1),k>1)+22⋅(количество не превышших n чисел вида 22(2k+1),k>1)+…S_n \geq 1 \cdot (\text{количество не превышших } n \text{ чисел вида } 2k + 1, k > 1) + 2 \cdot (\text{количество не превышших } n \text{ чисел вида } 2(2k + 1), k > 1) + 2^2 \cdot (\text{количество не превышших } n \text{ чисел вида } 2^2(2k + 1), k > 1) + \dots

  • 2l⋅(количество не превышших чисел вида 2l(2k+1),k>1),(∗)2^l \cdot (\text{количество не превышших чисел вида } 2^l(2k + 1), k > 1), (*)

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where ll is determined by the condition 3⋅2l≤n3 \cdot 2^l \leq n, 3⋅2l+1>n3 \cdot 2^{l+1} > n (there is no point in taking more than ll, since then the expression in the bracket will be equal to zero).

What can you say about the right side of this inequality?

Let’s consider the (i+1)(i+1)-th term: 2i(…)2^i(\ldots). The number in the bracket is obviously equal to the number of non-exceeding nn terms of the arithmetic progression 3⋅2i3 \cdot 2^i, 5⋅2i5 \cdot 2^i, 7⋅2i7 \cdot 2^i, …, that is, a progression with the first term 3⋅2i3 \cdot 2^i and the difference 2⋅2i2 \cdot 2^i. The number of such terms is no less than n−3⋅2i2i+1\frac{n-3 \cdot 2^i}{2^{i+1}} and, therefore, the ii term on the right side of the inequality is no less than n2−32⋅2i\frac{n}{2} - \frac{3}{2} \cdot 2^i. Basically, the solution to the problem is over. Everything else is various transformations of the right side () using the obtained inequalities. Let us replace, for example, the sum on the right side () when washed with eight terms. Then we will get

Sn>8⋅n2−32∑i=072i>S_n > 8 \cdot \frac{n}{2} - \frac{3}{2} \sum_{i=0}^{7} 2^i >

>8⋅n2−32⋅28=3,5n+(n2−384).> 8 \cdot \frac{n}{2} - \frac{3}{2} \cdot 2^8 = 3,5n + \left(\frac{n}{2} - 384\right).

For n>1000n > 1000 the expression in the bracket is positive and, therefore, we have proven that Sn>3,5nS_n > 3,5n for n>1000n > 1000. Thus problem M33 is completely solved.

However, a more precise inequality can be obtained. Let’s sum up all the terms on the right side (*); we get:

Sn>(l+1)n2−32∑i=0l2i>S_n > (l+1) \frac{n}{2} - \frac{3}{2} \sum_{i=0}^{l} 2^i >

>(l+1)n2−3⋅2l+12.> (l+1) \frac{n}{2} - \frac{3 \cdot 2^{l+1}}{2}.

Using the inequalities 3⋅2l≤n3 \cdot 2^l \leq n, 3⋅2l+1>n3 \cdot 2^{l+1} > n, we find that

Sn>n2log⁡2n3−n=S_n > \frac{n}{2} \log_2 \frac{n}{3} - n =

=n2(log⁡2n3−2)>n2(log⁡2n−4).= \frac{n}{2} \left(\log_2 \frac{n}{3} - 2\right) > \frac{n}{2} \left(\log_2 n - 4\right).

This formula shows, for example, that if n>21004n > 2^{1004} then Sn>500nS_n > 500 n.

Task. The sum of the remainders from dividing the numbers 2l+12^{l+1}, 2l+L2^{l+L} by the odd number m>1m > 1 is greater than m2(Llog⁡22m−1)\frac{m}{2} \left(\frac{L}{\log_2 2m} - 1\right).

Using this problem, the solution of which will be given below, one can prove that for an infinite number of values ​​of nn the sum of SnS_n is actually larger than n2(log⁡2n−4)\frac{n}{2} \left(\log_2 n - 4\right), that is, one can prove that the estimate of Sn>n2(log⁡2n−4)S_n > \frac{n}{2} \left(\log_2 n - 4\right) is very larger for an infinite number of values ​​of nn. This is not surprising, since our method of proof does not take into account multi-wanted numbers other than zero, while these remainders are often large. At the same time, the value of SnS_n cannot grow too quickly with the growth of nn, since there are too many of those of Sn≤1+2+…+(n−1)=n(n−1)2S_n \leq 1 + 2 + \ldots + (n-1) = \frac{n(n-1)}{2}.

We believe that the following hypothesis is true:

Hypothesis 1. For sufficiently large nn the inequality Sn≤n24S_n \leq \frac{n^2}{4} is true;

  1. there is a positive number c>0c > 0 such that cn2≤Sncn^2 \leq S_n.

We can neither prove nor verify these statements. Moreover, we do not know whether the weaker one is fair.

Conjecture 2. There is a positive number c>0c > 0 such that the inequality cn2≤Sncn^2 \leq S_n holds for an infinite number of values ​​of nn.

If you managed to prove or test one of these hypotheses, send us your reasoning. If they turn out to be interesting, we will publish them in one of the issues of the magazine. As a weak test of Hypothesis 2, the following can be proven.

Theorem. For an infinite number of values ​​of nn the following inequality holds:

Sn>n2132log⁡2n.S_n > \frac{n^2}{132 \log_2 n}.

The theorem is derived from the problem as follows. Consider the sum Σk\Sigma_k of the remainders from dividing the numbers 2k+12^{k+1}, …, 2n2^n by the number kk. According to the problem, if kk is odd, the sum Σk\Sigma_k is residually large, therefore the number Σ1+Σ2+…+Σn\Sigma_1 + \Sigma_2 + \ldots + \Sigma_n is also large. But how easy it is for*

*) The number n2132log⁡2n\frac{n^2}{132 \log_2 n} for large nn cities is greater than the number n2(log⁡2n−4)\frac{n}{2} \left(\log_2 n - 4\right). It is not difficult to prove, for example, that for a sufficiently large nn the ratio of these numbers is greater than n\sqrt{n}.

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tag, S1+S2+⋯+Sn=Σ1+⋯+ΣnS_1 + S_2 + \dots + S_n = \Sigma_1 + \dots + \Sigma_n,
poznym, the amount worth the left side is also
is large and, therefore, one of the terms, say SlS_l, is also large. We leave the careful execution of the proof to the reader. Let us now move on to solving the problem.

Solving the problem. Let’s write down the remainders from dividing the numbers 2l+1,…,2l+L2^{l+1}, \dots, 2^l + L by mm and put a “tick” between two consecutive remainders if the first is greater than the second. Then, firstly, the remainder before the checkmark is greater than m2\frac{m}{2}, and secondly, the number of numbers between two consecutive checkmarks is less than log⁡22m\log_2 2m, since the remainders between two checkmarks form a geometric progression with value 2 (indeed, 2log⁡22m−1=m>m−12\log_2 2m - 1 = m > m - 1, and every remainder is not greater than m−1m - 1). Thus, the number of spaces between the checkmarks is greater than Llog⁡22m−1\frac{L}{\log_2 2m} - 1 and since at the end of each gap there is a number greater than m2\frac{m}{2}, then everything is proven.

A. G. Kushiirenko

In this issue we publish solutions to problems F43, F48—F51

F43

Find the pressure at the center of a liquid planet of radius RR if the liquid is incompressible and has a density ρ\rho.

Divide the volume of the planet into thin spherical elephants with thickness Δr\Delta r. It is easy to show that the equilibrium of the granitization forces acting from the side of the layer on the particle inside this layer is equal to zero. Indeed, for this purpose, consider a cone with a small angle at the apex, in which part of the mass mm is placed. The cone cuts out areas of areas s1s_1 and s2s_2 (Fig. 1) from the layer. If the mass of the substance per unit surface of the layer is equal to μ\mu, then the granitonic forces acting on the mass mm from sections s1s_1 and s2s_2 are equal

F1=γmμs1r12,F2=γmμs2r22;F_1 = \gamma \frac{m\mu s_1}{r_1^2}, \quad F_2 = \gamma \frac{m\mu s_2}{r_2^2};

But

s1r12cos⁡α1=s2r22cos⁡α2=Ω\frac{s_1}{r_1^2} \cos \alpha_1 = \frac{s_2}{r_2^2} \cos \alpha_2 = \Omega

(Ω is the solid angle at the vertex of the cone), and α1=α2\alpha_1 = \alpha_2; protected triangles are similar, that is, ∠OA1M1=∠OA2M2,∠OA1B1=∠OA2B2\angle OA_1 M_1 = \angle OA_2 M_2, \angle OA_1 B_1 = \angle OA_2 B_2 (they rest on the same arc) and α1=∠OA1B1−∠OA1M1aα2=∠OA2B2−∠OA2M2\alpha_1 = \angle OA_1 B_1 - \angle OA_1 M_1 a\alpha_2 = \angle OA_2 B_2 - \angle OA_2 M_2.

Pozny s1r12=s2r22\frac{s_1}{r_1^2} = \frac{s_2}{r_2^2}. Thanks to this

F1=F2,F_1 = F_2, that is, these forces mutually balance each other. Carrying out a similar consideration for other parts of the layer, we will prove the statement made.

The force with which the layer element ΔsΔr\Delta s\Delta r bends to the center of the planet is equal to

F=γ43πr3ρΔsΔrρF = \gamma \frac{4}{3} \pi r^3 \rho \Delta s \Delta r\rho,

where rr is the distance from this element to the center of the planet. From here we find that the increase in pressure in a section of thickness Δs\Delta s is equal to

Δp=FΔs=43πγρ2rΔr.\Delta p = \frac{F}{\Delta s} = \frac{4}{3} \pi \gamma \rho^2 r \Delta r.

Posny pressure at a distance r0r_0 from the center of the planet will be equal to

p=p0+43πγρ2ΣrΔr.p = p_0 + \frac{4}{3} \pi \gamma \rho^2 \Sigma r \Delta r.

Since the sum rΔrr\Delta r is equal to the area

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The figure bounded by the graph y=ry=r and the axis rr (Fig. 2), then

∑rΔr=(R+r0)(R−r0)2=R2−r022.\sum r \Delta r = \frac{(R+r_0)(R-r_0)}{2} = \frac{R^2-r_0^2}{2}.

Because

p=p0+23πρ2(R2−r02);p = p_0 + \frac{2}{3} \pi \rho^2 (R^2-r_0^2);

p0p_0 is the pressure on the surface of the planet, which can be taken equal to zero. Then

p=23πρ2(R2−r02).p = \frac{2}{3} \pi \rho^2 (R^2-r_0^2).

At the center of the planet (r0=0r_0=0) the pressure will be equal to

pμ=23πρ2R2.p_\mu = \frac{2}{3} \pi \rho^2 R^2.

F48

A rope is wound around the armature shaft of the dynamo, to which a weight is attached. As the weight descends, it rotates the anchor. When the armature was sufficiently untwisted, a load resistance was attached to the adhesives of the dynamo. Draw on a graph the dependence of the speed of rotation of the anchor on the time from the moment the load begins to move.

Since before the load is connected, the moment of external forces acting on the armature is constant, the armature rotates with constant angular acceleration and its speed increases in proportion to time.

After connecting the load, current will flow through the armature winding. Due to this, a moment of force will act on the armature in the magnetic field of the stator, proportional (like the force acting on a conductor with current in a magnetic field) to the magnitude of the current. This moment of force slows down the rotation of the armature. Since the current flowing through the armature winding is proportional to the em.d.c. induction occurring in the winding, and ed.d.c. induction, in turn, is proportional to the rate of change of the magnetic flux propagating the winding, that is, the angular speed of rotation of the armature, then at a certain angular speed ω0\omega_0 the moment of force acting on the armature from the side of the load will be equal to the moment of the braking force acting on the armature in the magnetic field. ω0\omega_0 is the speed of steady rotation of the armature.

The graph of the dependence of the armature rotation speed on time is shown in Fig. 4. The cool line is for the case when the armature rotation speed at the moment the load was connected was less than ω0\omega_0, and the blue line—when it was more than ω0\omega_0.

F49

The U-shaped tube is filled with water (Fig. 4). Air has been removed from one elbow; the air pressure in the other leg at temperature T0=20∘CT_0=20^\circ C is equal to atmospheric pressure. Both ends of the tube are full. What will be the difference in water levels in the elbows if the tube is heated to T=100∘CT=100^\circ C?

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Fig. 4.

The pressure in the left knee is equal to the saturated vapor pressure. The right elbow contains both air and water vapor, and the pressure is equal to the sum of the partial pressures of air and steam. Moreover, the steam in the right vessel is also saturated, and its partial pressure is equal to the steam pressure in the left knee. Therefore, when considering the equilibrium of water, we can not take into account the vapor pressure in the left and right elbows.

Let us write down the equilibrium condition for water in the tube at T0=20∘CT_0=20^\circ\text{C}:

ρgh0=P0,P0=1 amm.\rho gh_0 = P_0, \quad P_0 = 1 \text{ amm.}

From here

h0=P0ρg≈10 m.h_0 = \frac{P_0}{\rho g} \approx 10 \text{ m.}

At 100∘C100^\circ\text{C}, the air pressure in the right knee becomes PP, and the difference in water levels in the knees becomes hh. At the same time

ρgh=P.(∗)\rho gh = P. \quad (*)

PP is related to P0P_0 by the combined gas law:

P0V0T0=PVT,\frac{P_0 V_0}{T_0} = \frac{PV}{T},

and l−l0=12(h−h0)l - l_0 = \frac{1}{2} (h - h_0). Since V0=l0sV_0 = l_0 s, V=lsV = ls (s is the cross-sectional area of ​​the tube), then from here we find

P=P0TT0l0l=P = P_0 \frac{T}{T_0} \frac{l_0}{l} =

=P0TT0l0l0+12(h−h0).= P_0 \frac{T}{T_0} \frac{l_0}{l_0 + \frac{1}{2} (h - h_0)}.

Substituting this expression into equation (*), we get

h=P0ρgTT0−l0l0+12Δh,h = \frac{P_0}{\rho g} \frac{T}{T_0} - \frac{l_0}{l_0 + \frac{1}{2} \Delta h},

or

h=h0TT0l0l0+12Δh.h = h_0 \frac{T}{T_0} \frac{l_0}{l_0 + \frac{1}{2} \Delta h}.

Assuming that 1/2Δh≪l01/2 \Delta h \ll l_0, we get

h=h0TT0≈13 m;h = h_0 \frac{T}{T_0} \approx 13 \text{ m};

Δh≈3 m,12Δh≈1,5 m≪l0=15 m\Delta h \approx 3 \text{ m}, \frac{1}{2} \Delta h \approx 1,5 \text{ m} \ll l_0 = 15 \text{ m}. This means that, comparing 1/2Δh1/2 \Delta h with l0l_0, we got a result that is not very different from the exact one.

F50

On a smooth horizontal table lie two identical cubes with masses mm, connected by a spring of stiffness kk and length l0l_0 into a non-growth system. A force FF, constant in magnitude and direction, will begin to act on the left cube (Fig. 5). Find the minimum and maximum distance between the cups as the system moves further.

Let the distance ll between the cups be minimum or maximum (we will say “extreme”). Then both cubes move with the same speed vv, and the kinetic energy of the system is 2mv22=mv22 \frac{mv^2}{2} = mv^2. At the same time

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Time, the potential energy of the system is equal to the potential energy of the sloped spring, that is, kx2/2kx^2/2, where xx is the change in the length of the spring (xx can be either positive - then the length of the spring l=l0−xl = l_0 - x is less than l0l_0, or negative - then the length of the spring is greater than l0l_0). The total energy of the system is equal to the sum of the kinetic and potential energy, that is, mv2+kx2/2mv^2 + kx^2/2. Since the system acquired this energy thanks to the force FF, we can write that

FL=mv2+kx22.FL = mv^2 + \frac{kx^2}{2}.

(*)

LL is the distance traveled by the left cube at the moment when the length of the spring became extreme (Fig. 6): L=S+l02−(l0−x)2=S+x2L = S + \frac{l_0}{2} - \frac{(l_0 - x)}{2} = S + \frac{x}{2} (SS is the distance traveled by the center of mass of the system).

The speed of the vv cups is equal to the speed of the center of mass of the system. A constant external force acts on the system, and it moves with uniform acceleration a=F/2ma = F/2m. Therefore, if we denote by tt the time from now

Fig. 7.

movement began until the moment when the length of the spring became equal to LL, then v=atv = at and L=at22+x2L = \frac{at^2}{2} + \frac{x}{2}. Substituting these expressions for vv and LL into equation (*), we obtain

F(at22+x2)=ma2t2+kx22.F \left( \frac{at^2}{2} + \frac{x}{2} \right) = ma^2 t^2 + \frac{kx^2}{2}.

Hence F2t24m+x2F=F2t24m+kx22\frac{F^2 t^2}{4m} + \frac{x}{2} F = \frac{F^2 t^2}{4m} + \frac{kx^2}{2} or Fx=kx2Fx = kx^2. Therefore, x1=0x_1 = 0, x2=F/kx_2 = F/k.

Thus, the minimum distance between a group is lmin⁡=l0−x2=l0−Fkl_{\min} = l_0 - x_2 = l_0 - \frac{F}{k}, and the maximum is lmax⁡=l0−x1=l0l_{\max} = l_0 - x_1 = l_0.

F51

Photographing a tiger from a distance of 20 meters is dangerous. What size should a 1mm pinhole camera be to make the tiger in the photo look striped? The distance between the stripes on a tiger’s skin is 20 cm.

A camera obscura is a box of responsibility. The photographic film placed in the camera receives a wide beam of rays from every point of the photographed object (Fig. 7). In order for a tiger to appear striped in a photograph, it is necessary that the areas on which the rays falling from the nearest points of neighboring stripes on the tiger’s pelt fall do not intersect. To do this, it is necessary that the film be located at a distance xx from the answer, more than d/tgαd/tg\alpha.

Because

tgα=l/2L+x,tg\alpha = \frac{l/2}{L + x}, then x>2d(L+x)lx > \frac{2d(L + x)}{l}.

Hence x>2dLl(1−2dl)x > \frac{2dL}{l\left(1 - \frac{2d}{l}\right)}. 2dl≪1\frac{2d}{l} \ll 1, therefore, neglecting 2d/l2d/l compared to 1 in the denominator of the formula, we get x>2dLl=20x > \frac{2dL}{l} = 20 cm. The chamber size must be greater than 20 cm.

I. Sh. Slovodechkiy

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In one of the squares in Krasnodar there is a round flower bed located in the center of the square square ABCD (Fig. 1). Two friends - Vasya and Petya - go to school right through this square. Moreover, sometimes they choose the AMC path (red line), on other days - the ADC path (blue line). Still, it is true that the first path is shorter. Petya believes that the second path is shorter, and here’s why: the circle they have to go around has a rather large radius. “Of course,” says Petya, “if the radius of the circle were not large or if there were no flower beds at all, then the path along the diagonal AC would be clearly shorter than the broken line ADC (Fig. 2). But the size of the circle is considerable, and if we assume that the circle were inscribed in a square, then, Petya argues, we would have a picture like the one in figure 3.” Now Vasya is convinced that the blue line is shorter than the red one: along the “blue” road you have to go “straight” all the time, making only one turn, while along the “red” road you have to make several turns, and sometimes it even seems to go back.

Two friends decided to dispel their doubts in this way: from point A they took different paths: Vasya through the park on the red line, Petya - around the blue line. They approached point C almost simultaneously. The dispute remained unresolved. Then they went back (each their own way) to point A. Now Petya arrived before Vasya. And the dispute was finally resolved by Petya’s crawl. True, it seemed to Vasya that Petya was faster than Vasya.

At home, Vasya decided to do mathematical calculations, denoting the radius of the circle by R, and the side of the square by a.

“It’s strange,” thought Vasya, “the answer to the question of the problem does not depend on the size of the radius of the circle.” However,” he continued his thought, “it was possible to do without calculations: after all, every boundary line, as is known, is longer than any boundary line that has the same ends.

What calculations did Vasya perform and what result did he get when using SEL?

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WHAT DO WE LOSE OR FIND HERE?

V. A. Petrov

Almost every written exam paper in mathematics includes some kind of equation. When solving it, the examinee must not only accurately check the calculations necessary to obtain the answer, but also be required to make sure that these calculations are correct. You need to be able to analyze each of the proposed transformations: does it lead to an equivalent equation, does it threaten the loss or acquisition of a solution.

Issues of tactics of “fighting” with built roots and with the loss of roots were considered in the article by A. G. Mordkovich “Someone loses, someone finds” («Kvant» No. 5, 1970) *). Now we invite you to check whether you are confident enough in this tactic. First, solutions to the equations are given. You need to analyze these decisions and answer the following question. Is the answer correct? If not, then what is here - are the roots lost or the structure found? Why? What is the correct answer? Compare your thoughts with ours on page 62.

  1. 2sin⁡4x=2(1−cos⁡4x)2\sin 4x = \sqrt{2(1 - \cos 4x)}.

Solution. Using the formula
2sin⁡2α=1−cos⁡2α,2\sin^2\alpha = 1 - \cos 2\alpha,
we get
2sin⁡4x=4sin⁡22x2\sin 4x = \sqrt{4\sin^2 2x}
or
sin⁡4x=sin⁡2x,\sin 4x = \sin 2x,
which is already very easy to solve.

Answer: x=nπx = n\pi and x=π6+nπ3x = \frac{\pi}{6} + n\frac{\pi}{3}, where n=0,±1,±2,…n = 0, \pm 1, \pm 2, \dots

*) This “tactics” is covered in more detail in the book by G.V. Dorofeev, M.K. Potanov, N.H. Rozov, very useful for applicants, “Mathematics Manual for Those Building Universities”, M., “Nauka”, 1970.

  1. 8cos⁡xcos⁡2xcos⁡4x=18\cos x\cos 2x\cos 4x = 1.

Solution. Multiplying both sides of the equation by sin xx and using the double angle sine formula three times, we get the simple equation
sin⁡8x=sin⁡x.\sin 8x = \sin x.
Answer: x=(2n+1)π9x = (2n + 1)\frac{\pi}{9} and x=2nπ7x = 2n\frac{\pi}{7}, where nn is any integer.

  1. sin⁡(15arccos⁡x)=1\sin \left(\frac{1}{5}\arccos x\right) = 1.

Solution. From this equation we find
arccos⁡x=5π2+10nπ\arccos x = \frac{5\pi}{2} + 10n\pi
(n=0,±1,±2,…n = 0, \pm 1, \pm 2, \dots).

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From here, by the definition of arccos xx, we obtain x=cos⁡(5π2+10nπ)=0x = \cos \left( \frac{5\pi}{2} + 10n\pi \right) = 0.

Answer: x=0x = 0.

  1. log⁡x−1(x2−5x+7)=1\log_{x-1} (x^2 - 5x + 7) = 1.

Solution. Let’s find the ODZ:

x2−5x+7>0,x−1>0,x^2 - 5x + 7 > 0, \quad x - 1 > 0,

whence x>1x > 1. According to the definition of a logarithmic function, we have x2−5x+7=x−1;x1=2,x2=4x^2 - 5x + 7 = x - 1; \quad x_1 = 2, \quad x_2 = 4.

Since both values ​​are included in the ODZ, they are solutions to the original equation.

  1. 2x−13+x−13=1\sqrt[3]{2x - 1} + \sqrt[3]{x - 1} = 1.

Solution. Let’s cube both sides of the equation:

3x−2+3(2x−1)(x−1)3×(2x−13+x−13)=1.3x - 2 + 3\sqrt[3]{(2x - 1)(x - 1)} \times (\sqrt[3]{2x - 1} + \sqrt[3]{x - 1}) = 1.

The expression in parentheses represents the left side of the original equation - it can be replaced with the right side. After this, the equation is reduced to the form

(2x−1)(x−1)=(1−x)3.(2x - 1) (x - 1) = (1 - x)^3.

Answer: x1=0,x2=1x_1 = 0, \quad x_2 = 1.

  1. Can the equation

x+ax+b+x=c\sqrt{x + a\sqrt{x + b}} + \sqrt{x} = c

have infinitely many solutions?

Solution. Move x\sqrt{x} to the right and square both sides:

x+ax+b=c2−2cx+x.x + a\sqrt{x + b} = c^2 - 2c\sqrt{x} + x.

After bringing similar terms we get: (a+2c)x=c2−b(a + 2c)\sqrt{x} = c^2 - b. For a+2c=0a + 2c = 0 and c2−b=0c^2 - b = 0 (and only in this case), the equation becomes an identity that is valid for all non-negative xx.

Answer: The equation has infinitely many solutions at a=−2ca = -2c and b=c2b = c^2. The solutions in this case are x≥0x \ge 0.

  1. cos⁡x2x2+(7−π)x−7π=1.\cos \frac{x}{2} \sqrt{x^2 + (7-\pi)x - 7\pi} = 1.

Solution. If, when raised to the power of some positive

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Entrance written exam in mathematics at the Faculty of Computational Mathematics and Cybernetics of Moscow State University in 1970

Sh. A. Alimov, F. P. Vasiliev, V. P. Modenov

In the last two decades, the importance of mathematical sciences in the general system of human knowledge has increased immeasurably. The main reason for this is the development of computational mathematics. The creation of electronic computers resulted in a real revolution not only in computing capabilities and methods, but also in the very nature of the application of mathematics. It became clear that the quality and quantity of mathematical machines, their application and management systems are an integral part that determines the scientific and technical level of the country.

In this regard, the need arose to train mathematicians of a new specialization. In 1970, a new faculty was opened at the M.V. Lomonosov Moscow State University - the Faculty of Computational Mathematics and Cybernetics. In the same year, the first admission to this faculty was made.

At the written exam in mathematics, each applicant was given a variant of five problems, the solution of which was given 4 hours. To obtain a satisfactory grade, more than two problems had to be solved. An excellent mark was given for correctly solving all five problems.

As an example, let’s look at a typical version made up of tasks offered in a written exam.

Option 0

  1. Determine all real values ​​of aa, for each of which the equation cos⁡4x−(a−2)cos⁡2x−3(a+1)=0\cos^4 x - (a-2)\cos^2 x - 3(a+1) = 0
    have a solution, and find all these solutions.

  2. Solve the equation
    ∣1+log⁡13x∣=3+∣2−log⁡13x∣.\left| 1 + \log \frac{1}{3} x \right| = 3 + \left| 2 - \log \frac{1}{3} x \right|.

  3. From the city AA to the city BB, located at a distance of 240 km from AA, an autorus leaves at a speed of 40 km/h. At the same time, from BB to AA at a constant speed of vv km/h, the automaton exits. Half an hour after the car meets, before reaching the city AA, it turns back and at the same speed towards BB. Determine all the values ​​of vv at which autoroms come to BB more equally than autorus.

  4. In triangle ABCABC, the length of side BCBC is equal to the arithmetic mean of the lengths of sides ABAB and ACAC. Angle AA is equal to α\alpha. Find the angles BB and CC, assuming that B≥CB \geq C. Investigate at what values ​​of the angle α\alpha the problem has a solution.

  5. In a right circular cone with vertex SS, the angle between the height SOSO and the generator is equal to φ. On the base plane outside the cone, two points AA and BB are chosen so that the lines SASA and SBSB are mutually perpendicular and form angles with a height SOSO corresponding to α\alpha and β\beta. Calculate the angle between the generators along which the lateral surface of the cone intersects the triangles OSAOSA and OSBOSB.

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Analysis of problems

  1. Note that 0≤cos⁡2x≤10 \leq \cos^2 x \leq 1 for all xx. Then, using the substitution cos⁡2x=t\cos^2 x = t, the equation is reduced to the system:

{t2−(a−2)t−3(a+1)=0,0≤t≤1,\begin{cases} t^2 - (a - 2)t - 3(a + 1) = 0, \\ 0 \leq t \leq 1, \end{cases}

which has the solution t=a+1t = a + 1 at −1≤a≤0-1 \leq a \leq 0. Hence,

cos⁡2x=a+1,\cos^2 x = a + 1,

where −1≤a≤0-1 \leq a \leq 0. From here

x=±arccos⁡a+1+πnx = \pm \arccos \sqrt{a + 1} + \pi n

(n=0,±1,±2,… ;−1≤a≤0n = 0, \pm 1, \pm 2, \dots; -1 \leq a \leq 0).

Most of those who applied coped with this task. Some of the applicants incorrectly solved equation (1), mistakenly believing that arccos⁡(−a+1)=arccos⁡a+1\arccos (-\sqrt{a + 1}) = \arccos \sqrt{a + 1}, and lost the solution corresponding to equation cos⁡x=−a+1\cos x = -\sqrt{a + 1}. Some applicants did not indicate all values ​​of aa for which a solution to the problem exists.

  1. Range of acceptable values ​​of the unknown: x>0x > 0. Let’s rewrite the equation in the form

∣1+t∣=3+∣2−t∣,|1 + t| = 3 + |2 - t|,

where t=log⁡13xt = \log \frac{1}{3} x. Sequentially spaced intervals t≤−1,−1<t<2,t≥2t \leq -1, -1 < t < 2, t \geq 2. For t≥2t \geq 2 we have 1+t=3+t−2,1 + t = 3 + t - 2,

that is, equation (1) is then satisfied effectively for all t≥2t \geq 2. Next, we verify that equation (1) for t≤−1t \leq -1 and −1<t<2-1 < t < 2 has no solution. Thus, equation (1) is all t≥2t \geq 2. Hence log⁡13x≥2\log \frac{1}{3} x \geq 2, and taking into account the domain of definition of finding

0<x≤1/9.0 < x \leq 1/9.

Some applicants, noticing the same equation (2), wrote that the equation is then validly satisfied for all tt, without taking into account the constraint t≥2t \geq 2.

  1. Let t(u)t(u) be the time of movement of the automaton before the first meeting with the automaton. Since the automaton and the automaton left at the same time, the equality is true

40t+vt=240.40t + vt = 240.

(1)

The car surfaces through t+12(u)t + \frac{1}{2}(u) after leaving the city BB and therefore returned to BB through 2t+1(u)2t + 1(u). After the first meeting, the bus traveled vt(κm)vt(\kappa m), spending vt40(u)\frac{vt}{40}(u) on this journey. Thus, the Bus needed t+vt40(u)t + \frac{vt}{40}(u) for the entire journey from AA to BB. In order for the car to arrive at BB earlier than the bus, the inequality

2t+1<t+vt40.2t + 1 < t + \frac{vt}{40}.

(2)

According to the conditions of the surface automaton, before reaching the city AA. Since at the moment of the first meeting he is at a distance of 40t(κm)40t(\kappa m) from AA and during the receiving path v2\frac{v}{2}, then this condition comes to the inequality

v2<40t.\frac{v}{2} < 40t.

(3)

Combining (1), (2) and (3), we arrive at the system:

{40t+vt=240,2t+1<t+vt40,v2<40t.\begin{cases} 40t + vt = 240, \\ 2t + 1 < t + \frac{vt}{40}, \\ \frac{v}{2} < 40t. \end{cases}

From equation (1) we find t=240v+40t = \frac{240}{v + 40} and substitute it into inequalities (2) and (3). By jointly solving the resulting inequalities for vv, we find 56<v<12056 < v < 120.

Most applicants were able to complete equation (1) and inequality (2), although some of them replaced the < sign in (2)

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to the ≤ sign. The main share of errors was caused by conditions (3), since many applicants did not understand the need for this requirement and limited themselves to only solving the system obtained from (1) and (2).

  1. According to the condition

BC=AB+AC2.BC = \frac{AB + AC}{2}.

(1)

Using the sine theorem we find

AB=BCsin⁡Csin⁡α,AC=BCsin⁡Bsin⁡αAB = BC \frac{\sin C}{\sin \alpha}, \quad AC = BC \frac{\sin B}{\sin \alpha}

and substitute it into (1). We get

sin⁡B+sin⁡C=2sin⁡α,\sin B + \sin C = 2 \sin \alpha,

sin⁡B+C2cos⁡B−C2=sin⁡α.\sin \frac{B + C}{2} \cos \frac{B - C}{2} = \sin \alpha.

Because

B+C=π−α,B + C = \pi - \alpha,

(2)

then sin⁡B+C2=cos⁡α2,\sin \frac{B + C}{2} = \cos \frac{\alpha}{2}, and

cos⁡B−C2=2sin⁡α2.\cos \frac{B - C}{2} = 2 \sin \frac{\alpha}{2}.

(3)

Since by condition B≥CB \geq C and, in addition, 0<C<π,0<B<π0 < C < \pi, 0 < B < \pi, then

0≤B−C<π.0 \leq B - C < \pi.

(4)

Noting that sin⁡α2>0\sin \frac{\alpha}{2} > 0, from conditions (2), (3), (4) for determining BB and CC we have the system:

{B−C=2arccos⁡(2sin⁡α2),B+C=π−α.\begin{cases} B - C = 2 \arccos \left(2 \sin \frac{\alpha}{2}\right), \\ B + C = \pi - \alpha. \end{cases}

(5)

From (5) there is

{B=π−α2+arccos⁡(2sin⁡α2),C=π−α2−arccos⁡(2sin⁡α2).\begin{cases} B = \frac{\pi - \alpha}{2} + \arccos \left(2 \sin \frac{\alpha}{2}\right), \\ C = \frac{\pi - \alpha}{2} - \arccos \left(2 \sin \frac{\alpha}{2}\right). \end{cases}

Thus, for all values ​​of α\alpha for which there is a triangle ABCABC that satisfies all the conditions of the problem, the values ​​of the angles BB and CC are obtained from formulas (6).

Let us investigate at what values ​​of α\alpha the problem has a solution. From (6) it necessarily follows

∣2sin⁡α2∣≤1.\left| 2 \sin \frac{\alpha}{2} \right| \leq 1.

Since 0<α<π0 < \alpha < \pi, then hence 0<sin⁡α2≤120 < \sin \frac{\alpha}{2} \leq \frac{1}{2} and, therefore, 0<α≤π30 < \alpha \leq \frac{\pi}{3}.

For the found values ​​of α\alpha, the values ​​A=α,BA = \alpha, B and CC, determined by formulas (6), are positive and in total equal to π\pi. To prove this, it is enough to check conditions C>0C > 0 or 0<α≤π30 < \alpha \leq \frac{\pi}{3} and, as follows from (6), B≥C,α+B+C=πB \geq C, \alpha + B + C = \pi.

Let us show that C>0C > 0 or, according to (5),

π−α2>arccos⁡(2sin⁡α2).\frac{\pi - \alpha}{2} > \arccos \left(2 \sin \frac{\alpha}{2}\right).

(7)

Since cos xx monotonically kills on the segment 0≤x≤π0 \leq x \leq \pi, and the quantities π−α2\frac{\pi - \alpha}{2} and arccos (2sin⁡α2)\left(2 \sin \frac{\alpha}{2}\right) belong to this segment, then, calculating the cosine of both sides of inequality (7), we have cos⁡π−α2=sin⁡α2<2sin⁡α2.\cos \frac{\pi - \alpha}{2} = \sin \frac{\alpha}{2} < 2 \sin \frac{\alpha}{2}.

For 0<α<π30 < \alpha < \frac{\pi}{3} this inequality is true.

Repeating our reasoning in reverse order, we are convinced of the validity of the inequality C>0C > 0.

Thus, a triangle ABCABC with angles A=α,B≥CA = \alpha, B \geq C and satisfying the conditions of the problem, the values ​​of angles BB and CC are given by formulas (6), 0<α≤π30 < \alpha \leq \frac{\pi}{3}.

Many applicants, having received a system for determining BB and CC, were unable to solve it, and some wrote the answer in the form (6), but did not investigate at what values ​​of α\alpha the problem has a solution. Some applicants indicated only the case of an equilateral triangle

α=B=C=π3.\alpha = B = C = \frac{\pi}{3}.

  1. Let xx be the exclusive angle between the generators SA1SA_1 and SB1SB_1 along which the lateral surface of the cone intersects the triangles OSAOSA and OSBOSB (see Fig.ok): ⇒ASB=π2,⇒OSA=α,\Rightarrow ASB = \frac{\pi}{2}, \Rightarrow OSA = \alpha,

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Few applicants managed this task.

Note that formulas (1) and (2) express the relationships between the internal two-faceted angle and the flat angles at the vertex of the trihedral angle. In the general case, if A,BA, B and CC are interior two angles, the opposite of the corresponding plane angles α\alpha, β\beta and γ\gamma of a trihedral angle, then the valid formulas are:

cos⁡A=cos⁡α−cos⁡βcos⁡γsin⁡βsin⁡γ,\cos A = \frac{\cos \alpha - \cos \beta \cos \gamma}{\sin \beta \sin \gamma},

cos⁡B=cos⁡β−cos⁡αcos⁡γsin⁡αsin⁡γ,\cos B = \frac{\cos \beta - \cos \alpha \cos \gamma}{\sin \alpha \sin \gamma},

cos⁡C=cos⁡γ−cos⁡αcos⁡βsin⁡αsin⁡β,\cos C = \frac{\cos \gamma - \cos \alpha \cos \beta}{\sin \alpha \sin \beta},

which are derived in the same way as formula (1). These formulas can be useful in solving many stereometric problems.

In conclusion, we suggest that you independently solve the following option offered in the written exam.

Option 1

  1. Determine all real values ​​of aa for each of which the equation cos⁡4x−(a+2)cos⁡2x−(a+3)=0\cos^4 x - (a+2)\cos^2 x - (a+3)=0 has a solution, and find all these solutions.

  2. Solve the equation

∣1−log⁡1x∣+2=∣3−log⁡1x∣.|1 - \log_1 x| + 2 = |3 - \log_1 x|.

  1. From the city AA to the city BB, located at a distance of 105 km from AA, an autorus leaves at a constant speed vv km/h. 30 minutes later, following him out of AA at a speed of 40 km/h, a car leaves, which, having caught up with the bus on the way, turns back and moves at the same speed. Determine all values ​​of vv at which the car returns to AA later than the car arrives to BB.

  2. In triangle ABCABC, side BCBC serves as the base of a semicircle whose area is equal to the area of ​​triangle ABCABC. Angle AA is equal to α\alpha. Find the angles BB and CC, assuming that B≥CB \geq C. Investigate at what values ​​of the angle α\alpha the problem has a solution.

  3. In a right circular cone with vertex SS, the angle between generators SASA and SBSB is equal to α\alpha, and the angle between their projections onto the plane of the base is equal to β\beta. Calculate the angle between the bissertrices of angles OSAOSA and OSBOSB, where point OO is the center of the circle that served as the base of the cone.

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ENTRANCE WRITTEN EXAM IN MATHEMATICS AT MIPT IN 1970

A. P. Savin, B. V. Fedosov

The problems offered at the entrance exam in mathematics at the Moscow Institute of Physics and Technology have always attracted the attention of teachers and school graduates, since the level of these problems is somewhat higher than in many technical universities.

In 1970, the composition of the tasks on the written exam at MIPT changed somewhat. Instead of the four problems usually offered, in 1970 the LET contained five problems (one easy problem was added). This set of tasks apparently continued in the future.

You can get acquainted with the problems of the MIPT entrance exams of previous years in the collection “Problems in Elementary Mathematics”*), which has already been published in several editions.

I would like to note that the difficulty of the entrance exam in mathematics at MIPT is often exaggerated. The fact that after all the exams in mathematics and physics (oral and written) there is still a competition of several people per place speaks for itself.

So that we can get a real idea of ​​the written exam in mathematics in 1970, we will analyze one of the options in detail.

Option 0

  1. A subway passenger goes down a moving escalator in 24 seconds. If a passenger walks at the same speed, but on a stationary escalator, then he descends in 42 seconds. How many seconds will it take him to descend while standing on the step of a moving escalator?

  2. Solve the equation
    tg 5x—2 tg 3x=tg 5x·tg² 3x.

  3. In triangle ABC the altitudes AD and CE are drawn. Find AC if BC=a, AB=b and DE/AC=k.

  4. In a regular tetradir ABCD, two sections are drawn, each of which is parallel to the edge AB and CD. Area of ​​part of face ABC enclosed between secants

planes, s cm² greater than the area of ​​the part of the ACD face enclosed between the same planes. How much is the area of ​​one section greater than the area of ​​the other?

  1. Find real solutions to the system of equations:

{4xy+y2+2z2=−3,4xz+x2+2z2=1,8yz+y2+2z2=1.\begin{cases} 4xy + y^2 + 2z^2 = -3, \\ 4xz + x^2 + 2z^2 = 1, \\ 8yz + y^2 + 2z^2 = 1. \end{cases}

Analysis of problems

  1. Let us denote by v1v_1 the speed of the escalator, LL its length and v2v_2 the speed of the passenger. Then the conditions of the problem will be written in the form of equations:

Lv1+v2=24,\frac{L}{v_1 + v_2} = 24,

Lv2=42.\frac{L}{v_2} = 42.

Let’s transform these equations:

v1L+v2L=124,v2L=142.\frac{v_1}{L} + \frac{v_2}{L} = \frac{1}{24}, \quad \frac{v_2}{L} = \frac{1}{42}.

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From the last two equations we immediately find that

v1L=156,\frac{v_1}{L} = \frac{1}{56},

and the required time is Lv1\frac{L}{v_1}, that is, 56 seconds.

The “highlight” of the problem is that from system D to equations (1) and (2) with three unknowns, you only need to find the ratio of two unknowns LL and v1v_1. Those applicants who tried to find LL, and v1v_1, and v2v_2, naturally, could not do this.

  1. Let’s transform this equation:

tg5x−tg3x=tg3x(1+tg3xtg5x),tg 5x - tg 3x = tg 3x (1 + tg 3x tg 5x),

(1)

tg5x−tg3x1+tg3x⋅tg5x=tg3x.\frac{tg 5x - tg 3x}{1 + tg 3x \cdot tg 5x} = tg 3x.

In the last transformation we divided both sides of equation (1) by 1+tg3x⋅tg5x1 + tg 3x \cdot tg 5x. In this case, we can lose the roots of equation (1), which are the roots of equation 1+tg3xtg5x=01 + tg 3x tg 5x = 0. Transforming the original equation further, we get

tg2x=tg3x,tg 2x = tg 3x,

where

3x=2x+kπ(k=0,±1,±2,…)3x = 2x + k\pi \quad (k = 0, \pm 1, \pm 2, \ldots)

or

x=kπ(k=0,±1,±2,…).x = k\pi \quad (k = 0, \pm 1, \pm 2, \ldots).

Let’s check whether we lost any roots when dividing equation (1) by 1+tg3x⋅tg5x1 + tg 3x \cdot tg 5x. Let x1x_1 be the root of the equation

1+tg3x⋅tg5x=0.1 + tg 3x \cdot tg 5x = 0.

Then, substituting tg5x1=−1tg3x1tg 5x_1 = -\frac{1}{tg 3x_1} into the original equation, we obtain

−1tg3x1−tg3x1=0-\frac{1}{tg 3x_1} - tg 3x_1 = 0

or

tg23x1=−1tg^2 3x_1 = -1, which is impossible. Therefore, no roots were lost.

Answer:

x=kπ(k=0,±1,±2,…).x = k\pi \quad (k = 0, \pm 1, \pm 2, \ldots).

Fig. 1. BC=a,BA=b,DEAC=kBC = a, BA = b, \frac{DE}{AC} = k.

Those applicants who tried to express tg3xtg 3x and tg5xtg 5x through tgxtg x and solve the resulting equation for tgxtg x, rarely succeeded due to the cumbersome calculations and the complexity of the resulting equation.

  1. Let us denote △ABC\triangle ABC by α\alpha, then from the right triangle ABDABD (Fig. 1)

BD=ABcos⁡α=bcos⁡α,BD = AB \cos \alpha = b \cos \alpha,

and from right triangle BECBEC

BE=BCcos⁡α=acos⁡α.BE = BC \cos \alpha = a \cos \alpha.

From the triangle BDEBDE using the cosine theorem we find the length of the segment EDED:

ED2=a2cos⁡2α+b2cos⁡2α−2abcos⁡3α.ED^2 = a^2 \cos^2 \alpha + b^2 \cos^2 \alpha - 2ab \cos^3 \alpha. (1)

From the triangle ABCABC we also use the cosine theorem to find the length of the segment ACAC:

AC2=a2+b2−2abcos⁡α.AC^2 = a^2 + b^2 - 2ab \cos \alpha. (2)

Now, using the correspondence DEAC=k\frac{DE}{AC} = k given in the problem statement, from equations (1) and (2) we obtain

(a2+b2−2abcos⁡α)cos⁡2αa2+b2−2abcos⁡α=k2.\frac{(a^2 + b^2 - 2ab \cos \alpha) \cos^2 \alpha}{a^2 + b^2 - 2ab \cos \alpha} = k^2.

Hence cos⁡2α=k2\cos^2 \alpha = k^2. Solution cos⁡α=k\cos \alpha = k corresponds to the case of acute angle α\alpha, and cos⁡α=−k\cos \alpha = -k corresponds to the case of angle α\alpha. It remains to substitute the found values ​​into equation (2),

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Fig. 2. SEFLK=SFGML+sS_{EFLK} = S_{FGML} + s.

To get both answers to a given problem:

AC=a2+b2+2abkAC = \sqrt{a^2 + b^2 + 2abk}

or

AC=a2+b2−2abkAC = \sqrt{a^2 + b^2 - 2abk}.

In this problem, the main difficulty is the remote choice of the unknown. Introducing the angle α\alpha as an additional unknown gives a short and elegant solution to the problem. If we try to use another element in this role, for example, the values ​​of the segment DEDE, then we end up with a more complex system of equations, the solution of which I often find myself unable to solve.

Fig. 3.

  1. Let us consider the polygons obtained in the section (Fig. 2) of the tetrahedron indicated by the planes. It is easy to show that both the quadrilateral EFGH and the quadrilateral KLMN are rectogenous. Let us turn two angles by planes ABC and ACD onto the plane (Fig. 3) and denote the length of the segment EF by xx, and the length of the segment LM by yy. Since both triangles ABC and ACD are regular, and the sides of the rectangular triangles EFGH and KLMN are respectively parallel to the edges AB and CD, the segment KL becomes a continuation of the segment LM, and the segment FG becomes a continuation of the segment EF. If we denote the edge of the tetrahedron by aa, then it is obvious that FG=a−xFG = a - x, and KL=a−yKL = a - y. The trapezoid EFLK and FGML, as you can easily see, have equal heights. Let’s find them. The height hh of the trapezoid EFLK is equal to the difference in the heights of regular triangles EFC and KLC, therefore

h=x32−(a−y)32=32(x+y−a).h = x \frac{\sqrt{3}}{2} - (a - y) \frac{\sqrt{3}}{2} = \frac{\sqrt{3}}{2} (x + y - a).

Let us find the area of ​​the indicated trapezoids. The area of ​​the trapezoid EFLK is

EF+LK2h=x+a−y2h,\frac{EF + LK}{2} h = \frac{x + a - y}{2} h,

and the area of ​​the trapezoid FGML is equal to

FG+ML2h=a−x+y2h.\frac{FG + ML}{2} h = \frac{a - x + y}{2} h.

Using the conditions that the difference between the indicated areas is equal to ss, we obtain

x+a−y2h−a−x+y2h=s\frac{x + a - y}{2} h - \frac{a - x + y}{2} h = s

or

s=h(x−y);s = h (x - y);

Substituting instead of hh the expression found for it, we get

s=(x−y)(x+y−a)32.s = (x - y) (x + y - a) \frac{\sqrt{3}}{2}.

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Let’s return to the rectangles EFGH and KLMN. Their areas are equal to x(a−x)x(a-x) and y(a−y)y(a-y), respectively, and the difference in areas

σ=y(a−y)−x(a−x)=(x−y)(x+y−a).\sigma = y(a-y) - x(a-x) = (x-y)(x+y-a).

Comparing the expressions for ss and σ\sigma, that σ=2s/3\sigma = 2s/\sqrt{3}

In this problem, the choice of unknowns is quite natural. The most difficult part of the solution is the transition from the spatial figure 2 to the development of two adjacent faces onto the plane (Fig. 3); After this, the problem can be solved without much difficulty.

  1. Let’s add the first and third equations with the notified second. We get 2x2+2y2+8z2+4xy+8xz+8yz=02x^2 + 2y^2 + 8z^2 + 4xy + 8xz + 8yz = 0

Reducing by 2, we see that on the left side of the equation there is a complete square of the expression x+y+2zx+y+2z, hence z=−12(x+y)z = -\frac{1}{2}(x+y). (1)

Subtract the third equation from the second equation of this system and obtain x2+4xz−y2−8yz=0x^2 + 4xz - y^2 - 8yz = 0. Let us substitute the found value zz (1) x2−2x(x+y)−y2+4y(x+y)=0x^2 - 2x(x+y) - y^2 + 4y(x+y) = 0 into it.

After opening the brackets and bringing similar terms, the equation is reduced to the form x2−2xy−3y2=0x^2 - 2xy - 3y^2 = 0. Let us express xx from it through yy:

x=y±2y.x = y \pm 2y.

So, either x=−yx = -y or x=3yx = 3y.

Let’s consider the first case: x=−yx = -y. From equation (1) we obtain z=0z = 0. And then from the third equation of the original system it follows that y2=1y^2 = 1.

From here we find two values ​​for yy: y=1y = 1 or y=−1y = -1.

Thus, in the first case we get two solutions:

x1=−1,y1=1,z1=0;x_1 = -1, y_1 = 1, z_1 = 0;

x2=1,y2=−1,z2=0.x_2 = 1, y_2 = -1, z_2 = 0.

Let’s consider the second case: x=3yx = 3y. From the same equation (1) it follows that z=−2yz = -2y. Substituting this value for zz into the third equation of the original system, we obtain that −7y2=1-7y^2 = 1. So, in the second case there are no valid solutions.

It remains to check that the solutions found in the first case satisfy the equations of the initial system. This turns out to be true. Thus, two valid solutions of this system have been found.

The main difficulty of this problem is transforming the equation of a given system to a simpler system. Those applicants who try to solve this problem “at ease” by eliminating the unknowns have encountered insurmountable difficulties. Note that this system can be reduced to other systems that differ from those we have analyzed, but they also allow a simple solution.

According to the information we have, almost all received solutions to at least one problem. The vast majority (about 95%) received at least two tasks, more than half of those received received at least three tasks, and a third received at least four tasks.

We present an option for an independent solution.

  1. Solve equation lg⁡(98−x3)lg⁡(2−x)=3\frac{\lg(98-x^3)}{\lg(2-x)} = 3

  2. Find the height of an equilibrated trapezoid if its diagonals are mutually perpendicular and the area of ​​the trapezoid is SS.

  3. In Δ ABC, the exterior angle at vertex AA is three times greater than BB, and the sides AB,BC,ACAB, BC, AC (in that order) form an arithmetic progression. Find the angles of the triangle.

  4. Solve the system of equations.

{3xy−16xz=−5,xz+8yz=4,yz−3xy=1\begin{cases} 3xy - \frac{16}{xz} = -5, \\ xz + \frac{8}{yz} = 4, \\ yz - \frac{3}{xy} = 1 \end{cases}

  1. At the base of the triangular paramid SABCSABC lies the regular triangle ABCABC. Each of the plane angles ⇒CSA\Rightarrow CSA and ⇒ASB\Rightarrow ASB is 45∘45^\circ and ⇒SAB=arctg2\Rightarrow SAB = \arctg 2. Through vertex CC a section is drawn perpendicular to edge SASA. Find the dihedral angle between the base plane and the section plane. (Find all solutions.)

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Problems of this type are often given in university application exams, and it is useful for applicants to become familiar with some methods for solving them.

A few words about the laws themselves. They can be formulated in different ways, and not in this case. The main thing is the concept of their physical content. Let’s remember the most important thing.

Newton’s first law states that a body has no acceleration (stands still or moves straight and uniformly) if no forces act on it or their total effect is zero. In other words, the acceleration a⃗=0\vec{a}=0 and the speed v⃗\vec{v} are constant if ΣF=0\Sigma F=0.

The vector meaning of the law is important. It is the vector sum of forces that must be equal to zero (Fig. 1), it is the velocity vector that remains constant in this case: the speed is unchanged in magnitude and direction.

If the resultant of all forces applied to the body R⃗=ΣF\vec{R}=\Sigma F is different from zero, then an acceleration proportional to this resultant and inversely proportional to the mass of the body mm inevitably arises.

a⃗=ΣFm\vec{a} = \frac{\Sigma F}{m}

This is Newton’s second law. And again, its vector character is very significant: the vector equality a⃗=ΣFm\vec{a} = \frac{\Sigma F}{m} means that the total acceleration is not only proportional to the resultant forces applied to the body, but also coincides with it in direction. You can, of course, think like this: each force causes its own acceleration, coinciding with it in direction, and the total acceleration is equal to the vector sum of these accelerations (Fig. 2).

It should be remembered that the direction of the force coincides with the acceleration, and not the speed, which, generally speaking, can be directed as an angular direction, depending on how the body moved previously. So, for example, during the flight of a stone thrown at an angle to the horizon, its speed continuously changes its magnitude and direction, while the one causing these changes

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the force of gravity P⃗=mg⃗\vec{P} = m\vec{g} and the acceleration of free fall g⃗\vec{g} are practically unchanged (Fig. 3).

The third law states that all forces in mechanics are forces of interaction between bodies, equal in magnitude, opposite in direction and applied to different bodies (Fig. 4). The latter is sometimes forgotten by asserting, for example, that a body standing on the ground is balanced according to Newton’s third law by the forces acting on it: the force of gravity P⃗\vec{P} and the reaction force of the support N⃗\vec{N} (Fig. 5). In fact, the equality of these forces has nothing to do with Newton’s third law and, as we will soon see, may not be satisfied at all.

Which of these forces, however, in accordance with Newton’s third law, has its own “pair”, equal in magnitude, opposite in direction and applied to another body, in our case - to the earth: support reaction force N⃗\vec{N} - force of pressure of the body on the ground N⃗′\vec{N}' force of attraction of the body to the earth P⃗\vec{P} - force P⃗′\vec{P}', pulling the earth towards the body (Fig.6).

Let us now consider how to solve problems. Newton’s laws are usually used when calculating forces and acceleration. To solve these problems (as, indeed, any others) there are no universal sieves; you just need to have a good understanding of the applied laws, correctly understand the physical system of the processes discussed in the problem, and know the most general ways of approaching its solution. You can, for example, propose the following, of course not at all obligatory, sequence of actions:

first, depict on a diagram moving bodies and the forces acting on them;

second, to determine the direction and nature of the movement (sometimes, however, this can only be done at the end);

third, for each movement of the body, select two axes (usually along the expected direction of movement and perpendicular to it) and distribute the forces acting on the body along these axes (project them onto them);

fourth, write down Newton’s second law for each body, separately for each axis. In this case, the projections of forces and accelerations

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on the axis are considered positive if their directions coincide with the positive direction of the axis, and negative if they are directed oppositely (Fig. 7);

five - having solved the compiled equations, find the unknowns.

Let’s look at a few examples.

  1. Find the tension of the threads and the acceleration of the loads in the system shown in Fig. 8. The thread is considered inextensible, the resistance forces, the mass of the block and the thread are not taken into account.

Let us first consider what forces act on each of the loads. Firstly, this is the gravity force P=mgP=mg. If we accept g=10 m/сек2g=10\text{ m}/\text{сек}^2, then P1=20 н,P2=5 н,P3=25 нP_1=20\text{ н}, P_2=5\text{ н}, P_3=25\text{ н}.

Secondly, the tension force of the threads acts on each of the weights: T1T_1 - on the first and second weights and T2T_2 - on the second and third.

Note, by the way, that the force T1T_1 is the same for the first and second loads only in the case when the mass of the block and thread can be neglected. If the mass of the thread were not small, then the acceleration of each section of the thread would be imparted by the difference in the tension forces of the threads. Therefore, the tension forces of the threads acting on different loads could not be the same.

The same is true for a block: it can be set in motion, strictly speaking, only if the thread is pulled stronger on one side than on the other.

Having depicted on the diagram the forces acting on the loads (Fig. 9), we will try to determine the direction and nature of the movement.

The right side of the system is heavier, so the weights m2m_2 and m3m_3 will begin to fall, and the weight m1m_1 will rise. The movement will be uniformly accelerated with the same acceleration for all loads, or the predominance of the weight of the right side in the absence of resistance forces and inextensibility of the threads is equivalent to the action of a constant resultant force on the system as a whole, which, according to Newton’s second law, should cause constant acceleration.

We can also estimate the magnitude of the pushing forces. It is clear, for example, that T1>P1T_1>P_1, or for the first load the acceleration, and therefore the resulting force, must be directed upward. Likewise T2<P3T_2<P_3, and P2+T2>T1P_2+T_2>T_1 (Fig. 9).

The choice of axes is appreciated: for the first load, it is convenient to direct one axle upward, for the second and third - downward (along the movement). As for the second (perpendicular) axis, then in this

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task, it is simply not needed: none of the forces are projected onto it—all of them are directed either up or down and therefore are projected entirely only onto the first axis.

Now you can easily write the equation of motion (the equation of Newton’s second law) for each of the three groups:

T1−P1=m1a,T_1 - P_1 = m_1 a,
P2+T2−T1=m2a,P_2 + T_2 - T_1 = m_2 a,
P3−T2=m3a.P_3 - T_2 = m_3 a.

We have obtained three equations, from which we can easily find three unknowns (a,T1a, T_1 and T2T_2).

Substituting, for example, T1T_1 and T2T_2 from (1) and (3) into (2), we obtain

aP2+P3−P1m1+m2+m3=2π/сек2.a \frac{P_2 + P_3 - P_1}{m_1 + m_2 + m_3} = 2 \pi / \text{сек}^2.

Substituting this result into equation (1) and (3), we find

T1=P1+m1a=24 н,T_1 = P_1 + m_1 a = 24 \text{ н},
T2=P3−m3a=20 н.T_2 = P_3 - m_3 a = 20 \text{ н}.

The axes, of course, could be directed differently, for example, for the first load not up, but down. Then instead of T1−P1=m1aT_1 - P_1 = m_1 a we would write P1−T1=−m1aP_1 - T_1 = -m_1 a, which would not affect the final result at all.

  1. Find the acceleration, the pressure of the body on the inclined plane and the friction force (Fig. 10). Friction coefficient k=0,2k = 0,2. The force F=10 нF = 10 \text{ н} is directed vertically upward.

Four forces act on the body: force FF - up, force of gravity PP - down, reaction of support NN - perpendicular to the inclined plane and friction force fтрf_{\text{тр}}, the direction of which can be found out only by determining the direction of movement of the body. In such cases, they usually estimate where the body would move without friction under the influence of all other forces, in our case - under the influence of forces F,PF, P and NN (Fig. 11a). The force of friction, it is very clear, is not able to change the direction of movement, but can only reduce its speed or even completely slow down the body.

It can be suggested that the body will slide along the inclined plane up or down. To determine the direction of movement, we choose two axes: the xx axis is directed along the inclined plane, the yy axis is directed perpendicular to it (Fig. 11b). Having expanded the forces F,PF, P and N∗N^* along these axes), we see

*) Let us note by the way that, having expanded the force along the axes, it is necessary to remember that it has already been replaced by others, and therefore it can either be crossed out at figure so as not to be considered as acting again. Or create a new figure with one “decomposed” force

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Let us assume that the body can only move downwards along the plane, since of the two forces acting along it, Psin⁡αP\sin\alpha is greater than Fsin⁡αF\sin\alpha. The friction force, therefore, can only be directed upward along the inclined plane.

In our example, we must, however, allow for one more possibility: the force FF may be so great that the body will not slide along the plane at all, but will turn away from it. However, comparing the “pressing” force Pcos⁡α=17,4P\cos\alpha=17,4 and force Fcos⁡α=8,7F\cos\alpha=8,7 we see that the first is greater than the second, and therefore the body cannot be torn off the plane.

It must be said that the difference between these forces Pcos⁡α−Fcos⁡α=8,7πP\cos\alpha-F\cos\alpha=8,7\pi gives the desired pressure force of the body on the plane and the support reaction NN, equal in magnitude to it.

Let us now write Newton’s second law, remembering that forces directed opposite to the positive direction of the axis are considered negative. For the yy axis we obtain.

Fcos⁡α+N−Pcos⁡α=0F\cos\alpha+N-P\cos\alpha=0

(1)

(there is no acceleration in this direction, therefore the sum of forces is zero). And for the axis xx we get:

Psin⁡α−Fsin⁡α−fтр=ma.P\sin\alpha-F\sin\alpha-f_{\text{тр}}=ma.

(2)

In problems of this type, mistakes are sometimes made when determining the magnitude of the friction force. To get used to problems with horizontal moving bodies, they often, without thinking twice, calculate the friction force as the product of the friction coefficient and the weight of the body.

In fact, fтр=k⋅Nf_{\text{тр}}=k\cdot N, where NN is the normal pressure force (support reaction), that is, the force acting on the body perpendicular to the sliding plane (or equal in magnitude and opposite in direction to the force of pressure of the body on the plane).

In our problem, we need to take into account both the angle of inclination of the plane and the force FF, which somewhat reduces the force of normal pressure:

fтр=k(Pcos⁡α−Fcos⁡α)=k(P−F)cos⁡α=0,2(20−10)0,87=1,74πf_{\text{тр}}=k(P\cos\alpha-F\cos\alpha)=k(P-F)\cos\alpha=0,2(20-10)0,87=1,74\pi

Now from equation (2) it is easy to find the acceleration of the body:

a=(P−F)sin⁡α−fтрm=(20−10)0,5−1,742=1,63π/cek2.a=\frac{(P-F)\sin\alpha-f_{\text{тр}}}{m}=\frac{(20-10)0,5-1,74}{2}=1,63\pi/cek^2.

  1. The rocket is equipped with a spring scale on which a block rests. Before departure the scales show 10 NN. In flight, the scales first show 30 NN, then 10 NN, 5 NN, 0 NN. What can be said about the acceleration and direction of the rocket’s motion at these moments in time?

Let’s look at the strength first.

Two forces act on the block: gravity PP and support reaction NN (Fig. 12). When the rocket has no vertical acceleration (for example, before takeoff), these forces are equal. In our case P=N=10P=N=10 NN.

If the rocket (and therefore the block) moves accelerated, upward, to the right, then these equal forces must be directed upward (N>PN>P). If the acceleration is directed downward, then P>NP>N.

What do the scales show? Of course, not gravity, as is sometimes thought. They all record the force with which the block presses on them. This force is applied to the scales and, in accordance with Newton’s third law, is equal in magnitude and opposite in direction to the reaction of the support NN applied to the block

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From the conditions of the problem it is clear that the support reaction force NN and the force of pressure on the support, or weight, equal to it in magnitude, then change during the flight and, generally speaking, are not equal to the gravitational force P=mgP=mg, which practically can be considered constant (if we pretend to change it with height). Let’s write down Newton’s second law for motion along an axis directed upward:

N−P=maN-P=ma

Substituting here N1=30N_1=30 κ\kappa, P=10P=10 κ\kappa, m=1m=1 κ(m=Pg=1010=1κ)\kappa \left( m=\frac{P}{g}=\frac{10}{10}=1 \kappa \right), we get: a1=N1−Pm−30−101=20 m/cek2a_1=\frac{N_1-P}{m}-\frac{30-10}{1}=20 \, m/cek^2. The acceleration is positive and is therefore directed upward.

For N2=10N_2=10 κ\kappa we get a2=0a_2=0, for N3=5N_3=5 κ\kappa a3=−5 m/cek2a_3=-5 \, m/cek^2, for N4=0N_4=0 a4=−ga_4=-g. In the last two cases, the acceleration is negative, which means it is directed downward, or in our equation we considered NN and aa to be directed equally (both positive).

As for the direction of movement, one should caution against the latter conclusions. It is erroneous, for example, to say that the rocket first moved upward (a1>0a_1>0), then stopped (a2=0a_2=0), began to accelerate downwards (a3<0a_3<0) and, finally, went into free fall (a4=−ga_4=-g). In fact, the rocket could move in other ways, for example, all the time upward: accelerated (a1>0a_1>0), at a constant speed (a2=0a_2=0), slowly (a3,4<0a_3,4<0). Acceleration equal to the acceleration of gravity only means that the resultant of all forces acting on the rocket is equal to the force of gravity; At the same time, it can move upward - with the engine turned off, if you do not take into account the resistance forces, or when it is working in such a way that these forces overcome the traction forces. All bodies in the rocket in this case will be in a state of improbability, that is, their pressure on the support and the reaction of the latter will be equal to zero.

The whole point is that we found only acceleration, and not speed and not direction of movement, about which, in the conditions of our task, unfortunately, it is impossible to say anything.

  1. A ball of mass mm hanging on a thread of length RR is moved to the side to a horizontal position and released (Fig. 13). Determine the tension in the thread and the acceleration of the ball when the thread is at an angle of α\alpha to the horizontal. Find the law of change in the tension forces of the thread, speed and acceleration of the ball depending on the angle α\alpha. Claim the forces of resistance.

To solve, we will use the same method as before: we will arrange the forces on figure, estimate what the direction and nature of the movement could be, select the axes and, having distributed the forces along them, write the equation of motion.

Two forces act on the ball: the gravitational force PP and the tension force of the thread TT (Fig. 14). It will move, very indo, along an arc of radius RR.

We will direct one of the axes (x)(x) tangentially to the trajectory, the second (y)(y) perpendicular to it - along the radius. Having expanded the forces along them, we see that the force PcosαPcos\alpha acts along the xx axis, and the TT and PsinαPsin\alpha forces act along the yy axis.

The force PcosαPcos\alpha causes the so-called tangential, or tangential, acceleration ata_t, which changes the speed in magnitude.

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ata_t is a vector directed like Pcos⁡αP \cos \alpha tangentially to the trajectory of the ball (Fig. 15).

The resultant forces TT, Psin⁡αP \sin \alpha impart centripetal (normal) acceleration to the ball, changing the speed in direction (Fig. 16.).

Having written Newton’s second law, for motion along the xx and yy axes we obtain:

Pcos⁡α=mat,P \cos \alpha = m a_t,

T−Psin⁡α=man.T - P \sin \alpha = m a_n.

From equation (1) we immediately find the tangential acceleration ata_t and the law of its change:

at=Pcos⁡αm=mgcos⁡αm=gcos⁡α.a_t = \frac{P \cos \alpha}{m} = \frac{mg \cos \alpha}{m} = g \cos \alpha.

The centripetal acceleration that occurs during any curved movement is also a vector. It is always directed inside the trajectory along the radius and is caused by the algebraic sum of the radial projections of all forces acting on the body. The magnitude of centripetal acceleration, as is known, is calculated by the formula an=v2Ra_n = v^2 R. RR is known, and we will find the speed by writing the law of conservation of energy:

mgh=mv22,m g h = \frac{m v^2}{2},

where h=Rsin⁡αh = R \sin \alpha (Fig. 17). Hence v=2gh=2gRsin⁡αv = \sqrt{2 g h} = \sqrt{2 g R \sin \alpha} and an=2gRsin⁡αa_n = 2 g R \sin \alpha. Velocity vv and centripetal acceleration ana_n are zero in the upper position (sin⁡α=0\sin \alpha = 0) and maximum in the lower position (α=90∘\alpha = 90^\circ, sin⁡α=1\sin \alpha = 1).

Tangential acceleration ata_t, on the contrary, is most significant at the beginning of the movement at the top (cos⁡α=1\cos \alpha = 1) and is equal to zero when the thread is vertical

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(with α=0\alpha = 0). After the ball passes the lowest point of the trajectory, ata_t becomes negative (from α<0\alpha < 0). It is directed against the speed (Fig. 18) and reduces it (by the way, this is clear from the law of conservation of energy - hh in formula (3) kills).

We found the values ​​of speed, tangential and centripetal acceleration for an arbitrary angle α\alpha, as well as the law of their change depending on the change in this angle. Their directions are also known for any moment in time (ata_t and vv - along the tangent, ana_n - along the radius). Terri, we can also determine the total acceleration equal to the vector sum of the tangential and centripetal acceleration (at+ana_t + a_n) (Fig. 19).

The tension force of the thread and the law of its change depending on the angle are not difficult to find from equation (2): T=Psin⁡α+manT = P\sin\alpha + ma_n.

Substituting here instead of ana_n the found value 2gsin⁡α2g \sin\alpha, we get T=Psin⁡α+2mgsin⁡αT = P\sin\alpha + 2mg\sin\alpha, or T=3Psin⁡αT = 3P\sin\alpha.

The thread tension is maximum when the ball passes the bottom position (sinα\alpha has the highest value of 1).

Try to solve the following problems yourself.

  1. Consider example 2 for the case when the force FF is directed not upward, but at an angle β=45∘\beta = 45^\circ to the inclined plane (Fig. 20) and is equal to: 15 к15\, \text{к}, 20 к20\, \text{к}, 30 к30\, \text{к} (the calculation is carried out for all three cases).

  2. Continue solving Example 4 by determining how, when the ball moves, the directions of the equal forces applied to the ball and the total acceleration change.

  3. Find the thread tension, acceleration and friction force of the load m2m_2 on the inclined plane (Fig. 21) for the friction coefficient k1=0,1k_1 = 0,1 and for k2=0,2k_2 = 0,2. The thread is considered indestructible, the mass of the block and thread is not taken into account.

  4. Solve a problem similar to the third one, but with the following changes: instead of the load m2m_2, there are two weights m2=2 кm_2 = 2\, \text{к} and m3=5 кm_3 = 5\, \text{к}, connected by a thread (Fig. 22); friction coefficient for the second load is k2=0,1k_2 = 0,1, for the third one k3=0,05k_3 = 0,05. Additionally, it is necessary to determine the thread tension between the second and third weights.

Fig. 20
Fig. 21
Fig. 22

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Moscow Mathematical…

Mathematics is needed in everything. It is needed in natural scientific research, engineering calculations, and various types of economic management systems.

Necessary mathematicians, the ability to solve problems related to the use of mathematical methods and computer technology in various fields of science and human activity. Such mathematicians are called specialists in applied mathematics.

Being a specialist in applied mathematics is difficult, but interesting and exciting. He must know, firstly, what to apply (general mathematics science), secondly, how to apply (special mathematical sciences), and thirdly, what to apply (specific issues of science and human activity).

Such specialists are trained at the Moscow Mathematical Technical Institute of the Ministry of Industry, Automation and Control Systems of the USSR *).

Moscow Mathematical Technical (MMT) has existed since 1967 and has already given two graduations on the basis of a 10-year school and one graduation on the basis of an 8-year school.

The duration of study at MMT for those who have completed the 8th grade of secondary school is 2 years 10 months, and for those who have completed the 10th grade - 1 year 10 months. Graduates receive the qualification “computer-mathematician” in the specialty “Applied Mathematics”.

They are prepared to work in computing and research centers, departments and laboratories, in design and engineering bureaus, and in enterprises.

In his work, a computer mathematician develops algorithms for solving problems on electronic computers, creates and uses programs for solving problems, implements solutions on the machine and analyzes the results obtained. Therefore, he must have a high mathematical culture. For this purpose, it is indicated that general mathematical disciplines are studied in MMT (algebra, geometry, mathematical analysis, linear algebra and analytical geometry, mathematical logic, probability theory), and special mathematical disciplines (linear and nonlinear programming, computational mathematics, programming and algorithmic languages, operations research, application of mathematical methods in natural scientific research, in automation and control systems, in solving economic problems). Those admitted after 8th grade also receive general secondary education.

In order to enroll in MMT after completing grades 8 or 10, it is enough to pass an oral exam in mathematics and a written exam in literature.

Each math exam ticket includes both theoretical questions and several exercises. When answering questions, the applicant is required to present the question clearly and mathematically correctly. When solving problems, you must be able to carefully justify each step of the solution, providing all the necessary references to the relevant definitions, aximons and theorems.

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The exam also asks additional questions about theory and its application in solving problems; the content of tickets and additional questions does not go beyond the scope of the school curriculum.

Here are samples of exam paper options from 1970

Option for those who have completed 8th grade

  1. Extracting the square root of a product.
  2. Sine, cosine and tangent angle and their meanings for an angle of 60°.
    3 a) Perform actions:

(1314−2527−1056)⋅230.04+46.75\left(13 \frac{1}{4} - 2 \frac{5}{27} - 10 \frac{5}{6}\right) \cdot 230.04 + 46.75

0,01

  1. Solve the system of equations:

{x2=20−y2,x+y=6\begin{cases} x^2 = 20 - y^2, \\ x + y = 6 \end{cases}

c) In an equilateral trapezoid, the bases are kk cm and ll cm. The diagonals are mutually perpendicular. Find the area of ​​the trapezoid.

Option for those who have completed 10th grade

  1. Exponential function, its properties and graph.
  2. Signs of parallelism of straight lines and planes.
    3 a) Simplify:

[12+y12−(x+y)12]−2−x+y2Vxy\left[ \frac{\frac{1}{2} + y}{\frac{1}{2}} - \frac{(x + y)}{\frac{1}{2}} \right]^{-2} - \frac{x + y}{2Vxy}

  1. Solve inequality:

log⁡2x−3x>1\log_2 x - 3 x > 1

c) Find the value of M(x)M(x) if M(x)=tg6x+sec⁡6xM(x) = \text{tg} 6x + \sec 6x, tg3x=2\text{tg} 3x = 2 and 0<x<π60 < x < \frac{\pi}{6}.

All that remains is to tell you the address of MMT: Moscow, E-43, Nizhnyaya Pervomaiskaya, 14 (there is no public service with equipment yet).

A. G. Terushkin

To note «Kvant»
for younger students

(see «Kvant» No. 4, 1971, 3rd cover page)

  1. Note that for each break we notify the number of pieces per one. The total number of pieces is 4×8=324 \times 8 = 32. Before breaking we had one piece, after the first breaking there were two, after the second breaking there were three, …, after the 31st breaking there were 32. Thus, in each order we break the chocolate bar, we will always have to break it exactly 31 times.

  2. The cipher is as follows: hard vowels are replaced with their corresponding soft vowels, and soft vowels with hard ones (aa with rr, yy with ll and tt. D.); similarly, voiced consonants are replaced by glyhnye, and glyhnye by their corresponding voiced ones (bb to nn, bb to ϕ\phi, 22 to kk and tt. D.); In addition, the hissing and whistling consonants (μ1−μ\mu_1 - \mu, x−μx - \mu) and signs 7−b7 - b have been rearranged.

Answer:
Our Tanya is crying loudly,
I dropped a ball into the stove.
Hush, Tanechka, don’t cry,
The ball will not sink in the stove.

  1. The required method is shown at figure 1.
  2. 7 375 428 413:125 473=58 781.
  3. The new arrangement of matches is shown at figure 2.

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To the article “Potential energy graphs”

Task 1

As shown in figure 1, at E<U0E < U_0 movement is possible in two areas ABAB and CDCD; if E>U0E > U_0, then there is only one area of ​​motion - NMNM.

Task 2

When the body moves to the right of the equilibrium position (point BB on figure 13), the tangent of the tangent angle to the potential energy graph becomes negative, i.e. the force is positive and takes the body out of the equilibrium position. The point BB is called the inflection point; Thus, we have proven that the equilibrium at the inflection point is unstable. Equilibrium positions are also points AA, CC and sections (C,∞)(C, \infty) and (−∞,A)(-\infty, A). Point CC and the entire section (C,∞)(C, \infty) correspond to an indifferent equilibrium. If you move a body from any point on the potential energy line (C,∞)(C, \infty), then it remains in equilibrium in the new position. A similar situation occurs at section (−∞,A)(-\infty, A), with the exception of point AA itself. The equilibrium at point AA is unstable; to make sure of this, it is enough to slightly shift the body to the right; the tangent of the angle of inclination becomes negative, i.e. the force is positive, and therefore directed from the equilibrium position (the sled rolled down from AA). The graph of sleep versus coordinate is shown in figure 2.

Task 3

A change in potential energy by a constant value CC graphically corresponds to a displacement of the abscissa axis up or down (depending on the sign CC) relative to the ordinate axis. In this case, very/no, the angle of inclination of the tangent to the “new” axis xx coincides with the angle of inclination to the “old” axis xx. Since the force is equal in magnitude to the tangent of this angle, it remains unchanged during this transformation of potential energy.

Task 4

A cube floating in a liquid is subject to two forces: the gravitational force and the buoyant force. As long as the immersion depth of the cube hh satisfies condition 0≤h≤a0 \leq h \leq a, the total force is equal to F=ρKa3g−ρKa2hgF = \rho_K a^3 g - \rho_K a^2 h g.

Let us put h=h0+xh = h_0 + x, where h0=aρKρKh_0 = a \frac{\rho_K}{\rho_K}.

Then F=−ρKa2gxF = -\rho_K a^2 g x if −h0≤x≤a−h-h_0 \leq x \leq a - h. After the cube is completely immersed in the liquid (h>ah > a), regardless of the depth, a constant force F=−(ρK−ρK)a3gF = -(\rho_K - \rho_K) a^3 g acts on it; similarly, a constant buoyant force F=ρKa3gF = \rho_K a^3 g acts on a cube not immersed in liquid. As a result, the dependence of dreams FF on the coordinate xx has the form shown in figure 3. As one would expect, x=0x = 0 is the equilibrium position. It is easy to verify by directly calculating the area that

U(x)=ρKa2g2x2, если −h0≤x≤a−h0;U(x) = \frac{\rho_K a^2 g}{2} x^2, \text{ если } -h_0 \leq x \leq a - h_0;

U(x)=ρKa2g2(a−h0)2+(ρK−ρK)a3gxU(x) = \frac{\rho_K a^2 g}{2} (a - h_0)^2 + (\rho_K - \rho_K) a^3 g x

at x>a−h0x > a - h_0, and

U(x)=ρKa2g2h02−ρKa3gx,U(x) = \frac{\rho_K a^2 g}{2} h_0^2 - \rho_K a^3 g x,

when x<−h0x < -h_0.

The potential energy graph is shown at figure 4. We chose the constant CC so that U(0)=0U(0) = 0. It can be seen that x=0x = 0 is the position of the missing equilibrium.

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To the article
“Hippocrates’ Bows”

Exercise 2c. Consider triangle BFC. We carry out additional constructions - segments BD, DC and FD (see Fig. 8e, in the article).

It is easy to show that the lines BF and DC are parallel. As a result, the areas of triangles BFC and BFD are equal. It remains to calculate the ratio of the area of ​​the circle whose circumference passes through points B. F and D to the area of ​​the triangle BFD.

To the article “Physics helps geometry”

  1. Place material points of equal mass at the vertices of the tetrahedron and look for the center of gravity of the resulting system.

  2. AL:LB=1:2. (Place a point of mass 2m at vertex A, and a point of mass m at vertex B and vertex C.)

  3. By placing a point of mass m at vertex A, a point of mass 4m at vertex B, and a point of mass 2m at vertex C, we prove that B’L = 1/7 AL and, therefore, the area BB’L is equal to 1/7 of the area ABL, that is, 1/21 of the area ABC. Repeating this reasoning for the other two shaded triangles, we find that the area of ​​the three shaded triangles is 1/7 of the area of ​​triangle ABC.

To the note “First acquaintance with nomograms”

  1. The parabola y=ax² is obtained from the parabolas y=x² by stretching along the Ox axis with a coefficient 1a\frac{1}{\sqrt{a}}. In this case, the straight lines transform into straight lines intersecting the ordinat axis at the same point (see Fig. 1). Therefore, marks p can be placed at the same height as before, that is, at points with ordinates p² and abscissas, respectively

±p/a\pm p/\sqrt{a}

  1. Justification of the nomogram for paraboles y=x².

Let’s say we want to know what m×n is equal to. To do this, we connect point A, whose coordinates are (-m, m²) (Fig. 2),

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with point BB, whose coordinates are (n,n2)(n, n^2). Let for definition m<nm < n. Let us drop perpendiculars from points AA and BB onto the abscissa axis and draw a straight line through point AA parallel to this axis. It is clear that EF=CN=m2EF = CN = m^2, therefore BC=BN−CN=n2−m2BC = BN - CN = n^2 - m^2. Triangles ADEADE and ABCABC are similar, and the similarity coefficient is

AEAC=AEAE+EC=mm+n.\frac{AE}{AC} = \frac{AE}{AE + EC} = \frac{m}{m + n}.

Hence,

DE=mm+nBC=mm+n(n2−m2)=m(n−m)=mn−m2.DE = \frac{m}{m + n} BC = \frac{m}{m + n} (n^2 - m^2) = m (n - m) = mn - m^2.

From here

DF=DE+EF=(mn−m2)+m2=mn.DF = DE + EF = (mn - m^2) + m^2 = mn.

The case m>nm > n is treated similarly. Case m=nm = n is very iden.

Analytical justification of the nomogram for the parabola y=ax2y = ax^2. The line passing through the points (−ma,m2)\left(-\frac{m}{\sqrt{a}}, m^2\right) and (na,n2)\left(\frac{n}{\sqrt{a}}, n^2\right) is given by the equation (at m+n≠0m + n \neq 0)

y=m2x−na−m−na+n2x−−man−−ma=m2n+n2mm+n=mny = m^2 \frac{x - \frac{n}{\sqrt{a}}}{-m - \frac{n}{\sqrt{a}}} + n^2 \frac{x - \frac{-m}{\sqrt{a}}}{n - \frac{-m}{\sqrt{a}}} = \frac{m^2 n + n^2 m}{m + n} = mn

It intersects the ordinate axis at the point

y=m2−na−m−na+n2−man−−ma=m2n+n2mm+n=mny = m^2 \frac{\frac{-n}{\sqrt{a}}}{-m - \frac{n}{\sqrt{a}}} + n^2 \frac{\frac{-m}{\sqrt{a}}}{n - \frac{-m}{\sqrt{a}}} = \frac{m^2 n + n^2 m}{m + n} = mn

To the article “What is it that we lose or find?”

  1. The answer contains construction roots, for example x=5π/6x = 5\pi/6; some solutions are lost, for example x=2π/3x = 2\pi/3. All this is the result of an incorrect transformation of the expression 4sin⁡22x\sqrt{4\sin^2 2x}. According to the definition of an arithmetic root,

4sin⁡22x=2∣sin⁡2x∣\sqrt{4\sin^2 2x} = 2|\sin 2x|

The correct answer is x=nπ/2x = n\pi/2 and x=π6+nπ2x = \frac{\pi}{6} + \frac{n\pi}{2}.

  1. The answer contains the construction of roots. They were obtained as a result of multiplying all parts of the equation by the function sin⁡x\sin x. Solutions to equation sin⁡8x=sin⁡x\sin 8x = \sin x are obviously also xx for which sin⁡x=0\sin x = 0, while for the original equation such xx are not solutions (check). Multiplying by a function can also lead to loss of roots, as this can lead to drying of OD3 (give an example!). In this example it does not do this, since the function sin⁡x\sin x is well defined.

The correct answer is: x=nπ/9x = n\pi/9, where nn is any odd number not a multiple of 9, and x=mπ/7x = m\pi/7, where mm is any odd number not a multiple of 7.

  1. The root found is postronium. It is incorrect to use the arc cosine of the number xx if m=xm = x and the number mm satisfies the inequality: 0≤m≤π0 \leq m \leq \pi. In this example, m=5π/2+10kπm = 5\pi/2 + 10k\pi and for which kk this inequality does not satisfy, and then the arckosi equation x=5π/2+10kπx = 5\pi/2 + 10k\pi, according to the definition of arckosi xx, has no solutions.

  2. Wrong to find OD3. It is also necessary to require that the base of the logarithm x−1x - 1 be different from 1, and then x=2x = 2 is not included in OD3 *).

  3. The root x=0x = 0 is construction. It was obtained as a result of replacing in the transformed equation the expression representing the left side of the original equation with its right side. Such a transformation could not lead to the loss of roots. Indeed, the last equation in the “solution” of Example 5 is a consequence of the original one; if the original equation is satisfied, then the last one is satisfied. The converse, as this example shows, is not true.

  4. The answer is odd. Indeed, let c=−1c = -1, a=−2a = -2, c=2c = 2, b=c2=1b = c^2 = 1. Then the equation has the form

x+2x+1+x=−1\sqrt{x + 2\sqrt{x} + 1} + \sqrt{x} = -1

and the answer question has no solutions at all (its left side is positive for any admissible xx). Next, let c=1c = 1, a=−2a = -2, b=1b = 1. Then the equation has the form

x−2x+1+x=1\sqrt{x - 2\sqrt{x} + 1} + \sqrt{x} = 1

and for example, the number x=4x = 4, again a question to answer, is not a solution. The fact is that when solving “by the method of squaring”, an equation is obtained that is not equivalent to the given one, but is its consequence. The received answer must be checked.

Examination. Substituting the parameter values ​​into the equation, we get

x−2cx+c2=c−x\sqrt{x - 2c\sqrt{x} + c^2} = c - \sqrt{x}

or

(x−c)2=c−x\sqrt{(\sqrt{x} - c)^2} = c - \sqrt{x}

From here

∣Vxˉ−c∣=c−x|V\bar{x} - c| = c - \sqrt{x}

*) Note that this root will be revealed from the answer by the authors of the school textbook (E. S. Kochetkov, E. S. Kochetkov, A. Algebra and elementary functions, M., “Prosveshchenie”, 1969, part 2, problem 1460, θ\theta).

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It is clear that for c<0c < 0 this equation has no solutions at all, but for c=0c = 0 it has a unique solution. Let c>0c > 0. Distance is also the value of the unknown that satisfies the 0≤x≤c20 \leq x \leq c^2 inequality. Then x≤c\sqrt{x} \leq c, ∣x−c∣=c−x|\sqrt{x} - c| = c - \sqrt{x}, and the equation obviously becomes an identity. So in this case the real equation has an infinite number of solutions: 0≤x≤c20 \leq x \leq c^2. It is easy to see that no values ​​of the unknown satisfy him.

Correct answer: an equation has infinitely many solutions if and only if a=−2ca = -2c, b=c2b = c^2 and c>0c > 0 (and the solutions are the numbers 0≤x≤c20 \leq x \leq c^2) *).

  1. The answer contains the construction of roots. The fact is that although all solutions to the equation ∣f(x)∣φ(x)=1|f(x)|\varphi(x) = 1 are contained among the equations ∣f(x)∣=1|f(x)| = 1 and φ(x)=0\varphi(x) = 0, among the latter there may be roots, a construction for the original equation. After all, it is entirely possible that for x=ax = a f(a)=1f(a) = 1 and φ(x)\varphi(x) does not exist, or φ(a)=0\varphi(a) = 0 and f(x)f(x) does not exist. Therefore, it is necessary to check whether the roots found above lie in OD3.

Examination. Since the exponent in the equations takes real values ​​only at x≥πx \geq \pi and x≤−7x \leq -7, then at k=0k = 0 and k=−1k = -1 the numbers x=2kπx = 2k\pi are not included in OD3. Not included in OD3 and x=πx = \pi, since in this case both the base and the exponent become zero. All other solutions found are included in OD3.

  1. The answer contains the construction of the solution. They were obtained as a result of incorrect use of the substitution method. Finding from the second equation that x=φ(y)x = \varphi(y), and putting together xx into the first equation φ(y)\varphi(y), we moved from the system
    {f(x,y)=0,g(x,y)=0\begin{cases} f(x, y) = 0, \\ g(x, y) = 0 \end{cases}
    to the system
    {f[φ(y),y]=0,f(x,y)=0.\begin{cases} f[\varphi(y), y] = 0, \\ f(x, y) = 0. \end{cases}
    instead of going to the system
    {f[φ(y),y]=0,x=φ(y)\begin{cases} f[\varphi(y), y] = 0, \\ x = \varphi(y) \end{cases}
    (here x=φ(y)x = \varphi(y) is an equation equivalent to equation g(x,y)=0g(x, y) = 0). In other words, having found yy from the first transformation of the equation, we find xx from the first original equation, but this should have been done from the second equation. Then we would get the correct answer: if y=4y = 4, then x=5x = 5, if y=1125y = \frac{112}{5}, then x=−1135x = -\frac{113}{5}.

*) The condition of the problem does not require such a complete answer. It would be enough to find some specific parameter values ​​for which a positive answer is obtained, and this is not at all difficult to do. However, such a complete solution is typical (and good!), so we present it.

  1. The answer is incorrect in case a=1a = 1. Indeed, for a=1a = 1 the system takes the form
    {x+y=1,x+y=1,\begin{cases} x + y = 1, \\ x + y = 1, \end{cases}
    and although it has an infinite number of solutions, still not every pair of numbers satisfies it. For example, the pair x=3x = 3, y=4y = 4 is not a solution to the system. The solutions of this system will be pairs of numbers x=tx = t, y=1−ty = 1 - t, where tt is any real number.

The construction of the solution resulted from careless use of the method of algebraic addition. System
{f(x,y)=0,g(x,y)=0\begin{cases} f(x, y) = 0, \\ g(x, y) = 0 \end{cases}
system is equivalent
{a1f(x,y)+b1g(x,y)=0,a2f(x,y)+b2g(x,y)=0,\begin{cases} a_1 f(x, y) + b_1 g(x, y) = 0, \\ a_2 f(x, y) + b_2 g(x, y) = 0, \end{cases}
if a1b2≠a2b1a_1 b_2 \neq a_2 b_1 (prove it). Otherwise, as our example shows, the possibility of resorting to constructed solutions. There will be no loss of roots (why?).

  1. The answer is correct for a≠0a \neq 0. For a=0a = 0 the equation has an infinite number of solutions: they fill the whole straight line y=−xy = -x. The loss of solution occurred due to the division of the equation into each other.

To the article “Entrance written exam in mathematics at the Faculty of Computational Mathematics and Cybernetics of Moscow State University in 1970”

1 - 3≤a≤−23 \leq a \leq -2,
x=±arccos⁡a+3+kπx = \pm \arccos \sqrt{a + 3} + k\pi,
k=0,±1,±2k = 0, \pm 1, \pm 2.

2 x≥16x \geq \frac{1}{6}.

3 30<v<33,630 < v < 33,6.

4 B=π−α2+12arccos⁡(π2sin⁡α−cos⁡α)B = \frac{\pi - \alpha}{2} + \frac{1}{2} \arccos \left( \frac{\pi}{2} \sin \alpha - \cos \alpha \right),
C=π−α2−12arccos⁡(π2sin⁡α−cos⁡α)C = \frac{\pi - \alpha}{2} - \frac{1}{2} \arccos \left( \frac{\pi}{2} \sin \alpha - \cos \alpha \right),
0<α≤2arctg2π0 < \alpha \leq 2 \arctg \frac{2}{\pi}.

5 arccos⁡(cos⁡2β2+sin⁡β2cos⁡α−cos⁡β)\arccos \left( \cos^2 \frac{\beta}{2} + \sin \frac{\beta}{2} \sqrt{\cos \alpha - \cos \beta} \right).

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To the article “Entrance written exam in mathematics at MIPT in 1970”

  1. x=−3x = -3. h=Sh = \sqrt{S}
  2. ⇒A=π−3\Rightarrow A = \pi - 3 arccos 3/43/4.
  3. B=arccos⁡3/4,⇒C=2arccos⁡3/4B = \arccos 3/4, \Rightarrow C = 2\arccos 3/4
  4. Four solutions:
    x1=22,y1=2,z1=22x_1 = \frac{\sqrt{2}}{2}, y_1 = \sqrt{2}, z_1 = 2\sqrt{2};
    x2=−22,y2=−2,z2=−22x_2 = -\frac{\sqrt{2}}{2}, y_2 = -\sqrt{2}, z_2 = -2\sqrt{2}
    x3=2,y3=−1/2,z3=4;x4=−2x_3 = 2, y_3 = -1/2, z_3 = 4; x_4 = -2.
    y4=1/2,z4=−4y_4 = 1/2, z_4 = -4.
  5. Two solutions: arctg 22 and arcsin 215\frac{2}{\sqrt{15}}.

To the article “Task on Newton’s laws”

  1. In all three cases, the projection of force FF onto the direction of possible movement Fcos⁡βF\cos \beta is greater than Psin⁡αP\sin \alpha, and therefore the body can only move upward along the plane.
    In the first case, on the plane N=Pcos⁡α−Fsin⁡β=6,8N = P\cos \alpha - F\sin \beta = 6,8 and the sliding friction force fTP=kN=1,36f_{TP} = kN = 1,36 is greater than the result of the other two forces acting along the plane, R=Fcos⁡β−Psin⁡α=0,6R = F\cos \beta - P\sin \alpha = 0,6 and therefore the body is motionless, and the static friction force (fTP,nf_{TP,n}) is equal in magnitude and opposite in direction to the force RR.
    In the second case, onto the plane N=3,3N = 3,3 and fTP=0,66f_{TP} = 0,66 and the body moves with acceleration
    a=Fcos⁡β−Psin⁡α−fTPm=1,72 м/сек2a = \frac{F\cos \beta - P\sin \alpha - f_{TP}}{m} = 1,72 \text{ м/сек}^2
    In the third case, Fsin⁡βF\sin \beta is greater than Pcos⁡αP\cos \alpha, the body breaks away from the plane and begins at an angle 19∘19^\circ to it with an acceleration a=5,9 м/сек2a = 5,9 \text{ м/сек}^2 (in all problems we assume g=10 м/сек2g = 10 \text{ м/сек}^2).

  2. The total acceleration (aполн=at2+an2a_{полн} = \sqrt{a_t^2 + a_n^2}) and the equilibrium forces TT and PP are directed at such an angle β\beta to the tangent to the trajectory that
    tgβ=anat=2gsin⁡αgcos⁡α=2tgαtg\beta = \frac{a_n}{a_t} = \frac{2g\sin \alpha}{g\cos \alpha} = 2tg\alpha
    (in particular, in the upper position - along the tangent, in the lower position - along the radius).

  3. In the first case:
    fTP=kN=k1P2cos⁡α=6,1f_{TP} = kN = k_1P_2\cos \alpha = 6,1
    a=P1−P2sin⁡α−fTPm1+m2=0,34 м/сек2a = \frac{P_1 - P_2\sin \alpha - f_{TP}}{m_1 + m_2} = 0,34 \text{ м/сек}^2
    T=P1−m1a=43,5T = P_1 - m_1a = 43,5
    In the second case, only motionless. T=45T = 45 and Static friction force fTP,n=T−P1−m1af_{TP,n} = T - P_1 - m_1a.

– P2sin⁡α=10P_2\sin \alpha = 10 and (силатренияскольженияfTP=k2P2cos⁡α=12,2сила трения скольжения f_{TP} = k_2P_2\cos \alpha = 12,2 and.).
4. fTP2=1,74f_{TP_2} = 1,74 and fTP3=2,17f_{TP_3} = 2,17 and a=0,53 м/сек2a = 0,53 \text{ м/сек}^2
The force T1T_1 of thread tension (by the inter-relief and second weights) is equal to 42,642,6 and aT2a T_2 (by the inter-relief and third weights) is equal to 29,829,8 and.

To ask “Moscow Mathematical…”
Option for those who have completed 8th grade
3. a) 10000.
6) x1=4x_1 = 4, y1=2y_1 = 2; x2=2x_2 = 2, y2=4y_2 = 4.
b) (k+l)2/4(k + l)^2/4
Option for those who have completed 10th grade
3. a) (x+y)24xy\frac{(x + y)^2}{4xy}.
6) 2<x<32 < x < 3.
b) M(x)=−3M(x) = -3.

You ask “What does indecisiveness lead to?”
(see «Kvant» No. 4, p. 7)

We only need one fact from analytical geometry: if the ends of a segment have coordinates (a1,b1)(a_1, b_1) and (a2,b2)(a_2, b_2), then the middle of this segment has coordinates
(a1+a22,b1+b22).\left(\frac{a_1 + a_2}{2}, \frac{b_1 + b_2}{2}\right).

Let Petya turn to the stage at point (a,b)(a, b), then at point (c,d)(c, d) - to Lucy’s house, at point (e,f)(e, f) - to the store and at point (a1,b1)(a_1, b_1) - again to the stage. Let’s find the coordinates of all these points, which are the midpoints of the segments connecting the last turning point with the corresponding vertex of the square
c=a2,d=b+12,e=a4,c = \frac{a}{2}, d = \frac{b + 1}{2}, e = \frac{a}{4},
f=b+14;f = \frac{b + 1}{4};
a1=12(a4+1)=18(a+4)a_1 = \frac{1}{2}\left(\frac{a}{4} + 1\right) = \frac{1}{8}(a + 4)
q1=12(b+14+1)=18(b+5)q_1 = \frac{1}{2}\left(\frac{b + 1}{4} + 1\right) = \frac{1}{8}(b + 5)
Check that then
a1−47=18(a−47),a_1 - \frac{4}{7} = \frac{1}{8}(a - \frac{4}{7}),
b1−57=18(b−57).b_1 - \frac{5}{7} = \frac{1}{8}(b - \frac{5}{7}).

Thus, the distances from the turning points to the stage to the point (4/7, 5/7) form a geometric progression and decrease by 8 times after each “round” in the direction of the stage - Lucy’s house - the store. This means that Petya is approaching a triangle with the coordinates of the vertices
(47,57),(27,67),(17,37)\left(\frac{4}{7}, \frac{5}{7}\right), \left(\frac{2}{7}, \frac{6}{7}\right), \left(\frac{1}{7}, \frac{3}{7}\right)

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Stamps and match labels dedicated to Russian mathematicians

In 1946, on the occasion of the 125th anniversary of the birth of the great Russian mathematician and mechanic Pafnutya Lvovich Chebyshev, figure artist E. Bulanova issued a series of postage stamps consisting of two miniatures. We present one of them at figure.

Above the portrait of the scientist is the inscription “Great Russian Mathematician,” which, however, does not fully reflect the role of P. L. Chebyshev in the development of Russian science. In addition to his brilliant mathematical achievements, P. L. Chebyshev left behind a number of outstanding research and inventions in mechanics, primarily related to the theory and practice of hinged-lever mechanisms that convert circular motion into rectilinear motion.

P. L. Chebyshev was the founder and inspirer of the St. Petersburg mathematical scale. Its outstanding representatives were academicians A. M. Lyapunov, A. A. Markov, V. A. Steklov. In 1967, a series of matchstick labels appeared with portraits of significant Russian physicists and mathematicians, among whom we see the St. Petersburg Mathematical Scale and his most prominent students. A. M. Lyapunov was not only a brilliant mathematician, but also a great mechanic. In 1967, for the 100th anniversary of his birth, also by figure E. Bulanova, a stamp was issued with a portrait of the scientist. Below it is a formula that gives the surface equation of the equilibrium figure of a rotating fluid. By the way, A. M. Lyapunov’s research on the equilibrium figures of a rotating fluid, the particles of which are engraved according to the law of universal gravitation, was undertaken on the initiative of his teacher P. L. Chebysheva.

The editor-in-chief is academician I. K. Kionn.
First Deputy Editor-in-Chief - Academician A. N. Kolmogorov.
Editorial collection: L. A. Artsimovich, M. I. Bashmakov, V. G. Botyansky, I. N. Bronshtein, N. V. Vasiliev, I. F. Ginzburg, V. G. Zubov, P. L. Kapitsa, V. A. Kirillin, V. A. Leshkovtsev (deputy “main editor”), V. P. Lishevsky, A. I. Markushevich, M. D. Millonshikov, N. A. Patrieeva, N. Kh. Rozov, A. P. Savin, I. Sh. Slobodetsky, M. L. Smolyansky (deputy “main editor”), Ya. A. Smorodinsky, V. A. Fabrikant.

Editorial Head L. V. Chernova
Chief artist A. I. Klimanov
Technical editor T. M. Makarova
Proofreaders T. S. Weisberg,
V. P. Sorokina
Publishing house “Science”
Main editorial office of physical and mathematical literature Moscow, V-71, Leninsky Prospekt, 15 Tel. 234-08-11

Delivered on January 27, 1971.
Signatures for printing 25/111 1971
Vumaga 70×100/16. Phys. oven l. 4.
Conditions. oven l. 5.2. Yu.-ed. l. 5.55.
Shooting gallery 287,380 copies T-03991.
Price 30 kopecks. Order 167
Chekhov printing plant Glavpoligrafroma
Press Committee under the Council of Ministers of the USSR, Chekhov, Moscow Region

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TO OUR READERS

Subscriptions continue for the second half of 1971 to the popular scientific journal of physics and mathematics «Kvant».

The magazine is designed primarily for students in grades 7–10. It is also useful for teachers, especially those who teach clubs or elective classes in physics or mathematics, as well as all lovers of mathematics and physics.

The main content of the magazine is a “physics and mathematics school,” that is, materials that help to better understand physics and mathematics, learn to apply these sciences to teach various phenomena and processes that we encounter in practice, and learn to solve problems.

The reader will find many tasks in the magazine. Among them are problems offered at entrance exams for various disciplines, problems offered at olympiads, and simply interesting problems.

Notes describing physical instruments and experiments will help the reader set up and test a physical experiment.

The magazine publishes on its pages articles of a review nature, telling about the achievements of science and problems that are still waiting to be solved, stories about scientists and stories from scientists themselves about how “science is done”, how scientific discoveries appear.

The magazine constantly publishes results on books - already published and those still being prepared for publication.

Room price 30 kopecks. When subscribing, refer to our index 70465.