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assumptions, the mass must vary in this way. (W© have to say “a few other |
assumptions” because we cannot prove anything unless we have some laws which |
--- Trang 312 --- |
we assume to be true, if we expect to make meaningful deductions.) To avoid |
the need to study the transformation laws of force, we shall analyze a collision, |
where we need know nothing about the laws of force, except that we shall assume |
the conservation of momentum and energy. Also, we shall assume that the |
momentum of a particle which is moving is a vector and is always directed in the |
direction oŸ the velocity. However, we shall not assume that the momentum is a |
constønt tìmes the velocity, as Newton did, but only that it is some ƒwncfion of |
velocity. We thus write the momentum vector as a certain coefficient times the |
vector velocity: |
Dp~Tn,„0®. (16.8) |
We©e put a subscript ø on the coeficient to remind us that it is a function of |
velocity, and we shall agree to call this coefficient m„ the “mass.” Of course, |
when the velocity is small, it is the same mass that we would measure in the |
slow-moving experiments that we are used to. Now we shall try to demonstrate |
that the formula for rm„ must be rmo/4/1 — 02/2, by arguing from the principle |
of relativity that the laws of physics must be the same in every coordinate system. |
1 9/2 6/2 |
¡ l 9/2 g/2 |
1 1 (b) |
Fig. 16-2. Two views of an elastic collision between equal obJects |
moving at the same speed In opposite directions. |
Suppose that we have two particles, like two protons, that are absolutely equal, |
and they are moving toward each other with exactly equal velocities. Theïir total |
mmomentum is zero. Now what can happen? After the collision, their directions |
of motion must be exactly opposite to each other, because If they are not exactly |
opposite, there will be a nonzero total vector momentum, and momentum would |
not have been conserved. Also they must have the same speeds, since they are |
exactly similar objects; in fact, they must have the same speed they started with, |
since we suppose that the energy is conserved in these collisions. 5o the diagram |
of an elastic collision, a reversible collision, will look like Fig. 16-2(a): all the |
arrows are the same length, all the speeds are equal. We shall suppose that such |
--- Trang 313 --- |
collisions can always be arranged, that any angle Ø can occur, and that any speed |
could be used in such a collision. Next, we notice that this same collision can be |
viewecd diferently by turning the axes, and just for convenience we sÖø/l turn |
the axes, so that the horizontal splits i evenly, as in Fig. 16-2(b). It is the same |
collision redrawn, only with the axes turned. |
„v2 : |
œ œ x tị tị x |
tu tu '94 œ |
w 1⁄⁄v v51 |
() 1ÍŸ1 (b) |
Fig. 16-3. Two more views of the collision, from moving cars. |
Now here is the real trick: let us look at this collision from the point of view of |
someone riding along ín a car that is moving with a speed equal to the horizontal |
component of the velocity of one particle. Then how does the collision look? |
Tt looks as though particle 1 is just going straight up, because it has lost its |
horizontal component, and it comes straight down again, also because i% does |
not have that component. That is, the collision appears as shown in Fig. 16-3(a). |
Particle 2, however, was going the other way, and as we ride pastf 1% appears tO |
ñy by at some terrifc speed and at a smaller angle, but we can appreciate that |
the angles before and after the collision are the sœme. Let us denote by u the |
horizontal component of the velocity of particle 2, and by œ the vertical velocity |
of particle 1. |
Now the question is, what is the vertical velocity œtan œ? If we knew that, we |
could get the correct expression for the momentum, using the law of conservation |
of momentum in the vertical direction. Clearly, the horizontal component of the |
1mmomentum is conserved: ¡% is the same before and after the collision for both |
particles, and is zero for particle 1. So we need use the conservation law only |
for the upward velocity wutanœ. But we cøn get the upward velocity, simply by |
looking at the same collision going the other wayl If we look at the collision of |
Eig. 16-3(a) from a car moving to the left with speed ứ, we see the same collision, |
except “turned over,” as shown in Eig. 16-3(b). Ñow particle 2 is the one that goes |
up and down with speed œ, and particle 1 has picked up the horizontal speed ứ. |
--- Trang 314 --- |
Of course, now we &noœ what the velocity wœtanœ is: iE is 04/1 — w2/c2 (see |
Eq. 16.7). We know that the change in the vertical momentum of the vertically |
moving particle is |
Ap = 2m„+ |
(2, because it moves up and back down). The obliquely moving particle has a |
certain velocity ø whose components we have found to be w and +04/1 — u2/c2, |
and whose mass is m„. The change in øerf2cøl momentum of this particle is |
therefore AjÈ' = 2m„+0v/1— u2/c2 because, in accordance with our assumed |
law (16.8), the momentum component is always the mass corresponding to the |
magnitude of the velocity times the component of the velocity in the direction of |
interest. Thus in order for the total momentum to be zero the vertical momenta, |
must cancel and the ratio of the mass moving with speed ø and the mass moving |
with speed + must therefore be |
— = V1 u2/e2. (16.9) |
°U |
Let us take the limiting case that +0 is inÑnitesimal. lÝ u is very tiny indeed, it |
1s clear that ø and œ are practically equal. In this case, m„„ —> nọ and rn„ —> my. |
The grand result is |
¬ .. (16.10) |
“ v1—u?/c2 |
]t is an interesting exercise now to check whether or not Eq. (16.9) is indeed true |
for arbitrary values of +, assuming that Eq. (16.10) is the right formula for the |
mass. Note that the velocity ø needed in Eq. (16.9) can be calculated rom the |
right-angle triangle: |
0U —= uẺ + 00Ẻ(1 — u2/c2). |
Tlt will be found to check out automatically, although we used it only in the limit |
Of smaill ơi. |
Now, let us accept that momentum is conserved and that the mass depends |
upon the velocity according to (16.10) and go on to find what else we can conclude. |
Let us consider what is commonly called an ?melastic collision. For simplicity, we |
shall suppose that two objects of the same kind, moving oppositely with equal |
speeds +0, hit each other and stick together, to become some new, statlonary |
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