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Notes on Relativity and Cosmology - Physics Department, UCSB

Notes on Relativity and Cosmology - Physics Department, UCSB

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6.6. DERIVING THE EXPRESSIONS 161<br />

where particle A has the same speed before as it does after, as does particle B.<br />

Also, the angle θ is the same both before <strong>and</strong> after. Such a symmetric situati<strong>on</strong><br />

must be possible unless there is an inherent breaking of symmetry in spacetime.<br />

Now, the velocity of particle A in this frame is to be slow enough that its<br />

momentum is given by the Newt<strong>on</strong>ian formula p A = m 0 v A . For c<strong>on</strong>venience, I<br />

have indicated coordinate directi<strong>on</strong>s x <strong>and</strong> y <strong>on</strong> the diagram in Alice’s reference<br />

frame. It’s velocity in the x directi<strong>on</strong> is zero, so its momentum in this directi<strong>on</strong><br />

must also be zero. Thus, particle A <strong>on</strong>ly has momentum in the y directi<strong>on</strong>. As<br />

a result, the change in the momentum of particle A is 2m 0 dy/dt, where dy/dt<br />

denotes the velocity in the y directi<strong>on</strong> after the collisi<strong>on</strong>.<br />

If momentum is to be c<strong>on</strong>served, the total vector momentum must be the<br />

same before as after. That is to say, if (in Alice’s frame of reference) we add<br />

the arrows corresp<strong>on</strong>ding to the momentum before, <strong>and</strong> the momentum after,<br />

we must get the same result:<br />

p before<br />

A<br />

p before<br />

A<br />

θ<br />

θ<br />

Total P<br />

p before<br />

B<br />

p B before<br />

For the next part of the argument notice that if, after the collisi<strong>on</strong>, we observe<br />

particle B for awhile, it will eventually hit the south wall. Let us call this event<br />

Y, where B hits the south wall after the collisi<strong>on</strong>. Recall that the collisi<strong>on</strong> takes<br />

place in the middle of the box. Event Y <strong>and</strong> the collisi<strong>on</strong> will be separated by<br />

some period of time ∆t B (as measured by Alice) <strong>and</strong> some displacement vector<br />

∆⃗x B = (∆x B , ∆y B ) in space as measured by Alice. If the box has some length<br />

2L in the north-south directi<strong>on</strong>, then since the collisi<strong>on</strong> took place in the middle,<br />

∆y B = L.<br />

Also, if we trace particle B back in time before the collisi<strong>on</strong>, then there was<br />

some event before the collisi<strong>on</strong> when it was also at the south wall. Let us call<br />

this event X, when B was at the south wall before the collisi<strong>on</strong>. By symmetry,<br />

this event will be separated from the collisi<strong>on</strong> by the same ∆t B <strong>and</strong> by −∆⃗x B .<br />

What I want you to notice, is that the displacement ∆⃗x B points in the same<br />

directi<strong>on</strong> as the momentum of particle B, since that is the directi<strong>on</strong> in which B<br />

moves. Thus, we can draw another nice right triangle:<br />

L<br />

θ<br />

∆ x B<br />

Note that this triangle has the same angle θ as the <strong>on</strong>e drawn above. As a<br />

result, we have<br />

L<br />

|∆x⃗<br />

B | = sin θ = p A<br />

|⃗p B | . (6.17)<br />

Note that, since p A has no x comp<strong>on</strong>ent, I have not bothered to represent it as

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