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This problem is about relativistic collisions where particles hit each other and then their energy is converted into a new particle with a greater mass.
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First, i want to point out that this problem is similar to problems 37 and 52 in this chapter.
00:20
So in problem 37, you had two masses colliding at the same speed, but they had different masses.
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So after the collision, you have a greater mass, but some speed, v.
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So the particle isn't stationary, new particle isn't stationary after the collision.
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So why do you define mass, but you can't find mass without knowing how much of the system's momentum is in speed.
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You have to find the value of fee, find the value of m.
00:53
So in that case, you started with the conservation momentum.
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Law and then you use conservation energy so you had similar terms you substituted those into the conservation momentum expression then use that to solve for v and gamma which is really just another form of v and you would find m and these are numerical values in this case pf the final momentum of the system is not equal zero so in question 52 we instead had a stationary mass, which was an iron nucleus.
01:32
It was, so the p initial was zero.
01:38
So it emitted a photon.
01:44
So the final momentum stays the same as zero, but that means that there was a p nucleus and a p photon.
01:58
So there's a recoil effect.
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The photon is released.
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Photon has its own momentum, iron atom recoils.
02:10
But the problem is, so in that case, you start with conservation of energy.
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So you know that there's energy of the photon.
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You know there's energy of the recoil and rest mass energy.
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But the problem is that energy is coming from the original mass being decreased to a smaller mass.
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The problem is that that doesn't tell you how the energy is.
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Is split up distributed between the recoil and the photon.
02:41
And you need to use momentum conservation, where the momentum of the nucleus is, magnitude is equal to the magnitude of the photon momentum.
03:00
To use that to find the speed v and then for you, i guess, and then use the speed you to find the kinetic energy, which is what that problem is looking for.
03:09
So in general, you use conservation laws to constrain other conservation laws.
03:16
So in this problem, we have two cases.
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One is we have a stationary particle.
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These are all protons, so the mass is the same in all cases.
03:27
So i'm just going to use m without subscripts.
03:32
The second proton is stationary.
03:36
The first one comes in at some high.
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Speed or momentum.
03:42
That means after the collision, there's a new particle, greater mass, but the momentum, final momentum in the system is not equal zero.
03:52
So you need to constrain the conservation of energy equation with conservation of momentum law of relationships.
04:10
So you can find how much of the kinetic energy actually goes into increasing the mass.
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In case two, you have, again, equal and opposite direction protons colliding head -on.
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In that case, they're in the same speed.
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So the magnitudes of p1 and p2 are the same.
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So the final mass is stationary.
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So the final momentum is zero.
04:42
In this case, all of k goes into increasing.
05:00
So the point of this problem is basically to show that case two is much more efficient for creating larger mass particles because in case one, you're losing some of the energy to the final momentum of the particle because it's going to keep going in some direction.
05:20
So all that being said, in case one, it wants us to find the relationship between the final mass, rest mass energy, with the connect energy input.
05:34
So, unfortunately, these collision problems, it's all about choosing which equations to use to try to get to where you want to go.
05:45
So we're starting with conservation of energy.
05:56
So the energy of the first incoming particle is a kinetic energy plus its rest mass energy, and e2 equals just the rest mass energy because it's stationary, so it has no kinetic energy.
06:28
So we also know that in general, e squared equals p .c squared plus mc squared squared.
06:42
So this is the energy momentum equation or relationship.
06:48
So we know from this that e1 squared is p1c squared plus mc squared squared squared.
06:58
So the value of these is that they will help us use conservation of momentum relationship to constrain the momentum term.
07:13
In these energy equations.
07:24
So that would have been p2c, the whole thing squared, but the momentum of the second particle is zero.
07:31
So in case two, we're not going to be able to do that.
07:40
So ef squared is pfc squared plus mz squared squared squared.
07:50
So in this case, there actually is a final momentum of the new mass, whereas in case two, that one is going to be the one that's going to be zero.
08:00
So this one will be zero in case two, but this one up here won't be.
08:11
So one last one equation we have is just since ef equals e1 plus e2, because that's what conservation of energy is.
08:31
That means ef squared equals e1 squared plus 2, e1, e2, plus...