Conservation of relativistic energy, collision of particles

In summary, the conversation discusses the concept of maximum number of pions that can be created in a system, and the factors that must be considered to determine this number. These factors include the assumption of pions having zero momentum and the total energy available for particle creation. The conversation also mentions the difficulty in achieving spin-coupling in a particle collider.
  • #1
milkism
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Homework Statement
Collision of a proton and antiproton forming bunch of pions, what's the maximum amount?
Relevant Equations
$$E=\gamma mc^2$$
Question:
ed202d42a87c0599c252b5e9ff5770bd.png

With maximum do they mean that the speed of the pions is the same as the proton and an antiproton? Otherwise there will be two unknowns, and if I use both relativistic-energy and momentum conservation equations I get difficult equations.
 
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  • #2
milkism said:
With maximum do they mean that the speed of the pions is the same as the proton and an antiproton?
No reason to think that. To find the maximum number of pions, what might you assume about their speeds?
 
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  • #3
Doc Al said:
No reason to think that. To find the maximum number of pions, what might you assume about their speeds?
I have no idea 😭😥,I'm sorry.
 
  • #4
What's the total momentum of the system?
 
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  • #5
Zero.
 
  • #6
Right! So how about assuming that all the created pions have zero momentum -- all the energy goes into their rest masses.
 
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  • #7
Doc Al said:
What's the total momentum of the
Doc Al said:
Right! So how about assuming that all the created pions have zero momentum -- all the energy goes into their rest masses.
Wouldn't that be $$E=nmc^2$$, with n amount.
 
  • #8
You're given the rest mass of the pions. How much total energy does the system have to create particles with?
 
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  • #9
Doc Al said:
You're given the rest mass of the pions. How much total energy does the system have to create particles with?
3752 MeV?
 
  • #10
milkism said:
3752 MeV?
You should at least sketch out why you think that. You're right, but you may have made two cancelling mistakes.

So how many pions can you get from that?
 
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  • #11
Ibix said:
You should at least sketch out why you think that. You're right, but you may have made two cancelling mistakes.

So how many pions can you get from that?
Using $$E=\gamma mc^2$$, calculating the Lorentz factor with the given velocity will be 2, so E becomes 2mc², but because both proton and antiproton have same mass and velocity, the total energy will be 4mc², that's how I got 3752 MeV.
So we have 3752 = nmc² = > 3752 MeV= n *134 MeV => 28 pions.
If the pions had the same velocity as the proton and antiproton it would have be 14 pions, that's what I had at first.
 
  • #12
Right.

Note that they've fudged the numbers so it comes out nice and round. The neutral pion mass is nearly 135MeV, while protons are only a bit over 938MeV. You'd need to speed your protons up a bit more to have enough energy for 28 pions.
 
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  • #13
milkism said:
So we have 3752 = nmc² = > 3752 MeV= n *134 MeV => 28 pions.

Good! (Thanks for jumping in, @Ibix -- I got called away.)
 
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  • #14
Doc Al said:
Thanks for jumping in, @Ibix -- I got called away.
Thanks for not saying "butting in". 😁
 
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  • #15
Doc Al said:
What's the total momentum of the system?
Of course, the proton-antiproton pair must be spin-coupled in the singlet state to conserve angular momentum as well. That might be a bit tricky to achieve in a particle collider.
 
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  • #16
kuruman said:
Of course, the proton-antiproton pair must be spin-coupled in the singlet state to conserve angular momentum as well. That might be a bit tricky to achieve in a particle collider.
Indeed. For the purpose of this exercise I think those worries can be ignored. :wink:
 
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1. What is the conservation of relativistic energy?

The conservation of relativistic energy is a fundamental principle in physics that states that the total energy of a closed system remains constant over time. This means that energy cannot be created or destroyed, but can only be transformed from one form to another. In the context of collisions between particles, this principle applies to the total energy of the particles before and after the collision.

2. How does the conservation of relativistic energy apply to collisions of particles?

In collisions between particles, the total energy of the particles before the collision (known as the initial energy) must be equal to the total energy after the collision (known as the final energy). This means that the sum of the kinetic energy and potential energy of the particles before the collision must be equal to the sum of their kinetic energy and potential energy after the collision.

3. What is the equation for calculating relativistic energy in a collision?

The equation for calculating relativistic energy in a collision is E = mc2, where E is the total energy, m is the mass of the particle, and c is the speed of light. This equation takes into account the mass-energy equivalence principle, which states that mass and energy are two forms of the same thing and can be converted into one another.

4. How does the conservation of relativistic energy relate to special relativity?

The conservation of relativistic energy is a fundamental principle of special relativity, which is a theory that describes how energy and mass are related at high speeds. In special relativity, the total energy of a particle is not just its kinetic energy, but also includes its rest mass energy (E = mc2). This means that the conservation of energy must take into account both forms of energy in a collision between particles.

5. Are there any exceptions to the conservation of relativistic energy?

The conservation of relativistic energy is a fundamental principle in physics and has been extensively tested and verified through experiments. However, there are some situations where it may not hold true, such as in the presence of strong gravitational fields or in certain quantum mechanical processes. In these cases, other principles and equations must be taken into account to accurately describe the conservation of energy.

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