Question about relativistic collision between particles

In summary, the conversation revolves around solving an exercise involving the disintegration of a photon into an electron and a positron in the presence of an electron. The equations of conservation of energy and momentum are applied to determine the threshold energy for this disintegration to occur. The conversation also discusses the possibility of the disintegration happening in the vacuum or in the presence of an atomic core. The conversation ends with a thank you to all those who provided assistance.
  • #1
Frank Einstein
170
1

Homework Statement


Good morning-afternoon. I have been tasked with solving the next exercice; but I am unable to spot the error. Please can anyone point me in the right direction?A)Calculate the thresold energy of a photon to disintegrate in an electron and a positron in the presence of an electron.

B)Show that you can't have the former disintegration in the vacuum

C)If the disintegration happens in the presencie of an atomic core, show that it's momentum is miminal.

Consider c (light speed =1)

Homework Equations


Conservation of energy: Ei=Ef
Conservation of momentum: Pi=Pf; since the photon is a maseless particle, Pγ=Eγ

The Attempt at a Solution



A) Ei=me+Eγ. Ef=2me+(me^2+p^2)^0.5 Then, I apply conservation of energy (I eliminate me at both sides)
Eγ=me+(me^2+p^2)^0.5 Eγ-me=(me^2+p^2)^0.5 Eγ^2+me^2-2Eγme=me^2+Eγ
So I arrive to 2Eγme=0. That has to be wrong.


B) I apply conservation of momentum. Pi=Eγ. If we go th the centre of mass, Pf=0; so the conservation of momentum is violated, so the desintegration doesn't happen.

C) Same as A), but substituting the mass of the original electron with the mass of a core.

Thanks for reading

 
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  • #2
Frank Einstein said:
A) Ei=me+Eγ. Ef=2me+(me^2+p^2)^0.5 Then, I apply conservation of energy (I eliminate me at both sides)
Eγ=me+(me^2+p^2)^0.5 Eγ-me=(me^2+p^2)^0.5 Eγ^2+me^2-2Eγme=me^2+Eγ
So I arrive to 2Eγme=0. That has to be wrong.

The final state has three particles, not two. There is the original electron plus the new electron-positron pair.
 
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  • #3
I can't see my mistake; the three particles are aknowledged; Ef=2me (both of the particles formed from the photon)+(me^2+p^2)^0.5, which is the electron in whose presence the disintegration happens.
 
  • #4
Frank Einstein said:
I can't see my mistake; the three particles are aknowledged; Ef=2me (both of the particles formed from the photon)+(me^2+p^2)^0.5, which is the electron in whose presence the disintegration happens.

OK, I see now that you're trying to work in a frame where the original electron carries all of the momentum that the photon had. It doesn't appear that there's any such frame. To check this, give the new electron and positron a small component of momentum ##p## in the direction of the photon (##p## can be ##<0##), so that
$$ E_f = 2 \sqrt{ m^2 + p^2} + \sqrt{ m^2 + (E-2p)^2}.$$
In the limit that ##|p|\ll m##, you will find that ##E \approx m^2 /(2|p|)##, so we cannot take ##p\rightarrow 0##.

It is easy to get bogged down in algebra in this problem because the final momenta are not very restricted. One estimate for the threshold would be under the assumption that each of the final state particles, being of the same mass, carry the same amount of momentum ##E/3##. Another sloppy estimate is to say that ##E\ge 2 m##, but this neglects the fact that there is less energy available in the center of mass frame. I'm not quite sure what they're looking for, since there are more complicated ways to compute a threshold here as well that would take a lot of algebra.
 
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  • #5
Wouldn't the threshold be where the two electrons and positron are at rest in the center-of-momentum frame?
 
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  • #6
One of the electrons has to have more energy than the other two particles; it comes from the conservation of momentum. The original electron, at rest first, "inherits" the momentum of the photon. Since the photon is a maseless particle, it's momentum can be described as Eγ/c; since I am using natural units, c=1, so the mometum of the electron is equal to the energy of the photon.
 
  • #7
vela said:
Wouldn't the threshold be where the two electrons and positron are at rest in the center-of-momentum frame?

Ah yes, this actually gives the same answer as the equimomentum case.

Frank Einstein said:
One of the electrons has to have more energy than the other two particles; it comes from the conservation of momentum. The original electron, at rest first, "inherits" the momentum of the photon. Since the photon is a maseless particle, it's momentum can be described as Eγ/c; since I am using natural units, c=1, so the mometum of the electron is equal to the energy of the photon.

I think if you solve the problem fully, you find that the produced pair particles almost always have nonzero momentum, but that the probability is peaked around having the components of momentum transverse to the photon momentum be equal and opposite. That's beyond the scope of the problem given here though.

I would suggest that you follow vela's suggestion, but you will have to convert the initial data into the center-of-mass frame first.
 
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  • #8
Frank Einstein said:
One of the electrons has to have more energy than the other two particles; it comes from the conservation of momentum. The original electron, at rest first, "inherits" the momentum of the photon. Since the photon is a maseless particle, it's momentum can be described as Eγ/c; since I am using natural units, c=1, so the mometum of the electron is equal to the energy of the photon.
In the lab frame, it's true that at least one of the particles has to be moving to conserve momentum, but your assumption that the initial electron absorbs all of the photon's momentum isn't correct. All you can say is that the total momentum of the three resulting particles has to equal the momentum of the photon.

In the center-of-mass frame, the photon and electron approach each other with equal and opposite momenta, so the total momentum of the system is 0.
 
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  • #9
Allright; I'll try to solve the system giving some energy to the new particles.
Thak you all for your help.
 

Related to Question about relativistic collision between particles

1. What is a relativistic collision?

A relativistic collision is a type of collision that occurs between particles that are moving at speeds close to the speed of light. In this type of collision, the principles of special relativity must be taken into account to accurately describe the behavior of the particles.

2. How do you calculate the energy and momentum in a relativistic collision?

In a relativistic collision, the energy and momentum are calculated using the equations of special relativity, specifically the energy-momentum relation and the relativistic momentum equation. These equations take into account the mass, velocity, and Lorentz factor of the particles involved in the collision.

3. What is the difference between an elastic and inelastic relativistic collision?

In an elastic relativistic collision, the total kinetic energy of the particles before and after the collision remains the same. In an inelastic collision, some of the kinetic energy is converted into other forms of energy, such as heat or sound.

4. How does the mass-energy equivalence principle apply to relativistic collisions?

The mass-energy equivalence principle, as described by Einstein's famous equation E=mc², applies to relativistic collisions because it takes into account the increase in mass of a particle as it approaches the speed of light. This increase in mass results in an increase in energy, which must be accounted for in the calculations of relativistic collisions.

5. Can you give an example of a real-world application of relativistic collisions?

Relativistic collisions have many applications in the field of particle physics, where particles are accelerated to near-light speeds in colliders such as the Large Hadron Collider. These collisions allow scientists to study the behavior of particles and test the predictions of special relativity. Additionally, understanding relativistic collisions is crucial in fields such as astrophysics, where high-speed collisions between particles can occur in events such as supernovas.

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