What is the role of zero-momentum frame in two-photon collision processes?

Also, the rest mass of an electron is typically written as ##m## rather than ##m_0##. I think the subscript zero is used for a particle that is not at rest.In summary, the zero-momentum frame is defined as the frame in which the total momentum is zero. In this frame, the two photons have equal and opposite momenta and the energy of each photon is equal to E'. In the frame of the galaxy, the energies of the photons are related to the energies in the zero-momentum frame by a factor of Γ. The expression for energy conservation in the galaxy frame is E_{HE}E_{CMB} = (mc^2)^2, and the expression for momentum conservation in the
  • #1
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Homework Statement


attachment.php?attachmentid=58027&stc=1&d=1366394833.png



Homework Equations



Zero-momentum frame is defined as the frame in which total momentum is zero.


The Attempt at a Solution



(a) In terms of the zero momentum variables, (e1 and e1 are to distinguish the two resultant particles)

[itex] \vec{p'}_{HE} + \vec{p'}_{CBR} = \vec{p'}_{e1} + \vec{p'}_{e2} = 0 [/itex]

This says that the photons have equal and opposite momenta in the zero-momentum frame, and so do the resultant particles. So the energy of both photons is equal, say to E'.

[itex] E'_{HE} + E'_{CBR} = 2E' = E_{e1} + E_{e2} = 2m_0c^2 [/itex]

I'm not sure if this right...I think this follows from the fact that we are dealing with the minimum photon energy situation, so the resultant particles would be stationary in the zero-momentum frame. Or is this the equation for the other frame in the question? (With the energies replaced)

(b) Based on the information given,

[itex] E_{HE} = \frac{1}{\Gamma} E'_{HE} [/itex]

And similar for the CMB photons.

I'm not sure how to write energy and momentum for the resultant particles in this frame. I'm guessing I have to substitute the above photon energy into the answer of part (a). But then I still don't know the energies/momenta of the resultant particles.

Feeling very confused now! Any help would be appreciated.
 

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  • #2
(a) is right.
For (b), consider that one energy will increase, one will decrease if you switch to the frame of the galaxy.
But then I still don't know the energies/momenta of the resultant particles.
You can assume that they have the same Γ as their Γ-factor.
 
  • #3
Do I need the explicit form of the doppler factor? The only thing I can think of is that the particles are moving in opposite directions maybe. Also, If (a) is correct, is the energy conservation equation sought in (b) given by:

[itex]E_{HE}+E_{CMB} = 2\Gamma m_0 c^2[/itex]

?
 
  • #4
They move in opposite directions in the frame of the galaxy, right.
Your last equation looks good, but you will need one more to calculate ##\Gamma##.
 
  • #5
So would the energies of the resultant particles be

[itex]\Gamma m_o c^2[/itex]

and

[itex]\frac{1}{\Gamma} m_0 c^2[/itex]

?

If I have the energies in the galaxy frame, I'm not sure where exactly to put them.
 
  • #6
The energies of the electron and positron are ##\Gamma m c^2##, they have no relative velocity (at the threshold), and their rest frame is moving such that we have a factor of ##\Gamma##.
 
  • #7
Ok so an equation for the electrons in the galaxy frame would be

[itex]\Gamma m_0 c^2 = \sqrt{(m_0 c^2)^2 + (p_ec)^2}[/itex]

I still don't understand by what you mean by saying that "one energy will decrease while the other will increase". Does this refer to the photon energies?
 
  • #8
Does this refer to the photon energies?
Right.

By the way, m0=m. The index 0 is not used any more in physics, masses are always "rest masses".
 
  • #9
So is

[itex]E_{CBR} = \frac{1}{\Gamma}E'_{CBR}[/itex]

and

[itex]E_{HE} = \Gamma E'_{HE}[/itex]

?
 
  • #11
So the identity they want can proved as

[itex]E_{HE}E_{CMB} = \frac{\Gamma}{\Gamma} E'_{HE}E'_{CMB} = (mc^2)^2[/itex]

So I have got all the equation except the momentum conservation one in the galaxy frame. I guess the photon momenta can be obtained by

[itex]p_{HE} = \frac{E_{HE}}{c}[/itex]

But what about the electron momenta?
 
  • #12
Eβ=pc
I don't think you need the electron momenta in the galaxy frame.
 
  • #13
Indeed, its not needed to prove the expression, but the question asked for the two conservation expression in both frames.

By β are you referring to v/c? I was thinking of using the "mass shell" formula.
 
  • #14
By β are you referring to v/c?
Right.
I was thinking of using the "mass shell" formula.
That is equivalent to my equation.
 
  • #15
I don't see how...assuming the expression is true

[itex]E = \frac{pc}{\beta} = \sqrt{(mc^2)^2 + (pc)^2}[/itex]

I haven't really seen this anywhere.

Anyway, are the products moving in the same direction in the galaxy frame? (as neither have any momentum in the zero-momentum frame)
 
  • #16
Anyway, are the products moving in the same direction in the galaxy frame?
They are.

Using ##p=\Gamma m v##, $$E^2
= m^2c^4 + \frac{m^2v^2c^2}{1-\frac{v^2}{c^2}}
= \frac{m^2c^4(1-\beta^2)}{1-\beta^2} + \frac{m^2\beta^2c^4}{1-\beta^2}
= \frac{m^2c^4}{1-\beta^2}$$
Therefore,
$$E^2-E^2\beta^2=m^2c^4$$
or
$$E^2-m^2c^4=E^2\beta^2$$
The left side is just ##p^2c^2##. Taking the square root on both sides, we get Eβ=pc. Now I used that relation twice... there is probably some easier way to get the same result.
 
  • #17
All clear! I understand better now, and I will keep that expression in mind.

Thanks mfb!
 
  • #18
One thing to note is that the Doppler factor ##\Gamma## is not the same as the relativistic gamma factor ##\gamma = 1/\sqrt{1-\beta^2}##. So, the momentum of an electron would be written ##p = \gamma mv## rather than ##p = \Gamma mv##.
 

1. What is a two-photon collision process?

A two-photon collision process is a type of interaction between two photons, or particles of light. This occurs when two photons collide and transfer energy to each other, resulting in the creation of new particles.

2. What is the significance of a two-photon collision process?

Two-photon collision processes are important in understanding the fundamental properties of particles and their interactions. They also play a role in various fields such as quantum mechanics, high energy physics, and astrophysics.

3. How is a two-photon collision process detected?

Two-photon collision processes are typically detected through the measurement of the resulting particles or radiation produced from the collision. This can be done using specialized detectors such as particle detectors or scintillation counters.

4. What are examples of particles produced in a two-photon collision process?

Some examples of particles that can be produced in a two-photon collision process include electron-positron pairs, muon-antimuon pairs, and quark-antiquark pairs. The specific particles produced depend on the energy and properties of the colliding photons.

5. How are two-photon collision processes studied in experiments?

Scientists use various experimental techniques, such as particle accelerators and colliders, to study two-photon collision processes. These experiments allow for the manipulation and control of the colliding photons, as well as the detection and analysis of the resulting particles.

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