Pair Production in Empty Space

In summary, the creation of electrons and quarks in the early universe is not related to pair production, which requires a nucleus or other particles. Instead, it is believed that a baryon asymmetry was created through thermal equilibrium and interactions between photons and fermions in the early universe. The exact process is still unknown, but it is theorized that it may have involved other particles besides a nucleus. Pair production from two photons has been observed in colliders, but in the early universe, it was mainly due to interactions between photons and fermions.
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Arman777
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I am not sure this question has been asked here before but I am curious about it. From the Modern Physics Course, I learned that we need a nucleus to create an electron and positron pair (with a photon). And the reason is stated as to conserve linear momentum. If this is the case then how the electrons or quarks created in the early universe?

Is it because in the near-nucleus case we have 1 photon that is creating 2-pairs and in the early universe we can have 2 photons so that there's no need a nucleus or there's something else?
 
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Arman777 said:
And the reason is stated as to conserve linear momentum.
Truth with modification. The reason is conservation of squared total 4-momentum, i.e., com energy.

Arman777 said:
If this is the case then how the electrons or quarks created in the early universe?
This has nothing to do with pair production. If it did there would be equal amounts of quarks and antiquarks, etc. Instead, you need to create a baryon asymmetry. We don't know how that happened, but there are some theories.

In the early universe, photons and fermions were at thermal equilibrium. Mainly due to 2-to-2 scatters. There was almost as much antimatter as matter. As the universe cooled down, the symmetric component annihilated away, leaving just the asymmetric component as surplus matter.
 
  • #3
Arman777 said:
Is it because in the near-nucleus case we have 1 photon that is creating 2-pairs and in the early universe we can have 2 photons so that there's no need a nucleus or there's something else?
That is a possible process, but there were also other particles around. It doesn't have to be a nucleus, a quark in a quark gluon plasma does the job as well, for example.

Pair production from two photons has been observed in colliders, by the way.
 
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Pair production in the early universe was essentially photon-photon interaction. (Note mfb comment).
 
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I see now, thanks all
 

1. What is pair production in empty space?

Pair production in empty space is a process in which a high-energy photon spontaneously transforms into a particle and its antiparticle in a vacuum. This process is governed by the laws of quantum mechanics and is a fundamental phenomenon in particle physics.

2. How does pair production occur in empty space?

Pair production occurs when a high-energy photon interacts with the electric field of a nucleus or an atom. The photon's energy is converted into the mass of the particle-antiparticle pair, which then separates and moves away from each other in opposite directions.

3. What particles can be produced in pair production?

In theory, any type of particle and its antiparticle can be produced in pair production. However, the most commonly produced particles are electrons and positrons due to their relatively low mass and high stability.

4. What is the significance of pair production in empty space?

Pair production is significant because it provides evidence for the existence of antimatter and confirms the principles of quantum mechanics. It also plays a crucial role in particle accelerators and other high-energy experiments.

5. Can pair production occur in the absence of an external electric field?

No, pair production cannot occur in the absence of an external electric field. The energy required for the production of the particle-antiparticle pair must come from the electric field of a nucleus or an atom. In a completely empty space, there is no electric field present to provide the necessary energy.

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