Observing Particle Annihilation: How Anti-Particles Affect Universe Formation

In summary, pair annihilation is observed by looking at the particles that result from the annihilation. This is seen in electron-positron annihilation and is due to energy/momentum conservation. However, baryon-anti-baryon annihilation is more complex and harder to observe. The idea of antimatter galaxies is possible but difficult to test, and the concept of antimatter repelling matter is incorrect. Therefore, it is not possible for dark matter to be composed of antimatter.
  • #1
Ryanw58
6
0
How do we know/observe a particle annihilating a anti-particle?

Is it impossible to theorize that in the early universe atoms of hydrogen were as abundant as anti-hydrogen atoms yet did not annihilate each other? Instead anti-Hydrogen repelled and pushed Hydrogen together to form clumps? In this instance Protons flow towards groups and anti-protons would surround and push groups together helping them stabilize into large clumps of gas.
 
Physics news on Phys.org
  • #2
In practice, pair annihilation (one particle annihilating with its antiparticle) is observed by looking at the particles that result from the annihilation.

For example, the most common type of annhilation that happens all the time is electron-positron annihilation that occurs whenever a nucleus decays via β+ decay. In that case, you will see two 511 keV photons emitted 180 degrees apart. That is, you have e+ + e- -> γ + γ. You must have two (or more) photons due to energy/momentum conservation, and the energy of 511 keV comes from the rest mass of the electron/positron - E = mc2.

Something like baryon-anti-baryon annihilation far more complicated, as they are composite particles, and there are many available exit channels.

As to antimatter galaxies: That's possible, although your suggested mechanism for action wouldn't work. You can get antimatter "clumps" during inflation. However, such a galaxy would be very difficult to distinguish from one made of matter, so it's an idea that is reasonably difficult to test. One way to do it is to look for annihilations during supercluster mergers, as done by CHANDRA. (Another good reason to have gamma telescopes!) However, no such signatures have been observed, to my knowledge.
 
  • #3
Your concept of matter/antimatter repelling each other is exactly backwards. They have opposite charges so would ATTRACT each other.

Since antimatter has identical properties to matter other than charge, there is no possibility that dark matter could be antimatter. As just one example, antimatter would clump, exactly like matter, but dark matter does not clump.
 
  • #4
Yes I realized that, But is it possible that the antimatter with a negative charge in its nucleus could drop its positron and then repel against the negative charged electron clouds of Protons?

Or for instance if a you take a proton with 2 elections and antiproton with one positron, would the one electron annihilate the positron leaving the antiproton as a Negative charged atom repulsive to electron clouds?
 
  • #5
Ryanw58 said:
Yes I realized that, But is it possible that the antimatter with a negative charge in its nucleus could drop its positron and then repel against the negative charged electron clouds of Protons?

Or for instance if a you take a proton with 2 elections and antiproton with one positron, would the one electron annihilate the positron leaving the antiproton as a Negative charged atom repulsive to electron clouds?

Irrelevant. I say again: Since antimatter has identical properties to matter other than charge, there is no possibility that dark matter could be antimatter. As just one example, antimatter would clump, exactly like matter, but dark matter does not clump.
 

1. What is particle annihilation?

Particle annihilation is a process in which a particle and its corresponding anti-particle collide and are converted into pure energy in the form of photons. This process is governed by the laws of quantum mechanics and is a fundamental aspect of the universe's structure.

2. How does particle annihilation affect universe formation?

Particle annihilation plays a significant role in the early stages of universe formation. As the universe was expanding and cooling after the Big Bang, particles and anti-particles were constantly being created and annihilated, leaving behind a small excess of particles that eventually formed the matter we see in the universe today.

3. How do anti-particles differ from regular particles?

Anti-particles have the same mass as their corresponding particles but have opposite charges. For example, an anti-electron (positron) has the same mass as an electron but has a positive charge instead of a negative charge. When a particle and an anti-particle meet, they annihilate each other, releasing energy in the process.

4. Can we observe particle annihilation in real-time?

Particle annihilation occurs at a very small scale and at extremely high energies, making it difficult to observe directly. However, scientists have been able to indirectly observe the effects of particle annihilation through experiments and observations of high-energy collisions, such as those at the Large Hadron Collider.

5. How does particle annihilation relate to the concept of antimatter?

Antimatter is a term used to describe particles that have the same mass as regular matter but have opposite charges. Particle annihilation is a process that occurs between particles and their corresponding anti-particles. The existence of antimatter is a result of particle annihilation, as particles and anti-particles were both created in equal amounts during the Big Bang.

Similar threads

  • Electromagnetism
Replies
28
Views
2K
Replies
49
Views
3K
Replies
13
Views
2K
  • Quantum Physics
Replies
28
Views
3K
  • Special and General Relativity
2
Replies
67
Views
3K
  • Astronomy and Astrophysics
Replies
19
Views
3K
  • High Energy, Nuclear, Particle Physics
2
Replies
35
Views
7K
  • Other Physics Topics
Replies
0
Views
733
  • Quantum Interpretations and Foundations
Replies
25
Views
1K
Back
Top