[Anti] Matter In The Early Universe - Over Complicated?

In summary, there are many models and speculations in particle physics that try to explain the observed asymmetry between matter and antimatter in the early universe. However, there are already many existing models that predict this asymmetry without modifying fundamental principles. While exotic scenarios are still being investigated, current observations and experiments have not provided evidence for the existence of antimatter galaxies or significant amounts of intergalactic antimatter.
  • #1
3CKPilot
5
0
Is it possible that particle physics is over complicating theories about why all the matter in the early universe didn't annihilate, even though equal amounts of matter and antimatter existed? Is it possible that inflation happened quickly enough that antimatter and matter were blown clear of each other, and were too far away from each other to re-attract and annihilate?
 
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  • #2
Yes, there are peculiar models in which matter and antimatter repel each other. There are even models in which matter attracts antimatter but antimatter repels matter. Many ideas, all speculations... Why would you need them if the standard model tells you there must be an asymmetry between what we call antimatter and matter ? Is it not to best investigate whether simple things which we have established can explain the observed asymmetry ? Although we do not have a general agreement on what produced this asymmetry, there are already many models predicting it without modifying fundamental principles. In any case, exotic scenarios are investigated as well, such as scalar-tensor gravitational theories, although there main motivation is not matter-antimatter asymmetry.
 
  • #3
3CKPilot said:
Is it possible that particle physics is over complicating theories about why all the matter in the early universe didn't annihilate, even though equal amounts of matter and antimatter existed? Is it possible that inflation happened quickly enough that antimatter and matter were blown clear of each other, and were too far away from each other to re-attract and annihilate?

I don't see how this would explain what we see today. If they didn't annihilate, then where ARE the other half? These antimatter of equal amount to our matter should still be around and should be plainly observed. We know how to detect them, and we can detect signatures of their presence. There should be planets made of them the same way we have for matter.

So where are they?

Zz.
 
  • #4
How do we know that say, a distant galaxy is not anti-matter? (I'm not suggesting that one is at all, just wondering what detection matters we actually have) Neutrino emissions from beta decays that shower us from that direction? I can't think of much else, maybe pion +- shower ratios or other particle shower rations from known stellar/galaxial reactions.
 
  • #5
K.J.Healey said:
How do we know that say, a distant galaxy is not anti-matter? (I'm not suggesting that one is at all, just wondering what detection matters we actually have) Neutrino emissions from beta decays that shower us from that direction? I can't think of much else, maybe pion +- shower ratios or other particle shower rations from known stellar/galaxial reactions.
As we look around us, we see many galaxies interacting with one another, including collisions that leave one another tidally distorted. If an antimatter galaxy (with intergalactic antimatter dust and gases) collided with a normal galaxy, we'd be in for a pretty big show. The absence of such observations suggests that either antimatter galaxies do not exist or (highly unlikely) that they repel galaxies made of normal matter. Experimenters at CERN intend to test the Weak Equivalence Principle using cold neutral antihydrogen to determine if the gravitational infall rates of matter and antimatter are the same. If the infall rates are not the same, that would be an interesting result.
 
  • #6
It is possible that there are antimatter galaxies very far away, and the sort of interaction that Turbo-1 describes is hard to see because it gets swallowed up in the diffuse x-ray background. However, in such a case we would expect to see anti-helium and anti-iron nuclei in primary cosmic rays, and every such for them has come up empty. These are the most stringent limits we have.
 
  • #7
The PAMELA satellite experiment (Payload for Antimatter Exploration and Light-nuclei Astrophysics) recently reported a measurement showing that the anti-proton to proton flux ratio in cosmic rays is about 2 x 10-4 .
See attached PDF.
 

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  • #8
Antiprotons are not anti-helium or anti-iron nuclei.
 
  • #9
Correct. No antihelium was seen. In fact the antiproton yield (see my reply #7) is consistent with antiproton production by very high energy (mostly ordinary proton) cosmic rays colliding with interstellar gas. So no real evidence for antigalaxies yet.
 

1. What is [Anti] Matter and how does it relate to the Early Universe?

[Anti] Matter refers to the opposing counterpart of regular matter, with the same properties but opposite charge. In the Early Universe, it is believed that there was an equal amount of matter and antimatter, but as the universe expanded and cooled, most of the antimatter annihilated with matter, leaving behind a slight excess of regular matter that formed the universe we know today.

2. Why is studying [Anti] Matter in the Early Universe important?

Understanding the properties and behavior of [Anti] Matter in the Early Universe can provide valuable insights into the fundamental laws and processes that govern our universe. It can also help us understand the origins of the universe and how it evolved.

3. How is [Anti] Matter created in the Early Universe?

In the Early Universe, [Anti] Matter was created through a process called pair production, where high-energy photons converted into matter-antimatter pairs. This process is also observed in high-energy particle collisions in modern-day particle accelerators.

4. What challenges do scientists face when studying [Anti] Matter in the Early Universe?

One of the biggest challenges is the scarcity of [Anti] Matter in the universe today, making it difficult to study and understand. Additionally, the complex interactions between matter and antimatter make it challenging to recreate and study in laboratory settings.

5. Can [Anti] Matter be used as a source of energy?

While [Anti] Matter has the potential to release a large amount of energy through annihilation with regular matter, it is currently not a viable source of energy due to the difficulty of creating and containing it. However, scientists continue to research and explore its potential uses in the future.

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