Did Antimatter Annihilate Matter During the Big Bang?

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Discussion Overview

The discussion centers on the absence of equal amounts of antimatter in the universe and the implications of this asymmetry in relation to the Big Bang. Participants explore concepts related to baryogenesis, charge conservation, and various cosmological models that attempt to explain the observed matter-antimatter imbalance.

Discussion Character

  • Exploratory
  • Debate/contested
  • Technical explanation
  • Conceptual clarification

Main Points Raised

  • Some participants suggest that charge and energy conservation does not necessarily apply to the conditions at the beginning of the universe, allowing for a matter-antimatter asymmetry without violating these conservation laws.
  • Others propose that baryogenesis is the process responsible for the imbalance between baryons and antibaryons, although the exact mechanism remains unknown.
  • It is noted that the observed imbalance is on the order of one part in ten billion, which some participants argue is significant compared to current CP violation measurements.
  • Some participants reference the Dirac-Milne universe model, which posits no asymmetry between matter and antimatter, while others express skepticism about its compatibility with cosmic microwave background (CMB) observations.
  • There is a discussion about the implications of a universe composed of equal amounts of matter and antimatter, particularly regarding gravitational effects and the formation of domains that could contribute to the CMB.
  • A participant introduces a speculative idea linking baryon asymmetry to the arrow of time, suggesting that matter and antimatter universes might expand in opposite temporal directions.
  • Concerns are raised about the adequacy of existing models to explain the observed phenomena, with calls for further investigation into alternative cosmological frameworks.

Areas of Agreement / Disagreement

Participants express a range of views on the mechanisms behind the matter-antimatter asymmetry, with no consensus reached on the validity of specific models or explanations. The discussion remains unresolved regarding the implications of these theories for our understanding of the universe.

Contextual Notes

Some participants note that the existing models may not fully account for observed phenomena such as the CMB, and there are unresolved questions regarding the nature of baryon number conservation and the role of quantum chromodynamics (QCD) in mass generation.

  • #31
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The law of conservation of matter and energy does not apply to the creation of the Universe. What you are doing by assuming that there was time before the Big Bang is like saying that there is a more south point than the most South point on a circle without flipping or turning its orientation. It doesn't work that way, that's what makes the "what banged" in the Big Bang so challenging. You're idea however might work if there was a Multiverse and matter could exist between Universes. However, it is a good way to go beyond that like you did, that is what I do not like about the Big Bang.
 
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  • #32
Chalnoth said:
Honestly I think that this view fails before it even gets started for the simple reason that we know of common particles that are their own anti-particles: photons. The only way to fit photons into this pictures is to make it so that they do not generate any gravitational field at all. And making it so that photons generate no gravitational field would rather drastically alter the expansion of our universe at very early times, almost certainly resulting in dramatically different BBN predictions.
Ok, this is a very convincing point, so my scenario seems purely fictional. Even so, I have a question.
Chalnoth said:
Basically this means that anti-matter picks up a minus sign for its mass when it occurs in the gravitational force, but still has a positive value for the mass when considering acceleration.
Why "but still has a positive value for the mass when considering acceleration"? Isn't ##F=-ma## then?
Chalnoth said:
This would mean that an anti-matter universe would behave, gravitationally, exactly like a matter universe. But if you had two clumps of mass, one made of anti-matter and the other made of matter, then they would gravitationally repel one another.
Understand, thanks. So, a universe filled with with anti-matter (minus sign for the matter) wouldn't imply that the matter density is negative, right?
 
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  • #33
timmdeeg said:
Ok, this is a very convincing point, so my scenario seems purely fictional. Even so, I have a question.

Why "but still has a positive value for the mass when considering acceleration"? Isn't ##F=-ma## then?

Understand, thanks.
I did not understand the question properly, could you please paraphrase it. I also did think of it that way, until I saw that diagram in a book. However I do stress that this idea may be considered and would be considered since the fact that a multiverse exists could be a possibility, which is what your theory is based on. But that is a very good perspective to look at it.
Thanks
 
  • #34
Quds Akbar said:
The law of conservation of matter and energy does not apply to the creation of the Universe.

Similarly, 'creation' or emergence wouldn't apply in such a case. The universe would just be. (E.g. no-boundary topologies work.)

But that depends on what you mean by "the Universe". The Hot Big Bang, where matter emerged and baryogenesis happened, emerges out of inflation. If inflation is eternal and consists of a multiverse, does the term "universe" apply? And how does it work? And what would it say on matter/antimatter asymmetry?

The OP would be answered with the idea of baryogenesis and the observation that it isn't obviously wrong (and very nearly good enough as of lately).
 
  • #35
timmdeeg said:
Why "but still has a positive value for the mass when considering acceleration"? Isn't ##F=-ma## then?
Well, what you'd do is have two masses for an object: m_i and m_g. For normal matter, m_i = m_g. For anti-matter, m_g = -m_i. The inertial mass, m_i is always positive. The term m_i appears in the acceleration equation, while m_g appears in the gravitational force.

timmdeeg said:
Understand, thanks. So, a universe filled with with anti-matter (minus sign for the matter) wouldn't imply that the matter density is negative, right?
The gravitational matter density would be negative in that case, yes.
 
  • #36
Chalnoth said:
The gravitational matter density would be negative in that case, yes.
And therefore would behave like a cosmological constant, gravitationally repelling(i). But that's confusing, because as you said, an anti-matter universe shouldn't be distinguishable from a matter universe. So, perhaps (i) is wrong or anti-matter doesn't mean negative mass, or something else?
 
  • #37
timmdeeg said:
And therefore would behave like a cosmological constant, gravitationally repelling(i). But that's confusing, because as you said, an anti-matter universe shouldn't be distinguishable from a matter universe. So, perhaps (i) is wrong or anti-matter doesn't mean negative mass, or something else?
A cosmological constant acts very differently. In Newtonian terms, it's effectively like adding an extra term to the force equation:

F = G m_1 \left(-{m_2 \over r^2} + {\Lambda r \over 3}\right)

This is the force of mass 2 on mass 1 (so the cosmological constant adds a pure acceleration term of any two objects away from one another).
 
  • #38
Chalnoth said:
A cosmological constant acts very differently. In Newtonian terms, it's effectively like adding an extra term to the force equation:

F = G m_1 \left(-{m_2 \over r^2} + {\Lambda r \over 3}\right)

This is the force of mass 2 on mass 1 (so the cosmological constant adds a pure acceleration term of any two objects away from one another).
Yes, I understand, but instead had the Friedmann term ##(\rho c^2 + 3p)## in my mind. As we agreed that the gravitational matter density ##\rho## is negative, it should act repelling, like negative pressure. On the other side a cloud consisting of particles with negative gravitational mass each, should gravitate attractive due to the acceleration law (because of ##m^2##). So, there must be a severe misconception. I suspect, I can't interpret the Friedmann term in that way and it would be great, if you could help me out.
 
  • #39
timmdeeg said:
Yes, I understand, but instead had the Friedmann term ##(\rho c^2 + 3p)## in my mind. As we agreed that the gravitational matter density ##\rho## is negative, it should act repelling, like negative pressure. On the other side a cloud consisting of particles with negative gravitational mass each, should gravitate attractive due to the acceleration law (because of ##m^2##). So, there must be a severe misconception. I suspect, I can't interpret the Friedmann term in that way and it would be great, if you could help me out.
I think you'd have to re-derive that equation with the new mass concept. I'm not entirely sure how it would turn out. I think it could be done in a consistent manner, but I'm not sure.
 
  • #40
Chalnoth said:
I think you'd have to re-derive that equation with the new mass concept. I'm not entirely sure how it would turn out. I think it could be done in a consistent manner, but I'm not sure.
Or, perhaps, there is a real contradiction, revealing that the conjecture to assign a negative gravitational mass for anti-matter is unphysical.
 
  • #41
How is mass defined at the current moment?
Is it the result of attractive forces or the result of how we weigh it or perhaps of how the matter interacts with gravitation?

In case it is the result of attractive forces it will remain positive even if it is perhaps anti-matter.
In case it is the result of interactions with gravitation is will change depending on whether or not the antimatter falls towards Earth or remain still(moves away perhaps)
if it is the result of how we weigh it... Gravitation, for all the fun people out there.

Sorry if this is an unwanted reply
 
  • #42
Can we stop talking about negative gravitational mass? It's been brought up at least twice that this is a non-starter because it disagrees with data.
 
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