Do cosmologists take spontaneous symmetry breaking seriously?

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Discussion Overview

The discussion revolves around the concept of spontaneous symmetry breaking (SSB) in cosmology, particularly in relation to the early Universe, vacuum energy, and the implications for cosmological expansion. Participants explore whether SSB can be likened to phase transitions, the nature of vacuum states, and the connection between the Standard Model of particle physics and cosmology.

Discussion Character

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

Main Points Raised

  • Some participants assert that cosmologists take the idea of the vacuum state changing in the early Universe seriously, suggesting it may resemble a phase transition.
  • There is a debate about whether this phase transition is first or second order, with some suggesting it resembles a second order phase transition due to the absence of latent heat.
  • Vacuum energy is discussed as potentially having a small effect on cosmological expansion, with ongoing investigations into its precise nature.
  • Participants mention the existence of regions of the Universe that may not be causally connected to ours, raising questions about whether these regions share the same vacuum state.
  • One participant highlights a perceived language barrier regarding the terminology of SSB, specifically distinguishing electroweak symmetry breaking within the Standard Model.
  • There are differing views on whether electroweak symmetry breaking should be classified as a first or second order phase transition, with references to various academic sources for further reading.
  • Concerns are raised about the lack of mathematical proofs or consensus on the universality classes associated with electroweak SSB.

Areas of Agreement / Disagreement

Participants express a range of views on the nature of spontaneous symmetry breaking and its implications for cosmology, with no clear consensus reached regarding the order of phase transitions or the specifics of vacuum energy's role in expansion.

Contextual Notes

Some discussions involve assumptions about the nature of vacuum states and the implications of phase transitions that remain unresolved. The relationship between the Standard Model and cosmological phenomena is also under examination, with varying levels of understanding among participants.

  • #31
mfb said:
That is exactly what I said.
We see them in their earlier stages, and we have theories that predict that the galaxies are still around, but we cannot see them in their current state (13.7 Gy after the big bang).You can easily extend that example to matter a few meters behind the particle horizon. Is there matter? Well, probably. It would be extremely odd if the universe would end right at our (Earth) range of causal interaction.

I'm really not seeing your point. Evidence of past causal interaction is as good as it gets. Even light from the sun is causally removed from us by about 8 minutes, and I'm unaware of any doubts about causal connections between the Earth and sun.
 
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  • #32
mfb said:
but we cannot see them in their current state (13.7 Gy after the big bang).
This is based on a particular foliation of space-time with cosmological time determining what is "current". The coordinate independent statement is that the object at some point passes a horizon. There is nothing particularly special about your choice of "current".
 
  • #33
Chronos said:
I'm really not seeing your point. Evidence of past causal interaction is as good as it gets. Even light from the sun is causally removed from us by about 8 minutes, and I'm unaware of any doubts about causal connections between the Earth and sun.
We can test the hypothesis "the sun is still there" in 8 minutes from now.
Orodruin said:
This is based on a particular foliation of space-time with cosmological time determining what is "current".
Yes, and it should be clear from the context what I mean.Edit: I think this is getting off-topic.
 
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  • #34
Chalnoth said:
Again, you're arguing the conclusion rather than considering the models that would lead to the conclusion.

Whether or not there are different regions with different low-energy laws of physics depends upon the underlying physical laws. If there are spontaneous symmetry breaking events, such that the vacuum has either multiple metastable local minima or has a class of degenerate states, then those laws of physics generically give rise to different regions with different low-energy laws of physics.

If, on the other hand, the underlying potential is relatively steep and monatonic, so that we don't have degenerate states or many metastable local minima, and the universe we observe is right at the global minimum of the vacuum energy, then there very likely would not be any other regions of space-time with different low-energy physics.

What you're saying is that until we have evidence to point one way or the other, we should always prefer the second set of models, because it predicts a unique universe. And I'm sorry, but I really don't think that's good science.

What I am saying is that, without evidence, the hypothesis of a multiverse based on the assumption of the characteristics of this universe being determined solely by a stochastic process is not good science.

And I'm not the only one Are Parallel Universes Unscientific Nonsense? Insider Tips for Criticizing the Multiverse (Max Tegmark), Paul Steinhardt Disowns Inflation, the Theory He Helped Create (Paul Steinhardt).

As Paul says, (in the Inflation + Landscape scenario giving rise to Level II parallel universes,) with an enormously flexible Inflation theory and ~10500 varieties of String theory one can explain anything and everything - but such theories don't actually explain anything while giving the false impression that they do.

Garth
 
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  • #35
Closed pending moderation

Edit: the thread will remain closed.
 
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