Do cosmologists take spontaneous symmetry breaking seriously?

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SUMMARY

Cosmologists take spontaneous symmetry breaking (SSB) seriously, particularly in the context of the early Universe, where it is likened to a second-order phase transition. Vacuum energy is generally considered to have a negligible effect on cosmic expansion, although its precise nature remains under investigation. There are regions of the Universe that are not causally connected to ours, suggesting that these areas may have different vacuum states. The electroweak symmetry breaking, a well-established concept in the Standard Model of particle physics, is believed to be a first-order phase transition, although discussions about its implications and the underlying physics continue to evolve.

PREREQUISITES
  • Understanding of spontaneous symmetry breaking in particle physics
  • Familiarity with the Standard Model of particle physics
  • Knowledge of phase transitions, particularly first and second-order transitions
  • Basic concepts of cosmology, including vacuum energy and the cosmological horizon
NEXT STEPS
  • Research the implications of electroweak symmetry breaking in the Standard Model
  • Explore the concept of vacuum energy and its role in cosmological expansion
  • Investigate the nature of phase transitions in quantum field theory
  • Examine current theories regarding the multiverse and its relation to spontaneous symmetry breaking
USEFUL FOR

Physicists, cosmologists, and students of theoretical physics interested in the interplay between particle physics and cosmology, particularly regarding early Universe phenomena and symmetry breaking.

  • #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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