Heat of the Big Bang: Understanding CMB & Accuracy

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Discussion Overview

The discussion revolves around the temperature of the universe at the time of the Big Bang and how this can be inferred from the Cosmic Microwave Background (CMB). Participants explore theoretical models, particularly in the context of General Relativity (GR) and inflationary theory, while questioning the accuracy of temperature estimates and the implications of quantum gravity.

Discussion Character

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

Main Points Raised

  • Some participants suggest that the temperature of the universe approaches infinity as one approaches the singularity in classical models based on GR.
  • There is a consensus that GR may not be valid at temperatures near the Planck temperature, necessitating a theory of quantum gravity.
  • One viewpoint posits that the highest temperature achieved in the universe was at the end of reheating after inflation, which is linked to the energy density of the inflation field.
  • Another participant raises the question of the temperature at the start of inflation, suggesting it could be significantly higher than the temperature after inflation ended, potentially by a factor of e^65.
  • Some argue that before reheating, the temperature was effectively zero, as the inflaton field dominated the energy density.
  • Concerns are raised about the assumptions underlying inflationary theory and Grand Unified Theories (GUTs), with skepticism expressed regarding their empirical validity.
  • A participant references a paper arguing that inflationary models do not eliminate the singularity associated with the Big Bang, prompting further clarification on the nature of singularities in these models.

Areas of Agreement / Disagreement

Participants express a mix of agreement and disagreement regarding the implications of inflation on the Big Bang singularity and the validity of temperature estimates. Multiple competing views remain on the nature of the universe's temperature at various stages of its evolution, particularly concerning the start of inflation and the role of GUTs.

Contextual Notes

Limitations include the unresolved status of quantum gravity theories, the dependence on definitions of temperature in extreme conditions, and the lack of empirical evidence for certain theoretical constructs like GUTs.

wolram
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How do we know how hot the big bang was, is there some way to extrapolate back from the
CMB, if there is i would like to know how such accuracy was achieved.

Thanks.
 
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In classical models based on GR, the temperature approaches infinity as as you approach the singularity.

At temperatures comparable to the Planck temperature, we don't expect GR to work well. We need a theory of quantum gravity instead. Since we don't have a working theory of quantum gravity, we can't say much about the temperature at times earlier than the time at which the temperature was the Planck temperature.
 
bcrowell said:
In classical models based on GR, the temperature approaches infinity as as you approach the singularity.

At temperatures comparable to the Planck temperature, we don't expect GR to work well. We need a theory of quantum gravity instead. Since we don't have a working theory of quantum gravity, we can't say much about the temperature at times earlier than the time at which the temperature was the Planck temperature.
I think most expect that the big bang theory no longer describes our universe at rather lower temperatures than the Planck temperature, however. The Planck temperature is just where we are sure the big bang theory is no longer valid.

The hottest temperature our universe achieved was most likely the temperature at the end of reheating after inflation ended. That temperature, then, would be due to the energy density of the field which drive inflation being converted into thermal energy. This initial thermal energy might be thought of as the temperature of the big bang.

Unfortunately, we don't yet know the details of the field which drove inflation, so we can't be quite sure what that temperature was. I believe it had to be below the GUT temperature, however, or else our universe would be nearly all magnetic monopoles.
 
Thanks bcrowell, Chalnoth, that's given me something to think about.
 
The temperature after inflation ended had to be below the GUT scale, which is something of the order of 1029 Kelvin.
 
clamtrox said:
The temperature after inflation ended had to be below the GUT scale, which is something of the order of 1029 Kelvin.
The real hard question is "What was the temperature at the start of inflation?".

I vaguely remember reading that the temperature was higher by about e^65 times.*
Obviously, this is ridiculously hot, but not infinitely hot.

*At least the expansion is sometimes quoted as approximately 65 e-folds.

Jim Graber
 
jimgraber said:
The real hard question is "What was the temperature at the start of inflation?".

I vaguely remember reading that the temperature was higher by about e^65 times.*
Obviously, this is ridiculously hot, but not infinitely hot.

*At least the expansion is sometimes quoted as approximately 65 e-folds.

Jim Graber
Well, it's not really possible for the temperature at the start of inflation to be all that high, as you still need the inflaton to dominate the energy density to have inflation at all. Before reheating, the temperature was zero for all intents and purposes.
 
jimgraber said:
The real hard question is "What was the temperature at the start of inflation?".

I vaguely remember reading that the temperature was higher by about e^65 times.*
Obviously, this is ridiculously hot, but not infinitely hot.

*At least the expansion is sometimes quoted as approximately 65 e-folds.

Jim Graber

Inflation indeed cools the universe by a factor of e^60 or so... That's OK though. What happens when inflation ends is that the field responsible for inflation decays into hot radiation and reheats the universe.

As for before inflation, well, that doesn't really matter at all. There doesn't even need to be any particles (and thus no temperature).
 
Chalnoth said:
Unfortunately, we don't yet know the details of the field which drove inflation, so we can't be quite sure what that temperature was. I believe it had to be below the GUT temperature, however, or else our universe would be nearly all magnetic monopoles.

You seem to be assuming that inflation occurred (for which there is some evidence, but nothing definitive) and that GUTs are valid (for which there is no empirical evidence). There's a nice quote by Martin Rees about this issue: "Skeptics about exotic physics might not be hugely impressed by a theoretical argument to explain the absence of particles that are themselves only hypothetical. Preventive medicine can readily seem 100 percent effective against a disease that doesn't exist!"

If you're trying to claim that inflation removes the big bang singularity in temperature, then you're incorrect. Here is a paper on that topic: Arvind Borde, Alan H. Guth, and Alexander Vilenkin, Inflationary spacetimes are not past-complete, http://arxiv.org/abs/gr-qc/0110012
 
  • #10
bcrowell said:
If you're trying to claim that inflation removes the big bang singularity in temperature, then you're incorrect.
Right. Minimal inflation (General Relativity + effective field theory) still has a singularity in the math. But I don't think anybody believes there actually was such a singularity. I wasn't claiming that the model of inflation avoids the singularity, but rather that the singularity unlikely to have actually occurred.
 

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