Heat of the Big Bang: Understanding CMB & Accuracy

In summary, the temperature at the start of the big bang cannot be accurately determined due to our lack of a working theory of quantum gravity. In classical models based on general relativity, the temperature approaches infinity as you approach the singularity. However, at temperatures comparable to the Planck temperature, general relativity is not expected to work well and a theory of quantum gravity is needed. The hottest temperature our universe achieved was most likely during reheating after inflation ended, but the exact temperature is uncertain due to our lack of knowledge about the field that drove inflation. It is believed that the temperature at the start of inflation was below the GUT scale, and the temperature before inflation is not relevant as there may not have been any particles present.
  • #1
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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  • #2
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.
 
  • #3
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 The Planck temperature is just where we are sure the big bang theory is no longer valid.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.
 
  • #4
Thanks bcrowell, Chalnoth, that's given me something to think about.
 
  • #5
The temperature after inflation ended had to be below the GUT scale, which is something of the order of 1029 Kelvin.
 
  • #6
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
 
  • #7
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.
 
  • #8
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).
 
  • #9
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.
 

Related to Heat of the Big Bang: Understanding CMB & Accuracy

1. What is the heat of the Big Bang?

The heat of the Big Bang refers to the intense energy and radiation generated during the birth of the universe approximately 13.8 billion years ago. This event is believed to have created the initial conditions for the universe to expand and evolve into its current state.

2. What is CMB and why is it important for understanding the Big Bang?

CMB stands for Cosmic Microwave Background, which is a faint glow of radiation that permeates the entire universe. This radiation is a remnant of the intense heat and energy released during the Big Bang and serves as a key piece of evidence for the theory. By studying the CMB, scientists can better understand the early stages of the universe and the accuracy of the Big Bang theory.

3. How is the accuracy of the Big Bang theory determined?

The accuracy of the Big Bang theory is determined by comparing its predictions and explanations to observed data, such as the CMB radiation and the distribution of galaxies in the universe. If these observations match up with the predictions of the theory, it is considered to be accurate.

4. Can the heat of the Big Bang be measured?

No, the heat of the Big Bang cannot be directly measured as it occurred billions of years ago. However, scientists can estimate the temperature of the universe at different stages of its evolution by studying the CMB radiation and other forms of radiation in the universe.

5. How does understanding the Big Bang and CMB benefit scientific research?

Understanding the Big Bang and CMB can help scientists gain a better understanding of the origin and evolution of the universe. It also allows for further research and exploration into other areas of cosmology, such as dark matter and dark energy. Additionally, studying the Big Bang and CMB can provide insights into the fundamental laws of physics and potentially lead to new discoveries and advancements in science and technology.

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