Hawking radiation / String Hagedorn temperature?

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Discussion Overview

The discussion revolves around the relationship between Hawking radiation and the Hagedorn temperature in string theory, exploring whether the similarity in their magnitudes is coincidental or indicative of a deeper connection. Participants examine the implications of these temperatures in the context of black hole formation and phase transitions in high-energy physics.

Discussion Character

  • Exploratory
  • Technical explanation
  • Debate/contested

Main Points Raised

  • One participant notes that the equivalent temperature for Hawking radiation from a Planck mass black hole is approximately 5×1030 K, while the Hagedorn temperature is around 1030 K, suggesting a potential connection.
  • Another participant questions how the Hagedorn temperature was calculated and proposes various models (e.g., D9 Brane/Antibrane, AdS Atick-Witten theory) that could be relevant.
  • Some participants assert that the similarity in temperatures is not a coincidence and relates to the order of Planck energy, although there is disagreement on the exact relationship and calculations involved.
  • One participant highlights that actual calculations introduce additional factors that can alter the expected values, leading to temperatures that are two orders of magnitude smaller than the Planck energy.
  • There is a discussion about the relationship between the Hagedorn temperature and the self-dual radius, with some participants agreeing that it is reasonable to expect the Hagedorn temperature to be on the order of the Planck temperature.

Areas of Agreement / Disagreement

Participants express differing views on whether the similarity in temperatures is coincidental or indicative of a deeper physical connection. Some assert it is not a coincidence, while others question the calculations and interpretations involved, indicating that the discussion remains unresolved.

Contextual Notes

Participants express uncertainty regarding the calculations of the Hagedorn temperature and its relationship to Hawking radiation, highlighting the complexity and potential dependencies on various theoretical models.

TeethWhitener
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I was playing around with numbers and found that the equivalent temperature for Hawking radiation from a Planck mass black hole is ~5×1030 K. Later, I saw that the Hagedorn temperature for strings (where the partition function is expected to diverge) is reported to be around ~1030 K. I thought "wow this is a really intriguing coincidence!" and then I started to wonder whether it's actually a coincidence. It could be that the string Hagedorn temperature demarcates a phase transition from "ordinary" matter to stringy black hole matter at sufficient energy density. If so, that (in my opinion) would mark a plausible and fairly impressive quantum-ish explanation of how black holes are formed.

Since I don't really know how the Hagedorn temperature was calculated, my question is this: Is it a coincidence? Or does this aspect of string theory actually predict a phase transition at the same order of magnitude that you would expect quantum effects to dominate a gravitational system (Hawking radiation from a Planck mass black hole)? Or is it a sleight of hand: maybe string theorists used what they know about Hawking radiation to come up with a plausible value for the Hagedorn temperature (which might give an estimate for some other parameter--such as string tension--that they'd like to know)?

A note: I have an advanced degree (in chemical physics), but I know nothing about string theory other than the pop-sci stuff, which is why I marked the thread "Basic." Be gentle :)
 
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A very good question. I don't know it too. Never calculated anything like this with numbers. And the question would be how? And with what kind of model?
D9 Brane/Antibrane? Axion dilaton field with axion hair? AdS Atick-Witten theory? Instanton D field? ...
I think there will be a difference between Superstringtheory and M theory. But which and why, I don't know too.
Would be really interesting to get to know this. But we have some String Cracks here, who might help
 
That's not coincidence. They are both of the order of Planck energy (divided by Boltzmann constant).

Since you are a chemical physicist, it may be illuminating for you to know that Planck distance (namely, inverse Planck energy times ##\hbar c##) is for gravity and string theory what Bohr radius is for chemistry and atomic theory.
 
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Demystifier said:
That's not coincidence. They are both of the order of Planck energy (divided by Boltzmann constant).
At least from what I've seen, they're both 2 orders of magnitude less than the Planck energy. To me, this isn't really "of the order of Planck energy." That's why I'm wondering how the string Hagedorn temperature was estimated.
 
TeethWhitener said:
At least from what I've seen, they're both 2 orders of magnitude less than the Planck energy.
When one performs actual calculations, one gets additional factors such as
$$\frac{E_{Planck}}{(4\pi)^2}$$
In this way one easily gets a result which is two orders magnitude smaller, despite the fact that the relevant energy is still the Planck energy ##E_{Planck}##.
 
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So basically, since the Hagedorn temperature is related to the self-dual radius, and since we choose the self-dual radius to be on the order of the Planck length, the Hagedorn temperature will be on the order of the Planck temperature? Is that somewhat right?
 
TeethWhitener said:
So basically, since the Hagedorn temperature is related to the self-dual radius, and since we choose the self-dual radius to be on the order of the Planck length, the Hagedorn temperature will be on the order of the Planck temperature? Is that somewhat right?
Yes.
 
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Demystifier said:
Yes.
Excellent, thanks for your help!
 

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