What is the origin of the Gibbons-Hawking temperature?

In summary, the conversation between Dr. Michio Kaku and a reader discusses the concept of Gibbons-Hawking temperature mentioned in Kaku's book "Parallel Universes". The reader asks for the full citation for the work by Lawrence Krauss and Glenn Starkman that Kaku referenced and how this temperature relates to the classical absolute zero. Kaku explains that this temperature is associated with the cosmological horizon in de Sitter spacetime and that it is not the same as absolute zero. He also notes that there is no exact formula for calculating this temperature, but it is proportional to the cosmological constant. The reader questions whether it is possible to temporarily cool something below this temperature, to which Kaku responds that it is uncertain due to
  • #1
Tim Miller
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I recently submitted the following question to Dr. Michio Kaku on his Facebook page regarding an unfamiliar concept in his book "Parallel Universes":

Dr. Kaku,

In your book "Parallel Universes", pg. 301, you mention something called the Gibbons-Hawking temperature, a theoretical low temperature limit of 10 negative log 29 degrees (is that Celsius of Kelvin?). You cited a work by Lawrence Krauss & Glenn Starkman. Can you give me the full citation for this work? Is this it: http://iopscience.iop.org/articl...? How does this relate to the absolute zero of classical physics (−273.15 °C; −459.67 °F), a theoretical point at which nearly all atomic/molecular motion ceases?
 
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  • #2
Tim Miller said:
the Gibbons-Hawking temperature, a theoretical low temperature limit of 10 negative log 29 degrees (is that Celsius of Kelvin?)

I believe this temperature (in Kelvin) is the temperature associated with the cosmological horizon due to the nonzero cosmological constant in our universe. Nothing in our universe (more precisely, in the causal patch within our cosmological horizon) can ever be at a lower temperature than this.
 
  • #3
Thanks for your reply! I'm still wondering how this number was arrived at and why scientists don't now call this number absolute zero instead of −273.15 °C / O°K.
 
  • #4
Tim Miller said:
I'm still wondering how this number was arrived at

Any horizon has a corresponding temperature associated with it. For the cosmological horizon in de Sitter spacetime, the temperature is proportional to the cosmological constant. I can't dig up an exact formula on line at the moment, but AFAIK the temperature ##10^{-29}## Kelvin is what you get when you plug the best current value for the cosmological constant in our universe into the appropriate formula.

Tim Miller said:
why scientists don't now call this number absolute zero

Because it isn't. The temperature associated with a horizon is not zero; it's positive. (Note that any time you see a temperature in physics or cosmology, it will be an absolute temperature unless it's explicitly stated otherwise, since the absolute temperature scale is the one that makes all the formulas involving temperature look simple.) The idea that absolute zero is "the lowest possible temperature" is only a heuristic; the actual physical definition is different.
 
  • #5
PeterDonis said:
I believe this temperature (in Kelvin) is the temperature associated with the cosmological horizon due to the nonzero cosmological constant in our universe. Nothing in our universe (more precisely, in the causal patch within our cosmological horizon) can ever be at a lower temperature than this.
Is that last sentence strictly true? My thought was that this temperature was similar to the CMB temperature in its impact on temperature of other bodies, and there are objects out there with temperatures lower than the CMB (e.g. the Boomerang Nebula). Nothing can stay at a lower temperature than the CMB for too long, because eventually it'll reach equilibrium. But they can definitely go below that temperature temporarily.
 
  • #6
kimbyd said:
My thought was that this temperature was similar to the CMB temperature in its impact on temperature of other bodies

I'm actually not sure whether that is true or not. If it is true, then yes, I think it would be possible to temporarily cool something below this temperature. But there might be other effects involved with the temperature associated with a horizon that are not present with the CMB.
 
  • #7
PeterDonis said:
I'm actually not sure whether that is true or not. If it is true, then yes, I think it would be possible to temporarily cool something below this temperature. But there might be other effects involved with the temperature associated with a horizon that are not present with the CMB.
The way I might imagine it could be true would be if this temperature were a fundamental property of the space-time, rather than just photons created at the horizon that fill the universe.
 
  • #8
kimbyd said:
if this temperature were a fundamental property of the space-time, rather than just photons created at the horizon that fill the universe

I'm actually not sure that either of these is a good description of the temperature associated with a horizon. We don't have a good microphysical model of how such a temperature arises, so we can't be sure.
 
  • #9
PeterDonis said:
I'm actually not sure that either of these is a good description of the temperature associated with a horizon. We don't have a good microphysical model of how such a temperature arises, so we can't be sure.
My suspicion is that ultimately, it doesn't actually matter. I'm pretty sure the universe where this temperature is relevant is an empty universe. That's a de Sitter universe, which is a stationary state. If such a universe is in a stationary state, then the finite temperature would just be an apparent temperature that has nothing to do with the underlying space-time. E.g. there would be no temperature fluctuations. This is the universe described here: https://arxiv.org/abs/1405.0298
 
  • #10
kimbyd said:
That's a de Sitter universe, which is a stationary state.

Just to be clear, the paper you linked to is a hypothesis about de Sitter spacetime; it is not a known fact about de Sitter spacetime. I don't know that the conclusions of the paper are generally accepted among physicists.
 
  • #11
PeterDonis said:
Any horizon has a corresponding temperature associated with it. For the cosmological horizon in de Sitter spacetime, the temperature is proportional to the cosmological constant. I can't dig up an exact formula on line at the moment, but AFAIK the temperature ##10^{-29}## Kelvin is what you get when you plug the best current value for the cosmological constant in our universe into the appropriate formula.
Because it isn't. The temperature associated with a horizon is not zero; it's positive. (Note that any time you see a temperature in physics or cosmology, it will be an absolute temperature unless it's explicitly stated otherwise, since the absolute temperature scale is the one that makes all the formulas involving temperature look simple.) The idea that absolute zero is "the lowest possible temperature" is only a heuristic; the actual physical definition is different.
 
  • #12
If the temperature is positive, the why is it expressed with a negative exponent?
 
  • #13
Tim Miller said:
If the temperature is positive, the why is it expressed with a negative exponent?

##10^{-29}## is greater than zero, so it's a positive number.
 
  • #14
Tim Miller said:
If the temperature is positive, the why is it expressed with a negative exponent?
Because it's less than one. E.g. ##10^{-1}=0.1##, ##10^{-4}=0.0001##.
 
  • #15
kimbyd said:
Because it's less than one. E.g. ##10^{-1}=0.1##, ##10^{-4}=0.0001##.
Thanks for the refresher. My memory is not what it used to be.
 

Related to What is the origin of the Gibbons-Hawking temperature?

What is the origin of the Gibbons-Hawking temperature?

The Gibbons-Hawking temperature is a concept in theoretical physics that was proposed by physicists Stephen Hawking and Gary Gibbons. It is related to the temperature of black holes and the concept of Hawking radiation.

Who came up with the idea of the Gibbons-Hawking temperature?

The concept was proposed by theoretical physicists Stephen Hawking and Gary Gibbons in the 1970s. They developed the idea as part of their work on black holes and the theory of quantum gravity.

What is the significance of the Gibbons-Hawking temperature?

The Gibbons-Hawking temperature is significant because it provides a theoretical framework for understanding the temperature of black holes. It also has implications for the behavior of black holes and the concept of Hawking radiation.

How is the Gibbons-Hawking temperature calculated?

The Gibbons-Hawking temperature is calculated using the surface area of the event horizon of a black hole and the fundamental constants of nature, such as the speed of light and the gravitational constant. The equation for calculating it is T = ħc^3/8πGMk, where T is the temperature, ħ is the reduced Planck constant, c is the speed of light, G is the gravitational constant, M is the mass of the black hole, and k is the Boltzmann constant.

What are the implications of the Gibbons-Hawking temperature for our understanding of black holes?

The Gibbons-Hawking temperature has significant implications for our understanding of black holes. It suggests that black holes emit thermal radiation, known as Hawking radiation, which causes them to slowly lose mass and eventually evaporate. This concept has important implications for the behavior and lifespan of black holes, and has contributed to our understanding of the thermodynamics of black holes.

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