Black Hole Entropy: Basis of Logarithm Explored

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SUMMARY

The discussion centers on the Bekenstein-Hawking entropy of black holes, which is defined as the area of the event horizon divided by 4 times the Planck length squared. Participants debate the logarithmic basis for entropy calculations, concluding that while the natural logarithm (base e) is standard in thermodynamics, base 2 may be more relevant for information theory. The role of Boltzmann's constant as a conversion factor is clarified, emphasizing that it does not change the logarithmic basis. The need for a microphysical model of black holes to fully understand these concepts is also highlighted.

PREREQUISITES
  • Understanding of Bekenstein-Hawking entropy
  • Familiarity with logarithmic functions and their bases
  • Knowledge of Boltzmann's constant and its applications
  • Basic concepts of black hole thermodynamics
NEXT STEPS
  • Research the implications of the Bousso’s Holographic Principle on black hole entropy
  • Study the relationship between entropy and temperature in black hole physics
  • Explore the significance of Hawking radiation in black hole thermodynamics
  • Examine the proposed new reference units for black hole entropy calculations
USEFUL FOR

The discussion is beneficial for physicists, astrophysicists, and students studying black hole thermodynamics, as well as anyone interested in the intersection of information theory and quantum gravity.

gerald V
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TL;DR
Which basis of the logarithm underlies the usual formula for Bekenstein-Hawking entropy?
In textbooks, Bekenstein-Hawking entropy of a black hole is given as the area of the horizon divided by 4 times the Planck length squared. But the corresponding basis of the logarithm and exponantial is not written out explicitly. Rather, one oftenly can see drawings where such elementary area is occupied by one bit of information. Thus, I would conclude that the basis of the logarithm and corresponding exponential is 2. Is this correct?

One can express the black hole entropy in vintage units simply by multiplying by Boltzmann‘s constant. In this constant, is there embedded the change of basis of the logarithm from 2 to Euler’s number ##e##?

Thank you very much in advance
 
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gerald V said:
the corresponding basis of the logarithm and exponantial is not written out explicitly.
That's because (a) nobody knows what it is, since we don't have a microphysical model of black holes that tells us what states we are coarse-graining over to obtain the Bekenstein-Hawking entropy, and (b) it doesn't really matter anyway in practical terms since the entropies obtained are so huge compared to the entropies of ordinary objects like stars with similar masses.

By convention, the base of logarithms is taken to be ##e## if it is not given explicitly. But, as I just noted, nobody really knows in this case.

gerald V said:
one oftenly can see drawings where such elementary area is occupied by one bit of information.
Nobody really knows whether that is true either. To know it, we would need to have a microphysical model of black holes, which, as above, we don't have.

gerald V said:
One can express the black hole entropy in vintage units simply by multiplying by Boltzmann‘s constant. In this constant, is there embedded the change of basis of the logarithm
No. Boltzmann's constant is just a conversion factor between energy units and temperature units.
 
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In thermodynamic discussions, the entropy is always defined with the basis ##e##. That's because the other related quantities are also defined with the ##e## basis, e.g. the Boltzmann factor ##e^{-\beta E}##. The basis ##2##, on the other hand, is more convenient when one is more interested in the information content than in the thermodynamic one.
 
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Well, the natural logarithm deals with nature, the log dualis with IT...:oldbiggrin:
 
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The basis in that reference is the natural logarithm. For the equivalent in bits, see the introduction to Bousso’s The Holographic Principle here:

https://arxiv.org/abs/hep-th/0203101
 
There is also a paper out there suggesting a new reference unit, instead of the Planck length. Such that an area of one such square unit has a limit of one bit. The linear unit is $$\frac{l_p}{\sqrt{\ln(2)}}$$
 
Hi, in fact the "exact value of the entropy of a black hole comes through the temperature defined by Hawking. Bekenstein never calculates the exact value. This entropy is build because the area of the black hole can only increase but the exact formula is not an agreement with the principal of statistical physics (kb log W). Look for the error ? Regards
 
Hi, I forget why 4 for the number of states in a Planck cellular ? Why not 1, 10 , 40. Regards
 
Is there a physical significance to logarithm bases in GR? Why not just change the base using basic log properties?
 
  • #10
geshel said:
There is also a paper out there
What paper? Please give a reference.
 
  • #11
patguy said:
the "exact value of the entropy of a black hole comes through the temperature defined by Hawking.
How? Please give a reference.

patguy said:
This entropy is build because the area of the black hole can only increase
Not if Hawking radiation exists.

patguy said:
the exact formula is not an agreement with the principal of statistical physics (kb log W).
What formula are you talking about? Please give a reference.
 
  • #12
PeterDonis said:
What paper? Please give a reference.
Yeah, should have looked it up before posting. I also misquoted it. The proposed value is twice what I wrote above, however looking at the paper again quickly there is something I'm missing. Anyway here is the paper:

http://www.lsv.fr/~dowek/Publi/planck.pdf
 

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