Erik Verlinde's paper on Emergent Entropy

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SUMMARY

Erik Verlinde's discussion centers on Bekenstein's entropy formula, derived from a thought experiment involving a particle with mass m and its interaction with a black hole. The key issue arises when considering a thermal gas of particles, which presents challenges to the second law of thermodynamics due to the infinite redshift effect. Bekenstein resolves this by positing that a particle within one Compton wavelength of the black hole's horizon contributes to the black hole's mass and entropy, effectively linking mass increase to information content. This concept underpins the area law for black hole entropy.

PREREQUISITES
  • Understanding of Bekenstein's entropy formula
  • Familiarity with black hole thermodynamics
  • Knowledge of Compton wavelength and its implications
  • Basic grasp of the second law of thermodynamics
NEXT STEPS
  • Read Bekenstein's original paper on black hole entropy
  • Explore the implications of black hole thermodynamics on information theory
  • Investigate the relationship between mass, entropy, and information in quantum mechanics
  • Study the concept of infinite redshift and its effects on particle behavior near black holes
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Physicists, cosmologists, and students of theoretical physics interested in black hole thermodynamics and the intersection of entropy and information theory.

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There is one paragraph that says:
"
Our starting assumption is directly motivated by Bekenstein's original thought experiment
from which he obtained is famous entropy formula. He considered a particle with
mass m attached to a ctitious "string" that is lowered towards a black hole. Just
before the horizon the particle is dropped in. Due to the in nite redshift the mass
increase of the black hole can be made arbitrarily small, classically. If one would take a
thermal gas of particles, this fact would lead to problems with the second law of thermodynamics.
Bekenstein solved this by arguing that when a particle is one Compton
wavelength from the horizon, it is considered to be part of the black hole. Therefore,
it increases the mass and horizon area by a small amount, which he identi ed with one
bit of information. This lead him to his area law for the black hole entropy."

I don't quite understand what he meant when he gave the thermal gas example. How does it lead to problems with the second law of thermodynamics?

Also how exactly does a particle being a Compton of wavelength away from the horizon (so as becoming part of the black hole) solve the problem?
 
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you have to read Bekenstein's original paper listed in the references.
 
I was hoping I get some help just concerning this very idea without getting to read the whole paper from whom are familiar with this.
 

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