"Bekenstein-Hawking black hole entropy formula"의 두 판 사이의 차이
		
		
		
		
		
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*  black hole entropy  | *  black hole entropy  | ||
** not proportional to the volume enclosed by the event horizon  | ** not proportional to the volume enclosed by the event horizon  | ||
| − | **  proportional to the area enclosed by the event horizon  | + | **  proportional to the area enclosed by the event horizon<math>S_{BH}=\frac{A_{H}}{4}</math>  | 
*  nonzero temperature  | *  nonzero temperature  | ||
** Hawking radiation  | ** Hawking radiation  | ||
2020년 11월 13일 (금) 07:07 판
introduction
- black hole entropy
- not proportional to the volume enclosed by the event horizon
 - proportional to the area enclosed by the event horizon\(S_{BH}=\frac{A_{H}}{4}\)
 
 - nonzero temperature
- Hawking radiation
 
 
expositions
- Then I discuss Verlinde's scheme and the extent to which it gives a clear case of emergence of gravity. Finally, I give a novel derivation of the Bekenstein-Hawking black hole entropy formula based on Verlinde's scheme
 - De Haro, Sebastian. “Dualities and Emergent Gravity: AdS/CFT and Verlinde’s Scheme.” arXiv:1501.06162 [gr-Qc, Physics:hep-Th, Physics:physics], January 25, 2015. http://arxiv.org/abs/1501.06162.
 
articles
- Youngsub Yoon, Quantum corrections to the Hawking radiation spectrum, http://arxiv.org/abs/1210.8355v6
 - Hod, Shahar. “Bekenstein’s Generalized Second Law of Thermodynamics: The Role of the Hoop Conjecture.” arXiv:1511.03665 [astro-Ph, Physics:gr-Qc, Physics:hep-Th], November 11, 2015. http://arxiv.org/abs/1511.03665.
 - Astorino, Marco. “Microscopic Entropy of the Magnetised Extremal Reissner-Nordstrom Black Hole.” arXiv:1507.04347 [hep-Th], July 15, 2015. http://arxiv.org/abs/1507.04347.