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We examine the idea that in quantum gravity, the entanglement entropy of a general region should be finite and the leading contribution is given by the Bekenstein-Hawking area law.
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R. Emparan, G. T. Horowitz and R. C. Myers, “Exact description of black holes on branes,” JHEP 0001
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2001
Cited alongside, same era.
S. Hawking, J. M. Maldacena and A. Strominger, “de Sitter entropy, quantum entanglement and AdS/CFT,” JHEP 0105
2001
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See, for example: S. de Haro, S. N. Solodukhin and K. Skenderis, “Holographic reconstruction of spacetime and renormalization in the AdS/CFT correspondence,” Commun. Math. Phys. 217
2002
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R. Bousso, “A Covariant entropy conjecture,” JHEP 9907
2002
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See, for example: E. P. Verlinde and H. L. Verlinde, “RG flow, gravity and the cosmological constant,” JHEP 0005
2003
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H. Casini, “Geometric entropy, area, and strong subadditivity,” Class. Quant. Grav. 21
2004
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R. C. Myers, “Higher Derivative Gravity, Surface Terms And String Theory,” Phys. Rev. D 36
2005
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2010
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2011
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2011
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2011
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2011
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R. C. Myers and A. Sinha, “Seeing a c-theorem with holography,” Phys. Rev. D 82
2011
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2011
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T. Jacobson, “Thermodynamics of space-time: The Einstein equation of state,” Phys. Rev. Lett. 75
2012
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2012
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2012
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2012
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2031
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R. C. Myers and B. Robinson, “Black Holes in Quasi-topological Gravity,” JHEP 1008
2055
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