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Assume that there exists a fundamental theory of gravity which has a fundamental length scale and which is capable of explaining black hole evolution process fully in terms of fundamental microscopic degrees of freedom.
1983
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C. R. Stephens, G. ’t Hooft and B. F. Whiting, “Black hole evaporation without information loss,” Class. Quant. Grav. 11
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R. M. Wald, “Quantum Gravity And Time Reversibility,” Phys. Rev. D 21
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E. Witten, “Anti-de Sitter space, thermal phase transition, and confinement in gauge theories,” Adv. Theor. Math. Phys. 2
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S. Kalyana Rama and B. Sathiapalan, “On the role of chaos in the AdS / CFT connection,” Mod. Phys. Lett. A 14
2000
Cited alongside, same era.
S. W. Hawking, “Information loss in black holes,” Phys. Rev. D 72
2005
Cited alongside, same era.
A. Ashtekar and M. Bojowald, “Black hole evaporation: A Paradigm,” Class. Quant. Grav. 22
2006
Cited alongside, same era.
For a review of fuzz ball picture, see e.g
2008
Cited alongside, same era.
S. D. Mathur and C. J. Plumberg, “Correlations in Hawking radiation and the infall problem,” JHEP 09
2011
Later among the works it cites.
B. Czech, K. Larjo and M. Rozali, “Black Holes as Rubik’s Cubes,” JHEP 08
2012
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2013
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2026
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