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H. A. Buchdahl, Phys. Rev. 116
1959
Earlier work this paper cites.
S. W. Hawking, Commun. Math. Phys. 43
1976
Earlier work this paper cites.
L. Susskind, L. Thorlacius, J. Uglum, “The Stretched horizon and black hole complementarity,” Phys. Rev. D48
1993
Earlier work this paper cites.
W. G. Unruh, Phys. Rev. D 14
1997
Earlier work this paper cites.
S. D. Mathur, “Emission rates, the correspondence principle and the information paradox,” Nucl. Phys. B 529
1998
Earlier work this paper cites.
O. Lunin and S. D. Mathur, “AdS/CFT duality and the black hole information paradox,” Nucl. Phys. B 623
2002
Earlier work this paper cites.
S. W. Hawking, Phys. Rev. D 72
2005
Earlier work this paper cites.
I. Bena and N. P. Warner, Adv. Theor. Math. Phys. 9
2005
Earlier work this paper cites.
V. Cardoso, O. J. C. Dias, J. L. Hovdebo and R. C. Myers, “Instability of non-supersymmetric smooth geometries,” Phys. Rev. D 73
2006
Earlier work this paper cites.
A. J. Amsel, D. Marolf and A. Virmani, JHEP 0804
Original
2008
Earlier work this paper cites.

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2017

Guo, Bin, Hampton, Shaun, Mathur, Samir D.

In the fuzzball paradigm the information paradox is resolved because the black hole is replaced by an object with no horizon.

One may therefore ask if observations can distinguish a traditional hole from a fuzzball.
We find: (a) It is very difficult to reflect quanta off the surface of a fuzzball, mainly because geodesics starting near the horizon radius cannot escape to infinity unless their starting direction is very close to radial.
(b) If infalling particles interact with the emerging radiation before they are engulfed by the horizon, then we say that we have a `firewall behavior'.

H. A. Buchdahl, Phys. Rev. 116
1959
Earlier work this paper cites.
S. W. Hawking, Commun. Math. Phys. 43
1976
Earlier work this paper cites.
L. Susskind, L. Thorlacius, J. Uglum, “The Stretched horizon and black hole complementarity,” Phys. Rev. D48
1993
Earlier work this paper cites.
W. G. Unruh, Phys. Rev. D 14
1997
Earlier work this paper cites.
S. D. Mathur, “Emission rates, the correspondence principle and the information paradox,” Nucl. Phys. B 529
1998
Earlier work this paper cites.
O. Lunin and S. D. Mathur, “AdS/CFT duality and the black hole information paradox,” Nucl. Phys. B 623
2002
Earlier work this paper cites.
S. W. Hawking, Phys. Rev. D 72
2005
Earlier work this paper cites.
I. Bena and N. P. Warner, Adv. Theor. Math. Phys. 9
2005
Earlier work this paper cites.
V. Cardoso, O. J. C. Dias, J. L. Hovdebo and R. C. Myers, “Instability of non-supersymmetric smooth geometries,” Phys. Rev. D 73
2006
Earlier work this paper cites.
A. J. Amsel, D. Marolf and A. Virmani, JHEP 0804
Original
2008
Earlier work this paper cites.