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Recently within the context of a microscopic quantum theory, the Black Hole's Quantum N-Portrait, it was shown that continuous global symmetries are compatible with quantum black hole physics.
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W. Israel, Phys. Rev
1972
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G. ’t Hooft, A Planar Diagram Theory for Strong Interactions. Nucl.Phys. B72 (1974) 461
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S. W. Hawking, Comm. Math. Phys. 43 (1975) 199
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W. Israel, Phys. Lett. A57 (1976) 107; L. Bombelli, R. K. Koul, J. H. Lee and R. D. Sorkin, Phys. Rev. D 34, 373 (1986); M. Srednicki, Phys. Rev. Lett. 71, 666 (1993); V. P. Frolov and I. Novikov, Phys. Rev. D 48, 4545 (1993)
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G. Dvali and C. Gomez, “Black Hole’s 1/N Hair,” arXiv:1203.6575 [hep-th]
Cited in the paper.
Cited in the paper.
G. Dvali and S. N. Solodukhin, “Black Hole Entropy and Gravity Cutoff,” arXiv:0806.3976 [hep-th]
Cited in the paper.
J. D. Bekenstein, Do we understand black hole entropy?, arXiv:gr-qc/9409015
Cited in the paper.
G. Dvali and C. Gomez, Self-Completeness of Einstein Gravity, arXiv:1005.3497 [hep-th]
Cited in the paper.
2008
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2011
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