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Recently we have suggested that the microscopic quantum description of a black hole is an overpacked self-sustained Bose-condensate of N weakly-interacting soft gravitons, which obeys the rules of 't Hooft's large-N physics.
G. ’t Hooft, A Planar Diagram Theory for Strong Interactions. Nucl.Phys. B72 (1974) 461
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Earlier work this paper cites.
E. Witten, Baryons in the 1/n Expansion. Nucl.Phys. B160 (1979) 57
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Earlier work this paper cites.
E. Witten, in Recent Developments in Gauge Theories eds. G. ’t Hooft et. al. Plenum Press, New York and London (1980)
1980
Earlier work this paper cites.
M. W. Choptuik, Universality And Scaling In Gravitational Collapse Of A Massless Scalar Field, Phys. Rev. Lett. 70 (1993) 9. C. Gundlach, Critical phenomena in gravitational collapse, Phys. Rept. 376 (2003) 339 [arXiv:gr-qc/0210101]
2003
Cited alongside, same era.
2009
Cited alongside, same era.
G. Dvali, C. Gomez, Black Hole’s Quantum N-Portrait, arXiv:1112.3359 [hep-th]
Cited in the paper.
G. Dvali and C. Gomez, Self-Completeness of Einstein Gravity, arXiv:1005.3497 [hep-th]
Cited in the paper.
2011
Later among the works it cites.
2011
Later among the works it cites.
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