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Classical black holes contain a singularity at their core.
1902
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M. Visser, “Wormholes, Baby Universes and Causality,” Phys. Rev. D 41
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M. Visser, “Lorentzian Wormholes: From Einstein to Hawking”, AIP press [now Springer], New York (1995)
1995
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E. Poisson and M. Visser, “Thin shell wormholes: Linearization stability”, Phys. Rev. D 52
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1996
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P. O. Mazur and E. Mottola, “Gravitational Condensate Stars: An Alternative to Black Holes”, (2001). [ arXiv:0109035 [gr-qc]]
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N. Dadhich, S. Kar, S. Mukherji and M. Visser, “ R = 0 R=0 space-times and selfdual Lorentzian wormholes,” Phys. Rev. D 65
2002
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D. L. Wiltshire, M. Visser and S. M. Scott, The Kerr spacetime: Rotating black holes in general relativity , (Cambridge University Press, Cambridge, 2009)
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M. Visser, “Physical observability of horizons,” Phys. Rev. D 90
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X. Calmet, “Quantum Aspects of Black Holes”, Springer Int. Pub. (2015)
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H. Culetu, “Nonsingular black hole with a nonlinear electric source”, Int. J. Mod. Phys. D 24
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A. F. Ali and M. M. Khalil, “Black hole with quantum potential”, Nuc. Phys. B 909
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A. Simpson and M. Visser, “Black-bounce to traversable wormhole”, JCAP 1902
2019
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See, for example, wikipedia.org/List_of_gravitational_wave_observations for a list of current (May 2020) gravitational wave observations
2020
Closest in time.