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The response of a gravitating object to an external tidal field is encoded in its Love numbers, which identically vanish for classical blackholes (BHs).
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K. Skenderis, M. Taylor, “The fuzzball proposal for black holes,” Phys. Rept. 467
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T. Damour and A. Nagar, “Relativistic tidal properties of neutron stars,” Phys. Rev. D 80
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2016
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R. Brustein, A. J. M. Medved, “Black holes as collapsed polymers,” Fortsch. Phys. 65
2017
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R. Brustein and A. J. M. Medved, “Black holes as collapsed polymers,” Fortsch. Phys. 65
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2017
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2018
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2018
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R. Brustein and A. J. M. Medved, “Quantum hair of black holes out of equilibrium,” Phys. Rev. D 97
2018
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2018
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2018
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2018
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S. D. Mathur, “Resolving the black hole causality paradox,” Gen. Rel. Grav. 51
2019
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R. Brustein, A. J. M. Medved, “Non-Singular Black Holes Interiors Need Physics Beyond the Standard Model,” Fortsch. Phys. 67
2019
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2019
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2019
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2019
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