Gravitational polarizability of black holes

Thibault Damour and Orchidea Maria Lecian
Phys. Rev. D 80, 044017 – Published 19 August 2009

Abstract

The gravitational polarizability properties of black holes are compared and contrasted with their electromagnetic polarizability properties. The “shape” or “height” multipolar Love numbers hl of a black hole are defined and computed. They are then compared to their electromagnetic analogs hlEM. The Love numbers hl give the height of the lth multipolar “tidal bulge” raised on the horizon of a black hole by faraway masses. We also discuss the shape of the tidal bulge raised by a test-mass m, in the limit where m gets very close to the horizon.

  • Figure
  • Received 16 June 2009

DOI:https://doi.org/10.1103/PhysRevD.80.044017

©2009 American Physical Society

Authors & Affiliations

Thibault Damour1,* and Orchidea Maria Lecian1,2,3,†

  • 1Institut des Hautes Etudes Scientifiques, 35, route de Chartres, 91440 Bures-sur-Yvette, France
  • 2APC, UMR 7164 du CNRS, Université Paris 7, 10, rue Alice Domon et Léonie Duquet, 75205 Paris Cedex 13, France
  • 3Sapienza-Università di Roma, Dipartimento di Fisica and ICRA, Piazzale Aldo Moro 5, 00185 Rome, Italy

  • *damour@ihes.fr
  • lecian@ihes.fr

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Issue

Vol. 80, Iss. 4 — 15 August 2009

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