Black Holes and Superradiant Instabilities
Superradiant amplification lends itself to extraction of energy from BHs, but can also be looked at as the chief cause of a number of important instabilities in BH spacetimes. Some of these instabilities lead to hairy BH solutions, whereas others extract
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Richard Brito · Vitor Cardoso · Paolo Pani
Superradiance New Frontiers in Black Hole Physics Second Edition
Lecture Notes in Physics Volume 971 Founding Editors Wolf Beiglböck, Heidelberg, Germany Jürgen Ehlers, Potsdam, Germany Klaus Hepp, Zürich, Switzerland Hans-Arwed Weidenmüller, Heidelberg, Germany Series Editors Matthias Bartelmann, Heidelberg, Germany Roberta Citro, Salerno, Italy Peter Hänggi, Augsburg, Germany Morten Hjorth-Jensen, Oslo, Norway Maciej Lewenstein, Barcelona, Spain Angel Rubio, Hamburg, Germany Manfred Salmhofer, Heidelberg, Germany Wolfgang Schleich, Ulm, Germany Stefan Theisen, Potsdam, Germany James D. Wells, Ann Arbor, MI, USA Gary P. Zank, Huntsville, AL, USA
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Richard Brito • Vitor Cardoso • Paolo Pani
Superradiance New Frontiers in Black Hole Physics Second Edition
Richard Brito Department of Physics Sapienza University of Rome Rome, Italy
Vitor Cardoso Instituto Superior Técnico University of Lisbon Lisbon, Portugal
Paolo Pani Department of Physics Sapienza University of Rome Rome, Italy
ISSN 0075-8450 ISSN 1616-6361 (electronic) Lecture Notes in Physics ISBN 978-3-030-46621-3 ISBN 978-3-030-46622-0 (eBook) https://doi.org/10.1007/978-3-030-46622-0 © The Editor(s) (if applicable) and The Author(s), under exclusive licence to Springer Nature Switzerland AG 2015, 2020 This work is subject to copyright. All rights are solely and exclusively licensed by the Publisher, whether the whole or par
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