Journal
CLASSICAL AND QUANTUM GRAVITY
Volume 33, Issue 17, Pages -Publisher
IOP Publishing Ltd
DOI: 10.1088/0264-9381/33/17/174001
Keywords
black holes; general relativity; observations of black holes; gravitational waves; tests of general relativity
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Funding
- European Union's H2020 ERC Consolidator Grant 'Matter and strong-field gravity: New frontiers in Einstein's theory' grant [MaGRaTh-646597]
- FCT [SFRH/BSAB/105955/2014]
- Government of Canada through Industry Canada
- Province of Ontario through Ministry of Economic Development Innovation
- H2020-MSCA-RISE Grant [StronGrHEP-690904]
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Black holes (BHs) in general relativity (GR) are very simple objects. This property, that goes under the name of 'no-hair', has been refined in the last few decades and admits several versions. The simplicity of BHs makes them ideal testbeds of fundamental physics and of GR itself. Here we discuss the no-hair property of BHs, how it can be measured in the electromagnetic or gravitational window, and what it can possibly tell us about our Universe.
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