The stochastic gravitational-wave background in the absence of horizons

DOI10.1088/1361-6382/aae1dezbMath1431.83034arXiv1805.08229OpenAlexW3101677756WikidataQ129228133 ScholiaQ129228133MaRDI QIDQ5218302

Vitor Cardoso, Richard Brito, Paolo Pani, Enrico Barausse, Irina Dvorkin

Publication date: 2 March 2020

Published in: Classical and Quantum Gravity (Search for Journal in Brave)

Full work available at URL: https://arxiv.org/abs/1805.08229

zbMATH Keywords

black holesgravitational wavesevent horizon

Mathematics Subject Classification ID

Black holes (83C57) Applications of statistics to physics (62P35) Quantization of the gravitational field (83C45) Space-time singularities, cosmic censorship, etc. (83C75) Observational and experimental questions in relativity and gravitational theory (83B05) Gravitational waves (83C35) Statistical astronomy (85A35)

Related Items (4)

On reflectivity of quantum black hole horizons ⋮ Tests for the existence of horizon through gravitational waves from a small binary in the vicinity of a massive object ⋮ On gravitational echoes from ultracompact exotic stars ⋮ Gravitational wave echoes from black hole area quantization

Cites Work

• Particle creation by black holes
• Ergosphere instability
• Gravitational collapse: The role of general relativity
• Nonviolent unitarization: basic postulates to soft quantum structure of black holes
• Black holes as bubbles of AdS
• Testing the black hole ‘no-hair’ hypothesis
• Measuring the spins of accreting black holes
• Quasinormal modes of black holes and black branes
• Where are all the gravastars? Limits upon the gravastar model from accreting black holes
• Black holes as particle detectors: evolution of superradiant instabilities
• Instability of hyper-compact Kerr-like objects
• Gravitational Collapse and Space-Time Singularities
• The fuzzball proposal for black holes: an elementary review

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