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Ultralight scalars and resonances in black-hole physics

Ultralight degrees of freedom coupled to matter lead to resonances, which can be excited when the Compton wavelength of the field equals a dynamical scale in the problem. For binaries composed of a star orbiting a supermassive black hole, these resonances lead to a smoking-gun effect: a periastron d...

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Detalles Bibliográficos
Autores principales: Fujita, Ryuichi, Cardoso, Vitor
Lenguaje:eng
Publicado: 2016
Materias:
Acceso en línea:https://dx.doi.org/10.1103/PhysRevD.95.044016
http://cds.cern.ch/record/2253213
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author Fujita, Ryuichi
Cardoso, Vitor
author_facet Fujita, Ryuichi
Cardoso, Vitor
author_sort Fujita, Ryuichi
collection CERN
description Ultralight degrees of freedom coupled to matter lead to resonances, which can be excited when the Compton wavelength of the field equals a dynamical scale in the problem. For binaries composed of a star orbiting a supermassive black hole, these resonances lead to a smoking-gun effect: a periastron distance which stalls, even in the presence of gravitational-wave dissipation. This effect, also called a floating orbit, occurs for generic equatorial but eccentric orbits, and we argue that finite-size effects are not enough to suppress it.
id oai-inspirehep.net-1501664
institution Organización Europea para la Investigación Nuclear
language eng
publishDate 2016
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spelling oai-inspirehep.net-15016642023-03-14T20:15:00Zdoi:10.1103/PhysRevD.95.044016http://cds.cern.ch/record/2253213engFujita, RyuichiCardoso, VitorUltralight scalars and resonances in black-hole physicsgr-qcGeneral Relativity and CosmologyUltralight degrees of freedom coupled to matter lead to resonances, which can be excited when the Compton wavelength of the field equals a dynamical scale in the problem. For binaries composed of a star orbiting a supermassive black hole, these resonances lead to a smoking-gun effect: a periastron distance which stalls, even in the presence of gravitational-wave dissipation. This effect, also called a floating orbit, occurs for generic equatorial but eccentric orbits, and we argue that finite-size effects are not enough to suppress it.Ultralight degrees of freedom coupled to matter lead to resonances, which can be excited when the Compton wavelength of the field equals a dynamical scale in the problem. For binaries composed of a star orbiting a supermassive black hole, these resonances lead to a smoking-gun effect: a periastron distance which {\it stalls}, even in the presence of gravitational-wave dissipation. This effect, also called a {\it floating orbit}, occurs for generic equatorial but eccentric orbits and we argue that finite-size effects are not enough to suppress it.arXiv:1612.00978oai:inspirehep.net:15016642016-12-03
spellingShingle gr-qc
General Relativity and Cosmology
Fujita, Ryuichi
Cardoso, Vitor
Ultralight scalars and resonances in black-hole physics
title Ultralight scalars and resonances in black-hole physics
title_full Ultralight scalars and resonances in black-hole physics
title_fullStr Ultralight scalars and resonances in black-hole physics
title_full_unstemmed Ultralight scalars and resonances in black-hole physics
title_short Ultralight scalars and resonances in black-hole physics
title_sort ultralight scalars and resonances in black-hole physics
topic gr-qc
General Relativity and Cosmology
url https://dx.doi.org/10.1103/PhysRevD.95.044016
http://cds.cern.ch/record/2253213
work_keys_str_mv AT fujitaryuichi ultralightscalarsandresonancesinblackholephysics
AT cardosovitor ultralightscalarsandresonancesinblackholephysics