Detection of scalar gravitational waves with a hollow spherical antenna

We study the response and cross sections for the absorption of GW energy generated in a Jordan-Brans-Dicke theory by a resonant mass detector shaped as a hollow sphere. As a source of the GW we take a binary system in the Newtonian approximation. For masses of the stars of the order of the solar mas...

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Detalles Bibliográficos
Autores: Coccia, E. (Eugenio), Fucito, F., Lobo Gutiérrez, José Alberto, 1953-, Salvino, M.
Tipo de recurso: artículo
Estado:Versión publicada
Fecha de publicación:2000
País:España
Institución:Universidad de Barcelona
Repositorio:Dipòsit Digital de la UB
OAI Identifier:oai:diposit.ub.edu:2445/12317
Acceso en línea:https://hdl.handle.net/2445/12317
Access Level:acceso abierto
Palabra clave:Ones gravitacionals
Relativitat general (Física)
Gravitational waves
General relativity (Physics)
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spelling Detection of scalar gravitational waves with a hollow spherical antennaCoccia, E. (Eugenio)Fucito, F.Lobo Gutiérrez, José Alberto, 1953-Salvino, M.Ones gravitacionalsRelativitat general (Física)Gravitational wavesGeneral relativity (Physics)We study the response and cross sections for the absorption of GW energy generated in a Jordan-Brans-Dicke theory by a resonant mass detector shaped as a hollow sphere. As a source of the GW we take a binary system in the Newtonian approximation. For masses of the stars of the order of the solar mass, the emitted GW sweeps a range of frequencies which include the first resonant mode of the detector.The American Physical Society2000info:eu-repo/semantics/articleinfo:eu-repo/semantics/publishedVersionapplication/pdfhttps://hdl.handle.net/2445/12317Articles publicats en revistes (Física de la Matèria Condensada)reponame:Dipòsit Digital de la UBinstname:Universidad de BarcelonaInglésReproducció digital del document publicat en format paper, proporcionada per PROLA i http://dx.doi.org/10.1103/PhysRevD.62.044019Physical Review D, 2000, vol. 62, núm 4, p. 044019-1-044019-7http://dx.doi.org/10.1103/PhysRevD.62.044019(c) The American Physical Society, 2000info:eu-repo/semantics/openAccessoai:diposit.ub.edu:2445/123172026-05-27T06:46:51Z
dc.title.none.fl_str_mv Detection of scalar gravitational waves with a hollow spherical antenna
title Detection of scalar gravitational waves with a hollow spherical antenna
spellingShingle Detection of scalar gravitational waves with a hollow spherical antenna
Coccia, E. (Eugenio)
Ones gravitacionals
Relativitat general (Física)
Gravitational waves
General relativity (Physics)
title_short Detection of scalar gravitational waves with a hollow spherical antenna
title_full Detection of scalar gravitational waves with a hollow spherical antenna
title_fullStr Detection of scalar gravitational waves with a hollow spherical antenna
title_full_unstemmed Detection of scalar gravitational waves with a hollow spherical antenna
title_sort Detection of scalar gravitational waves with a hollow spherical antenna
dc.creator.none.fl_str_mv Coccia, E. (Eugenio)
Fucito, F.
Lobo Gutiérrez, José Alberto, 1953-
Salvino, M.
author Coccia, E. (Eugenio)
author_facet Coccia, E. (Eugenio)
Fucito, F.
Lobo Gutiérrez, José Alberto, 1953-
Salvino, M.
author_role author
author2 Fucito, F.
Lobo Gutiérrez, José Alberto, 1953-
Salvino, M.
author2_role author
author
author
dc.subject.none.fl_str_mv Ones gravitacionals
Relativitat general (Física)
Gravitational waves
General relativity (Physics)
topic Ones gravitacionals
Relativitat general (Física)
Gravitational waves
General relativity (Physics)
description We study the response and cross sections for the absorption of GW energy generated in a Jordan-Brans-Dicke theory by a resonant mass detector shaped as a hollow sphere. As a source of the GW we take a binary system in the Newtonian approximation. For masses of the stars of the order of the solar mass, the emitted GW sweeps a range of frequencies which include the first resonant mode of the detector.
publishDate 2000
dc.date.none.fl_str_mv 2000
dc.type.none.fl_str_mv info:eu-repo/semantics/article
info:eu-repo/semantics/publishedVersion
format article
status_str publishedVersion
dc.identifier.none.fl_str_mv https://hdl.handle.net/2445/12317
url https://hdl.handle.net/2445/12317
dc.language.none.fl_str_mv Inglés
language_invalid_str_mv Inglés
dc.relation.none.fl_str_mv Reproducció digital del document publicat en format paper, proporcionada per PROLA i http://dx.doi.org/10.1103/PhysRevD.62.044019
Physical Review D, 2000, vol. 62, núm 4, p. 044019-1-044019-7
http://dx.doi.org/10.1103/PhysRevD.62.044019
dc.rights.none.fl_str_mv (c) The American Physical Society, 2000
info:eu-repo/semantics/openAccess
rights_invalid_str_mv (c) The American Physical Society, 2000
eu_rights_str_mv openAccess
dc.format.none.fl_str_mv application/pdf
dc.publisher.none.fl_str_mv The American Physical Society
publisher.none.fl_str_mv The American Physical Society
dc.source.none.fl_str_mv Articles publicats en revistes (Física de la Matèria Condensada)
reponame:Dipòsit Digital de la UB
instname:Universidad de Barcelona
instname_str Universidad de Barcelona
reponame_str Dipòsit Digital de la UB
collection Dipòsit Digital de la UB
repository.name.fl_str_mv
repository.mail.fl_str_mv
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score 15,300719

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