Forecasting constraints on deviations from general relativity in f ( Q ) gravity with standard sirens
Autor(a) principal: | |
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Data de Publicação: | 2022 |
Outros Autores: | |
Tipo de documento: | Artigo |
Idioma: | eng |
Título da fonte: | Repositório Institucional da UFRGS |
Texto Completo: | http://hdl.handle.net/10183/262335 |
Resumo: | In this work, we explore how modified gravity theories based on the nonmetricity scalar, known as fðQÞ gravity, affect the propagation of gravitational waves from inspiraling of binary systems. We discuss forecast constraints on fðQÞ gravity by considering standard siren events in two contexts: (i) simulated sources of gravitational waves as black hole–neutron star binary systems, emitting in the frequency band of the third-generation detector represented by the Einstein Telescope (ET); (ii) three standard siren mock catalogs based on the merger of massive black hole binaries that are expected to be observed in the operating frequency band of the Laser Interferometer Space Antenna (LISA). We find that, within the ET sensitivity, in combination with supernova and cosmic chronometer data, it will be possible to test deviations from general relativity at < 3% accuracy in the redshift range 0 <z< 5, while the main free parameter of the theory is globally constrained at 1.6% accuracy within the same range. In light of LISA’s forecasts, combined to supernova and cosmic chronometer data, in the best scenario, we find that the main free parameter of the theory will be constrained at 1.6% accuracy up to high redshifts. Therefore, we conclude that future gravitational wave observations by ET and LISA will provide a unique way to test, with good accuracy, the nature of gravity up to very large cosmic distances. |
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D'Agostino, RoccoNunes, Rafael da Costa2023-07-19T03:38:48Z20220556-2821http://hdl.handle.net/10183/262335001166270In this work, we explore how modified gravity theories based on the nonmetricity scalar, known as fðQÞ gravity, affect the propagation of gravitational waves from inspiraling of binary systems. We discuss forecast constraints on fðQÞ gravity by considering standard siren events in two contexts: (i) simulated sources of gravitational waves as black hole–neutron star binary systems, emitting in the frequency band of the third-generation detector represented by the Einstein Telescope (ET); (ii) three standard siren mock catalogs based on the merger of massive black hole binaries that are expected to be observed in the operating frequency band of the Laser Interferometer Space Antenna (LISA). We find that, within the ET sensitivity, in combination with supernova and cosmic chronometer data, it will be possible to test deviations from general relativity at < 3% accuracy in the redshift range 0 <z< 5, while the main free parameter of the theory is globally constrained at 1.6% accuracy within the same range. In light of LISA’s forecasts, combined to supernova and cosmic chronometer data, in the best scenario, we find that the main free parameter of the theory will be constrained at 1.6% accuracy up to high redshifts. Therefore, we conclude that future gravitational wave observations by ET and LISA will provide a unique way to test, with good accuracy, the nature of gravity up to very large cosmic distances.application/pdfengPhysical Review. D, Particles and fields. Woodbury. Vol. 106, no. 12 (Dec. 2022), 124053, 11 p.GravidadeOndas gravitacionaisRelatividade geralForecasting constraints on deviations from general relativity in f ( Q ) gravity with standard sirensEstrangeiroinfo:eu-repo/semantics/articleinfo:eu-repo/semantics/publishedVersioninfo:eu-repo/semantics/openAccessreponame:Repositório Institucional da UFRGSinstname:Universidade Federal do Rio Grande do Sul (UFRGS)instacron:UFRGSTEXT001166270.pdf.txt001166270.pdf.txtExtracted Texttext/plain46152http://www.lume.ufrgs.br/bitstream/10183/262335/2/001166270.pdf.txt1004361bb7850b4f21cff0fb7a2af93fMD52ORIGINAL001166270.pdfTexto completo (inglês)application/pdf646607http://www.lume.ufrgs.br/bitstream/10183/262335/1/001166270.pdfeba90d95e493f4d0e2610e33af819b3dMD5110183/2623352023-07-20 03:35:05.555146oai:www.lume.ufrgs.br:10183/262335Repositório de PublicaçõesPUBhttps://lume.ufrgs.br/oai/requestopendoar:2023-07-20T06:35:05Repositório Institucional da UFRGS - Universidade Federal do Rio Grande do Sul (UFRGS)false |
dc.title.pt_BR.fl_str_mv |
Forecasting constraints on deviations from general relativity in f ( Q ) gravity with standard sirens |
title |
Forecasting constraints on deviations from general relativity in f ( Q ) gravity with standard sirens |
spellingShingle |
Forecasting constraints on deviations from general relativity in f ( Q ) gravity with standard sirens D'Agostino, Rocco Gravidade Ondas gravitacionais Relatividade geral |
title_short |
Forecasting constraints on deviations from general relativity in f ( Q ) gravity with standard sirens |
title_full |
Forecasting constraints on deviations from general relativity in f ( Q ) gravity with standard sirens |
title_fullStr |
Forecasting constraints on deviations from general relativity in f ( Q ) gravity with standard sirens |
title_full_unstemmed |
Forecasting constraints on deviations from general relativity in f ( Q ) gravity with standard sirens |
title_sort |
Forecasting constraints on deviations from general relativity in f ( Q ) gravity with standard sirens |
author |
D'Agostino, Rocco |
author_facet |
D'Agostino, Rocco Nunes, Rafael da Costa |
author_role |
author |
author2 |
Nunes, Rafael da Costa |
author2_role |
author |
dc.contributor.author.fl_str_mv |
D'Agostino, Rocco Nunes, Rafael da Costa |
dc.subject.por.fl_str_mv |
Gravidade Ondas gravitacionais Relatividade geral |
topic |
Gravidade Ondas gravitacionais Relatividade geral |
description |
In this work, we explore how modified gravity theories based on the nonmetricity scalar, known as fðQÞ gravity, affect the propagation of gravitational waves from inspiraling of binary systems. We discuss forecast constraints on fðQÞ gravity by considering standard siren events in two contexts: (i) simulated sources of gravitational waves as black hole–neutron star binary systems, emitting in the frequency band of the third-generation detector represented by the Einstein Telescope (ET); (ii) three standard siren mock catalogs based on the merger of massive black hole binaries that are expected to be observed in the operating frequency band of the Laser Interferometer Space Antenna (LISA). We find that, within the ET sensitivity, in combination with supernova and cosmic chronometer data, it will be possible to test deviations from general relativity at < 3% accuracy in the redshift range 0 <z< 5, while the main free parameter of the theory is globally constrained at 1.6% accuracy within the same range. In light of LISA’s forecasts, combined to supernova and cosmic chronometer data, in the best scenario, we find that the main free parameter of the theory will be constrained at 1.6% accuracy up to high redshifts. Therefore, we conclude that future gravitational wave observations by ET and LISA will provide a unique way to test, with good accuracy, the nature of gravity up to very large cosmic distances. |
publishDate |
2022 |
dc.date.issued.fl_str_mv |
2022 |
dc.date.accessioned.fl_str_mv |
2023-07-19T03:38:48Z |
dc.type.driver.fl_str_mv |
Estrangeiro info:eu-repo/semantics/article |
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article |
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publishedVersion |
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001166270 |
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http://hdl.handle.net/10183/262335 |
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eng |
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Physical Review. D, Particles and fields. Woodbury. Vol. 106, no. 12 (Dec. 2022), 124053, 11 p. |
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