Forecast constraints on f (T) gravity with gravitational waves from compact binary coalescences

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MetadadosDescriçãoIdioma
Autor(es): dc.contributorInstituto Nacional de Pesquisas Espaciais-
Autor(es): dc.contributorUniversidade Estadual Paulista (UNESP)-
Autor(es): dc.creatorNunes, Rafael C.-
Autor(es): dc.creatorAlves, Márcio E. S. [UNESP]-
Autor(es): dc.creatorDe Araujo, José C. N.-
Data de aceite: dc.date.accessioned2022-08-04T22:08:21Z-
Data de disponibilização: dc.date.available2022-08-04T22:08:21Z-
Data de envio: dc.date.issued2022-04-28-
Data de envio: dc.date.issued2022-04-28-
Data de envio: dc.date.issued2019-09-09-
Fonte completa do material: dc.identifierhttp://dx.doi.org/10.1103/PhysRevD.100.064012-
Fonte completa do material: dc.identifierhttp://hdl.handle.net/11449/221373-
Fonte: dc.identifier.urihttp://educapes.capes.gov.br/handle/11449/221373-
Descrição: dc.descriptionThe direct detection of gravitational waves (GWs) opened a new chapter in the modern cosmology to probe possible deviations from the general relativity (GR) theory. In the present work, we investigate for the first time the modified GW form propagation from the inspiraling of compact binary systems within the context of f(T) gravity in order to obtain new forecasts/constraints on the free parameter of the theory. First, we show that the modified waveform differs from the GR waveform essentially due to induced corrections on the GWs amplitude. Then, we discuss the forecasts on the f(T) gravity assuming simulated sources of GWs as black hole binaries, neutron star binaries and black hole-neutron star binary systems, which emit GWs in the frequency band of the Advanced LIGO (aLIGO) interferometer and of the third generation Einstein Telescope (ET). We show that GW sources detected within the aLIGO sensitivity can return estimates of the same order of magnitude of the current cosmological observations. On the other hand, detection within the ET sensitivity can improve by up to 2 orders of magnitude the current bound on the f(T) gravity. Therefore, the statistical accuracy that can be achieved by future ground based GW observations, mainly with the ET detector (and planed detectors with a similar sensitivity), can allow strong bounds on the free parameter of the theory, and can be decisive to test the theory of gravitation.-
Descrição: dc.descriptionDivisão de Astrofísica Instituto Nacional de Pesquisas Espaciais, Avenida dos Astronautas 1758-
Descrição: dc.descriptionUniversidade Estadual Paulista Instituto de Ciência e Tecnologia-
Descrição: dc.descriptionUniversidade Estadual Paulista Instituto de Ciência e Tecnologia-
Idioma: dc.languageen-
Relação: dc.relationPhysical Review D-
???dc.source???: dc.sourceScopus-
Título: dc.titleForecast constraints on f (T) gravity with gravitational waves from compact binary coalescences-
Tipo de arquivo: dc.typelivro digital-
Aparece nas coleções:Repositório Institucional - Unesp

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