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Autori principali: Amarilo, K. M., Filho, M. B. Ferreira, Filho, A. A. Araújo, Reis, J. A. A. S.
Natura: Preprint
Pubblicazione: 2023
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Accesso online:https://arxiv.org/abs/2307.10937
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author Amarilo, K. M.
Filho, M. B. Ferreira
Filho, A. A. Araújo
Reis, J. A. A. S.
author_facet Amarilo, K. M.
Filho, M. B. Ferreira
Filho, A. A. Araújo
Reis, J. A. A. S.
contents This paper focuses on how the production and polarization of gravitational waves are affected by spontaneous Lorentz symmetry breaking, which is driven by a self-interacting vector field. Specifically, we examine the impact of a smooth quadratic potential and a non-minimal coupling, discussing the constraints and causality features of the linearized Einstein equation. To analyze the polarization states of a plane wave, we consider a fixed vacuum expectation value (VEV) of the vector field. Remarkably, we verify that a space-like background vector field modifies the polarization plane and introduces a longitudinal degree of freedom. In order to investigate the Lorentz violation effect on the quadrupole formula, we use the modified Green function. Finally, we show that the space-like component of the background field leads to a third-order time derivative of the quadrupole moment, and the bounds for the Lorentz-breaking coefficients are estimated as well.
format Preprint
id arxiv_https___arxiv_org_abs_2307_10937
institution arXiv
publishDate 2023
record_format arxiv
spellingShingle Gravitational waves effects in a Lorentz-violating scenario
Amarilo, K. M.
Filho, M. B. Ferreira
Filho, A. A. Araújo
Reis, J. A. A. S.
General Relativity and Quantum Cosmology
High Energy Physics - Theory
This paper focuses on how the production and polarization of gravitational waves are affected by spontaneous Lorentz symmetry breaking, which is driven by a self-interacting vector field. Specifically, we examine the impact of a smooth quadratic potential and a non-minimal coupling, discussing the constraints and causality features of the linearized Einstein equation. To analyze the polarization states of a plane wave, we consider a fixed vacuum expectation value (VEV) of the vector field. Remarkably, we verify that a space-like background vector field modifies the polarization plane and introduces a longitudinal degree of freedom. In order to investigate the Lorentz violation effect on the quadrupole formula, we use the modified Green function. Finally, we show that the space-like component of the background field leads to a third-order time derivative of the quadrupole moment, and the bounds for the Lorentz-breaking coefficients are estimated as well.
title Gravitational waves effects in a Lorentz-violating scenario
topic General Relativity and Quantum Cosmology
High Energy Physics - Theory
url https://arxiv.org/abs/2307.10937