Compact objects with primary hair in shift and parity symmetric beyond Horndeski gravities

Fuente: arXiv
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Main Authors: Bakopoulos, Athanasios, Chatzifotis, Nikos, Nakas, Theodoros
Format: Preprint
Published: 2023
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author Bakopoulos, Athanasios
Chatzifotis, Nikos
Nakas, Theodoros
author_facet Bakopoulos, Athanasios
Chatzifotis, Nikos
Nakas, Theodoros
contents In this work, we delve into the model of the shift symmetric and parity-preserving Beyond Horndeski theory in all its generality. We present an explicit algorithm to extract static and spherically symmetric black holes with primary scalar charge adhering to the conservation of the Noether current emanating from the shift symmetry. We show that when the functionals $G_2$ and $G_4$ of the theory are linearly dependent, analytic homogeneous black-hole solutions exist, which can become regular by virtue of the primary charge contribution. Such geometries can easily enjoy the preservation of the Weak Energy Conditions, elevating them into healthier compact objects than most hairy black holes in modified theories of gravity. Finally, we revisit the concept of disformal transformations as a solution-generating mechanism and discuss the case of generic $G_2$ and $G_4$ functionals.
format Preprint
id arxiv_https___arxiv_org_abs_2312_17198
institution arXiv
publishDate 2023
record_format arxiv
spellingShingle Compact objects with primary hair in shift and parity symmetric beyond Horndeski gravities
Bakopoulos, Athanasios
Chatzifotis, Nikos
Nakas, Theodoros
General Relativity and Quantum Cosmology
High Energy Physics - Theory
In this work, we delve into the model of the shift symmetric and parity-preserving Beyond Horndeski theory in all its generality. We present an explicit algorithm to extract static and spherically symmetric black holes with primary scalar charge adhering to the conservation of the Noether current emanating from the shift symmetry. We show that when the functionals $G_2$ and $G_4$ of the theory are linearly dependent, analytic homogeneous black-hole solutions exist, which can become regular by virtue of the primary charge contribution. Such geometries can easily enjoy the preservation of the Weak Energy Conditions, elevating them into healthier compact objects than most hairy black holes in modified theories of gravity. Finally, we revisit the concept of disformal transformations as a solution-generating mechanism and discuss the case of generic $G_2$ and $G_4$ functionals.
title Compact objects with primary hair in shift and parity symmetric beyond Horndeski gravities
topic General Relativity and Quantum Cosmology
High Energy Physics - Theory
url https://arxiv.org/abs/2312.17198