Black-bounce solutions in a k-essence theory under the effects of bumblebee gravity

Fuente: arXiv
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Main Authors: Pereira, Carlos F. S., Silva, Marcos V. de S., Belich, H., Rodrigues, Denis C., Fabris, Júlio C., Rodrigues, Manuel E.
Format: Preprint
Published: 2025
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_version_ 1866916780155338752
author Pereira, Carlos F. S.
Silva, Marcos V. de S.
Belich, H.
Rodrigues, Denis C.
Fabris, Júlio C.
Rodrigues, Manuel E.
author_facet Pereira, Carlos F. S.
Silva, Marcos V. de S.
Belich, H.
Rodrigues, Denis C.
Fabris, Júlio C.
Rodrigues, Manuel E.
contents In the present study, we analyze the effects of violation of Lorentz symmetry for black-bounce solutions in a $k$-essence theory that has the form of a power law for the configuration $n=1/3$. We perform such analysis for a known model explored in previous work $Σ^2=x^2+a^2$ and complement the proposal with a new black-bounce model for the area functions $Σ^2_1=\sqrt{x^4+d^4}$. This model has the Schwarzschild-de Sitter asymptomatic behavior for $x\to{-\infty}$, and we investigate the scalar field, potential, and energy conditions for both models. We have shown that the violation of Lorentz symmetry can be generated through $k$-essence without the need for an additional field. These results corroborate the validation of other previously investigated wormhole solutions.
format Preprint
id arxiv_https___arxiv_org_abs_2503_09920
institution arXiv
publishDate 2025
record_format arxiv
spellingShingle Black-bounce solutions in a k-essence theory under the effects of bumblebee gravity
Pereira, Carlos F. S.
Silva, Marcos V. de S.
Belich, H.
Rodrigues, Denis C.
Fabris, Júlio C.
Rodrigues, Manuel E.
General Relativity and Quantum Cosmology
In the present study, we analyze the effects of violation of Lorentz symmetry for black-bounce solutions in a $k$-essence theory that has the form of a power law for the configuration $n=1/3$. We perform such analysis for a known model explored in previous work $Σ^2=x^2+a^2$ and complement the proposal with a new black-bounce model for the area functions $Σ^2_1=\sqrt{x^4+d^4}$. This model has the Schwarzschild-de Sitter asymptomatic behavior for $x\to{-\infty}$, and we investigate the scalar field, potential, and energy conditions for both models. We have shown that the violation of Lorentz symmetry can be generated through $k$-essence without the need for an additional field. These results corroborate the validation of other previously investigated wormhole solutions.
title Black-bounce solutions in a k-essence theory under the effects of bumblebee gravity
topic General Relativity and Quantum Cosmology
url https://arxiv.org/abs/2503.09920