Study of Null Geodesics and their Stability in Horndeski Black Holes

Fuente: arXiv
Saved in:
Bibliographic Details
Main Authors: Carvajal, D. A., González, P. A., Olivares, Marco, Papantonopoulos, Eleftherios, Vásquez, Yerko
Format: Preprint
Published: 2025
Subjects:
Online Access:
Tags: Add Tag
No Tags, Be the first to tag this record!
_version_ 1866911104732495872
author Carvajal, D. A.
González, P. A.
Olivares, Marco
Papantonopoulos, Eleftherios
Vásquez, Yerko
author_facet Carvajal, D. A.
González, P. A.
Olivares, Marco
Papantonopoulos, Eleftherios
Vásquez, Yerko
contents We study the motion of particles in the background of a scalar-tensor theory of gravity in which the scalar field is kinetically coupled to the Einstein tensor and we present the null geodesic structure for asymptotically flat, AdS, and dS Horndeski black holes, studying the effect of the cosmological constant on the orbits. Also, we consider three classical test of the gravity in the solar system, such as, the bending of the light, the gravitational redshift, and the Shapiro time delay in order to constraint the coupling parameters of the scalar field to gravity. Calculating the Lyapunov exponent we explore the stability of these geodesics for various values of the cosmological constant.
format Preprint
id arxiv_https___arxiv_org_abs_2503_02083
institution arXiv
publishDate 2025
record_format arxiv
spellingShingle Study of Null Geodesics and their Stability in Horndeski Black Holes
Carvajal, D. A.
González, P. A.
Olivares, Marco
Papantonopoulos, Eleftherios
Vásquez, Yerko
General Relativity and Quantum Cosmology
High Energy Physics - Theory
We study the motion of particles in the background of a scalar-tensor theory of gravity in which the scalar field is kinetically coupled to the Einstein tensor and we present the null geodesic structure for asymptotically flat, AdS, and dS Horndeski black holes, studying the effect of the cosmological constant on the orbits. Also, we consider three classical test of the gravity in the solar system, such as, the bending of the light, the gravitational redshift, and the Shapiro time delay in order to constraint the coupling parameters of the scalar field to gravity. Calculating the Lyapunov exponent we explore the stability of these geodesics for various values of the cosmological constant.
title Study of Null Geodesics and their Stability in Horndeski Black Holes
topic General Relativity and Quantum Cosmology
High Energy Physics - Theory
url https://arxiv.org/abs/2503.02083