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Scalar perturbations of two-dimensional Horava–Lifshitz black holes

In this article, we study the stability of black hole solutions found in the context of dilatonic Horava–Lifshitz gravity in 1 + 1 dimensions by means of the quasinormal modes approach. In order to find the corresponding quasinormal modes, we consider the perturbations of massive and massless scalar...

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Published in:The European physical journal. C, Particles and fields Particles and fields, 2016-02, Vol.76 (2), p.1, Article 75
Main Authors: Cruz, Miguel, Gonzalez-Espinoza, Manuel, Saavedra, Joel, Vargas-Arancibia, Diego
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description In this article, we study the stability of black hole solutions found in the context of dilatonic Horava–Lifshitz gravity in 1 + 1 dimensions by means of the quasinormal modes approach. In order to find the corresponding quasinormal modes, we consider the perturbations of massive and massless scalar fields minimally coupled to gravity. In both cases, we found that the quasinormal modes have a discrete spectrum and are completely imaginary, which leads to damping modes. For a massive scalar field and a non-vanishing cosmological constant, our results suggest unstable behavior for large values of the scalar field mass.
doi_str_mv 10.1140/epjc/s10052-016-3927-x
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subjects Analysis
Astronomy
Astrophysics and Cosmology
Black holes
Elementary Particles
Gravity (Force)
Hadrons
Heavy Ions
Measurement Science and Instrumentation
Nuclear Energy
Nuclear Physics
Physics
Physics and Astronomy
Quantum Field Theories
Quantum Field Theory
Regular Article - Theoretical Physics
String Theory
title Scalar perturbations of two-dimensional Horava–Lifshitz black holes
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