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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 |
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container_title | The European physical journal. C, Particles and fields |
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creator | Cruz, Miguel Gonzalez-Espinoza, Manuel Saavedra, Joel Vargas-Arancibia, Diego |
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 |
format | article |
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1
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1
+
1
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1
+
1
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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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