Stability analysis of Schwarzschild black holes in dynamical Chern-Simons gravity

Masashi Kimura
Phys. Rev. D 98, 024048 – Published 27 July 2018

Abstract

Dynamical Chern-Simons gravity has an interesting feature that the parity violating term exists, and the coupling is determined by a dynamical scalar field. When the spacetime has spherical symmetry, the parity violating term vanishes, and then the metric of the Schwarzschild spacetime with vanishing scalar field is an exact solution of dynamical Chern-Simons gravity. The effect of the Chern-Simons coupling appears in the study of perturbation around the Schwarzschild spacetime. Due to the parity violating term, the odd parity metric perturbation and the perturbed scalar field are coupled, and the perturbed field equations take the form of the coupled system of the Schrödinger equations. We prove linear mode stability for a generic massive scalar.

  • Received 27 April 2018

DOI:https://doi.org/10.1103/PhysRevD.98.024048

© 2018 American Physical Society

Physics Subject Headings (PhySH)

Gravitation, Cosmology & Astrophysics

Authors & Affiliations

Masashi Kimura

  • CENTRA, Departamento de Física, Instituto Superior Técnico, Universidade de Lisboa, Avenida Rovisco Pais 1, 1049 Lisboa, Portugal

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Issue

Vol. 98, Iss. 2 — 15 July 2018

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