Quasinormal modes of black holes in Horndeski gravity

We study the perturbations to General Relativistic black holes (i.e. those without scalar hair) in Horndeski scalar-tensor gravity. First, we derive the equations of odd and even parity perturbations of both the metric and scalar field in the case of a Schwarzschild black hole, and show that the gra...

Full description

Bibliographic Details
Main Authors: Tattersall, O, Ferreira, P
Format: Journal article
Published: American Physical Society 2018
_version_ 1797096361869443072
author Tattersall, O
Ferreira, P
author_facet Tattersall, O
Ferreira, P
author_sort Tattersall, O
collection OXFORD
description We study the perturbations to General Relativistic black holes (i.e. those without scalar hair) in Horndeski scalar-tensor gravity. First, we derive the equations of odd and even parity perturbations of both the metric and scalar field in the case of a Schwarzschild black hole, and show that the gravitational waves emitted from such a system contain a mixture of quasi-normal mode frequencies from the usual General Relativistic spectrum and those from the new scalar field spectrum, with the new scalar spectrum characterised by just two free parameters. We then specialise to the sub-family of Horndeski theories in which gravitational waves propagate at the speed of light $c$ on cosmological backgrounds; the scalar quasi-normal mode spectrum of such theories is characterised by just a single parameter $\mu$ acting as an effective mass of the scalar field. Analytical expressions for the quasi-normal mode frequencies of the scalar spectrum in this sub-family of theories are provided for both static and slowly rotating black holes. In both regimes comparisons to quasi-normal modes calculated numerically show good agreement with those calculated analytically in this work.
first_indexed 2024-03-07T04:40:44Z
format Journal article
id oxford-uuid:d18c33df-5572-4a96-8cd0-646cc28b05b1
institution University of Oxford
last_indexed 2024-03-07T04:40:44Z
publishDate 2018
publisher American Physical Society
record_format dspace
spelling oxford-uuid:d18c33df-5572-4a96-8cd0-646cc28b05b12022-03-27T07:57:46ZQuasinormal modes of black holes in Horndeski gravityJournal articlehttp://purl.org/coar/resource_type/c_dcae04bcuuid:d18c33df-5572-4a96-8cd0-646cc28b05b1Symplectic Elements at OxfordAmerican Physical Society2018Tattersall, OFerreira, PWe study the perturbations to General Relativistic black holes (i.e. those without scalar hair) in Horndeski scalar-tensor gravity. First, we derive the equations of odd and even parity perturbations of both the metric and scalar field in the case of a Schwarzschild black hole, and show that the gravitational waves emitted from such a system contain a mixture of quasi-normal mode frequencies from the usual General Relativistic spectrum and those from the new scalar field spectrum, with the new scalar spectrum characterised by just two free parameters. We then specialise to the sub-family of Horndeski theories in which gravitational waves propagate at the speed of light $c$ on cosmological backgrounds; the scalar quasi-normal mode spectrum of such theories is characterised by just a single parameter $\mu$ acting as an effective mass of the scalar field. Analytical expressions for the quasi-normal mode frequencies of the scalar spectrum in this sub-family of theories are provided for both static and slowly rotating black holes. In both regimes comparisons to quasi-normal modes calculated numerically show good agreement with those calculated analytically in this work.
spellingShingle Tattersall, O
Ferreira, P
Quasinormal modes of black holes in Horndeski gravity
title Quasinormal modes of black holes in Horndeski gravity
title_full Quasinormal modes of black holes in Horndeski gravity
title_fullStr Quasinormal modes of black holes in Horndeski gravity
title_full_unstemmed Quasinormal modes of black holes in Horndeski gravity
title_short Quasinormal modes of black holes in Horndeski gravity
title_sort quasinormal modes of black holes in horndeski gravity
work_keys_str_mv AT tattersallo quasinormalmodesofblackholesinhorndeskigravity
AT ferreirap quasinormalmodesofblackholesinhorndeskigravity