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General theories of linear gravitational perturbations to a Schwarzschild Black Hole

Abstract:

We use the covariant formulation proposed by Tattersall, Lagos, and Ferreira [Phys. Rev. D 96, 064011 (2017)] to analyze the structure of linear perturbations about a spherically symmetric background in different families of gravity theories, and hence study how quasinormal modes of perturbed black holes may be affected by modifications to general relativity. We restrict ourselves to single-tensor, scalar-tensor and vector-tensor diffeomorphism-invariant gravity models in a Schwarzschild blac...

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Publication status:
Published
Peer review status:
Peer reviewed

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Publisher copy:
10.1103/PhysRevD.97.044021

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Institution:
University of Oxford
Division:
MPLS Division
Department:
Physics; Astrophysics
Role:
Author
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Institution:
University of Oxford
Division:
MPLS
Department:
Physics
Sub department:
Astrophysics
Oxford college:
Oriel College
Role:
Author
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Funding agency for:
Tattersall, OJ
Grant:
1804725
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Funding agency for:
Ferreira, PG
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Funding agency for:
Ferreira, PG
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Publisher:
American Physical Review Publisher's website
Journal:
Physical Review D Journal website
Volume:
97
Issue:
4
Pages:
1-27
Publication date:
2018-02-16
DOI:
EISSN:
2470-0029
ISSN:
2470-0010
Source identifiers:
746949
Keywords:
Pubs id:
pubs:746949
UUID:
uuid:fa0baf02-4bb5-4440-9b23-15d4405866fc
Local pid:
pubs:746949
Deposit date:
2018-01-23

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