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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
More by this author
Institution:
University of Oxford
Division:
MPLS
Department:
Physics
Sub department:
Astrophysics
Oxford college:
Oriel College
Role:
Author
More from this funder
Name:
Science and Technology Facilities Council
Funding agency for:
Tattersall, OJ
Ferreira, PG
Grant:
1804725
More from this funder
Name:
Kavli Foundation
Funding agency for:
Lagos, M
More from this funder
Name:
European Research Council
Funding agency for:
Ferreira, PG
More from this funder
Name:
Beecroft Institute of Particle Astrophysics and Cosmology
Funding agency for:
Ferreira, PG
More from this funder
Name:
Leverhulme Trust
Funding agency for:
Ferreira, PG
Publisher:
American Physical Review
Journal:
Physical Review D More from this journal
Volume:
97
Issue:
4
Pages:
1-27
Publication date:
2018-02-16
DOI:
EISSN:
2470-0029
ISSN:
2470-0010
Keywords:
Pubs id:
pubs:746949
UUID:
uuid:fa0baf02-4bb5-4440-9b23-15d4405866fc
Local pid:
pubs:746949
Source identifiers:
746949
Deposit date:
2018-01-23

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