- 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...
Expand abstract - Publication status:
- Published
- Peer review status:
- Peer reviewed
- Version:
- Accepted manuscript
- Files:
-
-
(pdf, 441.7KB)
-
- Publisher copy:
- 10.1103/PhysRevD.97.044021
-
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- Funding agency for:
- Tattersall, OJ
- Funding agency for:
- Ferreira, PG
- Publisher:
- American Physical Review Publisher's website
- Journal:
- Physical Review D Journal website
- Volume:
- 97
- Issue:
- 4
- Pages:
- 1-27
- Chapter number:
- 044021
- Publication date:
- 2018-02-16
- DOI:
- EISSN:
-
2470-0029
- ISSN:
-
2470-0010
- Pubs id:
-
pubs:746949
- URN:
-
uri:fa0baf02-4bb5-4440-9b23-15d4405866fc
- UUID:
-
uuid:fa0baf02-4bb5-4440-9b23-15d4405866fc
- Local pid:
- pubs:746949
- Paper number:
- 4
- Keywords:
- Copyright holder:
- © 2018 American Physical Society
- Copyright date:
- 2018
- Notes:
- This is the author accepted manuscript following peer review version of the article. The final version is available online from American Physical Review at: 10.1103/PhysRevD.97.044021
Journal article
General theories of linear gravitational perturbations to a Schwarzschild Black Hole
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+ Science and Technology Facilities Council
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+ Beecroft Institute of Particle Astrophysics and Cosmology
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