Winstanley, E. orcid.org/0000-0001-8964-8142 (2003) On the existence of conformally coupled scalar field hair for black holes in (anti-)de Sitter space. Foundations of Physics, 33 (1). pp. 111-143. ISSN 0015-9018
Abstract
The Einstein-conformally coupled scalar field system is studied in the presence of a cosmological constant. We consider a massless or massive scalar field with no additional self-interaction, and spherically symmetric black hole geometries. When the cosmological constant is positive, no scalar hair can exist and the only solution is the Schwarzschild–de Sitter black hole. When the cosmological constant is negative, stable scalar field hair exists provided the mass of the scalar field is not too large.
Metadata
Item Type: | Article |
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Authors/Creators: |
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Copyright, Publisher and Additional Information: | © 2003 Plenum Publishing Corporation. This is an author produced version of a paper subsequently published in Foundations of Physics. Uploaded in accordance with the publisher's self-archiving policy. |
Keywords: | Black hole hair; conformal scalar field; (anti-)de Sitter space; negative cosmological constant; gauged extended supergravity; linear-stability; Baryon number; parity sector; no-hair; solitons; nonexistence; gravity; systems |
Dates: |
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Institution: | The University of Sheffield |
Academic Units: | The University of Sheffield > Faculty of Science (Sheffield) > School of Mathematics and Statistics (Sheffield) |
Depositing User: | Symplectic Sheffield |
Date Deposited: | 27 Jul 2016 13:59 |
Last Modified: | 23 Mar 2018 09:07 |
Published Version: | http://dx.doi.org/10.1023/A:1022871809835 |
Status: | Published |
Publisher: | Springer Verlag |
Refereed: | Yes |
Identification Number: | 10.1023/A:1022871809835 |
Open Archives Initiative ID (OAI ID): | oai:eprints.whiterose.ac.uk:102578 |