Stable black holes in shift-symmetric Horndeski theories

Tretyakova, D. A.; Takahashi, K.

doi:10.1088/1361-6382/aa8057

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Поле DC	Значение	Язык
dc.contributor.author	Tretyakova, D. A.	en
dc.contributor.author	Takahashi, K.	en
dc.date.accessioned	2021-08-31T15:01:42Z	-
dc.date.available	2021-08-31T15:01:42Z	-
dc.date.issued	2017	-
dc.identifier.citation	Tretyakova D. A. Stable black holes in shift-symmetric Horndeski theories / D. A. Tretyakova, K. Takahashi. — DOI 10.1088/1361-6382/aa8057 // Classical and Quantum Gravity. — 2017. — Vol. 34. — Iss. 17. — 175007.	en
dc.identifier.issn	2649381	-
dc.identifier.other	Final	2
dc.identifier.other	All Open Access, Green	3
dc.identifier.other	https://www.scopus.com/inward/record.uri?eid=2-s2.0-85027971307&doi=10.1088%2f1361-6382%2faa8057&partnerID=40&md5=3bacef381d3aaf9313837cfc5d207c11
dc.identifier.other	http://arxiv.org/pdf/1702.03502	m
dc.identifier.uri	http://elar.urfu.ru/handle/10995/102083	-
dc.description.abstract	In shift-symmetric Horndeski theories, a static and spherically symmetric black hole can support linearly time-dependent scalar hair. However, it was shown that such a solution generically suffers from ghost or gradient instability in the vicinity of the horizon. In the present paper, we explore the possibility to avoid the instability, and present a new example of theory and its black hole solution with a linearly time-dependent scalar configuration. We also discuss the stability of solutions with static scalar hair for a special case where nonminimal derivative coupling to the Einstein tensor appears. © 2017 IOP Publishing Ltd.	en
dc.format.mimetype	application/pdf	en
dc.language.iso	en	en
dc.publisher	Institute of Physics Publishing	en
dc.rights	info:eu-repo/semantics/openAccess	en
dc.source	Classical Quantum Gravity	2
dc.source	Classical and Quantum Gravity	en
dc.subject	BLACK HOLE STABILITY	en
dc.subject	HORNDESKI THEORY	en
dc.subject	SCALAR-TENSOR GRAVITY	en
dc.title	Stable black holes in shift-symmetric Horndeski theories	en
dc.type	Article	en
dc.type	info:eu-repo/semantics/article	en
dc.type	info:eu-repo/semantics/publishedVersion	en
dc.identifier.doi	10.1088/1361-6382/aa8057	-
dc.identifier.scopus	85027971307	-
local.contributor.employee	Tretyakova, D.A., Institute for Natural Sciences, Ural Federal University, Lenin av. 51, Yekaterinburg, 620083, Russian Federation
local.contributor.employee	Takahashi, K., Research Center for the Early Universe (RESCEU), Graduate School of Science, University of Tokyo, Tokyo, 113-0033, Japan, Department of Physics, Graduate School of Science, University of Tokyo, Tokyo, 113-0033, Japan
local.issue	17	-
local.volume	34	-
dc.identifier.wos	000406836000002	-
local.contributor.department	Institute for Natural Sciences, Ural Federal University, Lenin av. 51, Yekaterinburg, 620083, Russian Federation
local.contributor.department	Research Center for the Early Universe (RESCEU), Graduate School of Science, University of Tokyo, Tokyo, 113-0033, Japan
local.contributor.department	Department of Physics, Graduate School of Science, University of Tokyo, Tokyo, 113-0033, Japan
local.identifier.pure	04e7eccc-98c8-457f-9626-be4ea255059d	uuid
local.identifier.pure	2037241	-
local.description.order	175007	-
local.identifier.eid	2-s2.0-85027971307	-
local.identifier.wos	WOS:000406836000002	-
Располагается в коллекциях:	Научные публикации ученых УрФУ, проиндексированные в SCOPUS и WoS CC

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