Compact stars in vector–tensor-Horndeski theory of gravity

dc.contributor.author	Momeni, Davood
dc.contributor.author	Faizal, Mir
dc.contributor.author	Myrzakulov, Kairat
dc.contributor.author	Myrzakulov, Ratbay
dc.date.accessioned	2025-01-10T06:55:29Z
dc.date.available	2025-01-10T06:55:29Z
dc.date.issued	2017
dc.identifier.issn	2413-2179
dc.identifier.other	DOI 10.1140/epjc/s10052-017-4606-2
dc.identifier.uri	http://rep.enu.kz/handle/enu/20800
dc.description.abstract	In this paper, we will analyze a theory of modified gravity, in which the field content of general relativity will be increased to include a vector field. We will use the Horndeski formalism to non-minimally couple this vector field to the metric. As we will be using the Horndeski formalism, this theory will not contain Ostrogradsky ghost degree of freedom. We will analyze compact stars using this vector–tensor-Horndeski theory	ru
dc.language.iso	en	ru
dc.publisher	Eurasian Physical Technical Journal C	ru
dc.relation.ispartofseries	77:37;
dc.title	Compact stars in vector–tensor-Horndeski theory of gravity	ru
dc.type	Article	ru