Classification of the Horndeski cosmologies via Noether symmetries

dc.contributor.author	Capozziello S.
dc.contributor.author	Dialektopoulos K.
dc.contributor.author	Sushkov S.
dc.date.accessioned	2019-01-22T20:45:52Z
dc.date.available	2019-01-22T20:45:52Z
dc.date.issued	2018
dc.identifier.issn	1434-6044
dc.identifier.uri	https://dspace.kpfu.ru/xmlui/handle/net/148653
dc.description.abstract	© 2018, The Author(s). Adopting Noether point symmetries, we classify and integrate dynamical systems coming from Horndeski cosmologies. The method is particularly effective both to select the form of Horndeski models and to derive exact cosmological solutions. Starting from the Lagrangians selected by the Noether symmetries, it is possible to derive several modified theories of gravity like f(R) gravity, Brans–Dicke gravity, string inspired gravity and so on. In any case, exact solutions are found out.
dc.relation.ispartofseries	European Physical Journal C
dc.title	Classification of the Horndeski cosmologies via Noether symmetries
dc.type	Article
dc.relation.ispartofseries-issue	6
dc.relation.ispartofseries-volume	78
dc.collection	Публикации сотрудников КФУ
dc.source.id	SCOPUS14346044-2018-78-6-SID85048276531

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