A new type of scalar field inflation

Germani, C; Kehagias, A

dc.contributor.author	Germani, C	en
dc.contributor.author	Kehagias, A	en
dc.date.accessioned	2014-03-01T02:52:33Z
dc.date.available	2014-03-01T02:52:33Z
dc.date.issued	2010	en
dc.identifier.issn	0094243X	en
dc.identifier.uri	https://dspace.lib.ntua.gr/xmlui/handle/123456789/35923
dc.subject	Inflation	en
dc.subject	Modified Gravity	en
dc.title	A new type of scalar field inflation	en
heal.type	conferenceItem	en
heal.identifier.primary	10.1063/1.3462690	en
heal.identifier.secondary	http://dx.doi.org/10.1063/1.3462690	en
heal.publicationDate	2010	en
heal.abstract	In this short note we discuss the possibility of producing a slow rolling inflationary background by considering a massive scalar field whose kinetic term is non-minimally coupled to gravity. © 2010 American Institute of Physics.	en
heal.journalName	AIP Conference Proceedings	en
dc.identifier.doi	10.1063/1.3462690	en
dc.identifier.volume	1241	en
dc.identifier.spage	595	en
dc.identifier.epage	599	en