Decoupling of the general scalar field mode and the solution space for Bianchi type i and v cosmologies coupled to perfect fluid sources

Christodoulakis, T; Grammenos, Th; Helias, Ch; Kevrekidis, PG; Spanou, A

dc.contributor.author	Christodoulakis, T	en
dc.contributor.author	Grammenos, Th	en
dc.contributor.author	Helias, Ch	en
dc.contributor.author	Kevrekidis, PG	en
dc.contributor.author	Spanou, A	en
dc.date.accessioned	2014-03-01T01:23:54Z
dc.date.available	2014-03-01T01:23:54Z
dc.date.issued	2006	en
dc.identifier.issn	0022-2488	en
dc.identifier.uri	https://dspace.lib.ntua.gr/xmlui/handle/123456789/17139
dc.subject.classification	Physics, Mathematical	en
dc.subject.other	EXPONENTIAL POTENTIALS	en
dc.subject.other	INFLATIONARY UNIVERSE	en
dc.subject.other	SCALING SOLUTIONS	en
dc.subject.other	HAIR THEOREM	en
dc.subject.other	EVOLUTION	en
dc.subject.other	CONSTANT	en
dc.subject.other	SYMMETRY	en
dc.subject.other	FLATNESS	en
dc.subject.other	HORIZON	en
dc.title	Decoupling of the general scalar field mode and the solution space for Bianchi type i and v cosmologies coupled to perfect fluid sources	en
heal.type	journalArticle	en
heal.identifier.primary	10.1063/1.2188210	en
heal.identifier.secondary	http://dx.doi.org/10.1063/1.2188210	en
heal.identifier.secondary	042505	en
heal.language	English	en
heal.publicationDate	2006	en
heal.abstract	The scalar field degree of freedom in Einstein's plus matter field equations is decoupled for Bianchi type I and V general cosmological models. The source, apart from the minimally coupled scalar field with arbitrary potential V(Phi), is provided by a perfect fluid obeying a general equation of state p=p(rho). The resulting ODE is, by an appropriate choice of final time gauge affiliated to the scalar field, reduced to first order, and then the system is completely integrated for arbitrary choices of the potential and the equation of state. (c) 2006 American Institute of Physics.	en
heal.publisher	AMER INST PHYSICS	en
heal.journalName	Journal of Mathematical Physics	en
dc.identifier.doi	10.1063/1.2188210	en
dc.identifier.isi	ISI:000237136800013	en
dc.identifier.volume	47	en
dc.identifier.issue	4	en