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

dc.creator	Christodoulakis, T.	en
dc.creator	Grammenos, T.	en
dc.creator	Helias, C.	en
dc.creator	Kevrekidis, P. G.	en
dc.creator	Spanou, A.	en
dc.date.accessioned	2015-11-23T10:24:43Z
dc.date.available	2015-11-23T10:24:43Z
dc.date.issued	2006
dc.identifier	10.1063/1.2188210
dc.identifier.issn	0022-2488
dc.identifier.uri	http://hdl.handle.net/11615/26682
dc.description.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
dc.source.uri	<Go to ISI>://WOS:000237136800013
dc.subject	EXPONENTIAL POTENTIALS	en
dc.subject	INFLATIONARY UNIVERSE	en
dc.subject	SCALING SOLUTIONS	en
dc.subject	HAIR	en
dc.subject	THEOREM	en
dc.subject	EVOLUTION	en
dc.subject	CONSTANT	en
dc.subject	SYMMETRY	en
dc.subject	FLATNESS	en
dc.subject	HORIZON	en
dc.subject	Physics, Mathematical	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
dc.type	journalArticle	en

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