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

被引:27
作者
Christodoulakis, T [1 ]
Grammenos, T
Helias, C
Kevrekidis, PG
Spanou, A
机构
[1] Univ Athens, Dept Phys, GR-15784 Athens, Greece
[2] Univ Thessaly, Dept Mech & Ind Engn, Volos 38334, Greece
[3] Univ Massachusetts, Dept Math & Stat, Amherst, MA 01003 USA
[4] Natl Tech Univ Athens, Dept Phys, GR-15773 Athens, Greece
关键词
D O I
10.1063/1.2188210
中图分类号
O4 [物理学];
学科分类号
0702 ;
摘要
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.
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页数:11
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