Power-Law Inflation in Spacetimes Without Symmetry
103028 Relativitätstheorie
0103 physical sciences
FOS: Physical sciences
General Relativity and Quantum Cosmology (gr-qc)
01 natural sciences
General Relativity and Quantum Cosmology
103028 Theory of relativity
DOI:
10.1007/s00220-006-0133-y
Publication Date:
2006-10-17T12:18:25Z
AUTHORS (2)
ABSTRACT
16 pages<br/>We consider models of accelerated cosmological expansion described by the Einstein equations coupled to a nonlinear scalar field with a suitable exponential potential. We show that homogeneous and isotropic solutions are stable under small nonlinear perturbations without any symmetry assumptions. Our proof is based on results on the nonlinear stability of de Sitter spacetime and Kaluza-Klein reduction techniques.<br/>
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