Stability of the anisotropically inflating Bianchi type VI expanding solutions

Details Stability of the anisotropically inflating Bianchi type VI expanding solutions Stability of the anisotropically inflating Bianchi type VI expanding solutions

Mar 2011

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2011phrvd..83f3004k&link_type=abstract

Physical Review D, vol. 83, Issue 6, id. 063004

Physics

3

Relativity And Gravitation, Modified Theories Of Gravity, Origin And Formation Of The Universe, Mathematical And Relativistic Aspects Of Cosmology

Scientific paper

A special class of the Bianchi type VI expanding solutions was speculated to break the cosmic no-hair theorem that will not approach the late-time de Sitter solution. We will show that an unstable mode always exists when the perturbation of the field equations is applied to the system. In addition to a model-independent perturbation formula, a simplification is also achieved by the introduction of a δR=0 solution good for quadratic models in all Bianchi spaces. The result shows that this special class of anisotropically expanding solutions is unstable.

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