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• W1963570895 startingPage "1416" @default.
• W1963570895 abstract "We prove a cosmic no-hair theorem for Bianchi models in power-law inflation. Provided that the potential of an inflaton $ensuremath{varphi}$ is $mathrm{exp}(ensuremath{-}{ensuremath{lambda}}_{ensuremath{kappa}ensuremath{varphi}})$ with $0ensuremath{le}ensuremath{lambda}<sqrt{frac{2}{3}}$, we find that the isotropic power-law solution is the unique attractor for any initially expanding Bianchi-type models except type IX. For Bianchi type IX, this conclusion is also true if the initial ratio of the vacuum energy to the maximum three-curvature is larger than one half." @default.
• W1963570895 created "2016-06-24" @default.
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• W1963570895 date "1992-02-15" @default.
• W1963570895 modified "2023-09-30" @default.
• W1963570895 title "Cosmic no-hair theorem in power-law inflation" @default.
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• W1963570895 doi "https://doi.org/10.1103/physrevd.45.1416" @default.
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