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A model of chaotic inflation based on the theory of a scalar field with potential \lambda\phi^4 perfectly matches the observational data if one adds to it a tiny non-minimal coupling to gravity -\xi/2 \phi^2 R with \xi > 0.002.
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2009
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2009
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2010
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2010
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F. Bezrukov and D. Gorbunov, “Light inflaton after LHC8 and WMAP9 results,” arXiv:1303.4395 [hep-ph]
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2013
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