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- W1975223670 abstract "Abstract The cosmological curvature perturbation may be generated when some ‘curvaton’ field, different from the inflaton, oscillates in a background of unperturbed radiation. In its simplest form the curvaton paradigm requires the Hubble parameter during inflation to be bigger than 10 7 GeV, but this bound may be evaded if the curvaton field (or an associated tachyon) is strongly coupled to a field which acquires a large value at the end of inflation. As a result the curvaton paradigm might be useful in improving the viability of low-scale inflation models, in which the supersymmetry-breaking mechanism is the same as the one which operates in the vacuum." @default.
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- W1975223670 date "2004-01-01" @default.
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- W1975223670 title "Can the curvaton paradigm accommodate a low inflation scale?" @default.
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- W1975223670 doi "https://doi.org/10.1016/j.physletb.2003.11.019" @default.
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