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- W2169587009 abstract "If the tensor-to-scalar ratio $r$ of cosmological perturbations takes a large value $rsim 0.1$, which may be inferred by recent BICEP2 result, we can hope to determine thermal history, in particular, the reheating temperature, $T_R$, after inflation by space-based laser interferometers. It is shown that upgraded and upshifted versions of DECIGO may be able to determine $T_R$ if it lies in the range $6times 10^6< T_R < 5times 10^7$GeV and $3times 10^7<T_R<2times 10^8$GeV, respectively. Although these ranges include predictions of some currently plausible inflation models, since each specification can probe $T_R$ of at most a decade range, we should determine the specifications of DECIGO with full account of constraints on inflation models to be obtained by near-future observations of temperature anisotropy and B-model polarization of the cosmic microwave background radiation." @default.
- W2169587009 created "2016-06-24" @default.
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- W2169587009 date "2015-01-22" @default.
- W2169587009 modified "2023-10-17" @default.
- W2169587009 title "Prospects of determination of reheating temperature after inflation by DECIGO" @default.
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- W2169587009 doi "https://doi.org/10.1093/ptep/ptu176" @default.
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