Abstract
If the tensor-to-scalar ratio r of cosmological perturbations takes a large value r∼0.1, which may be inferred from the recent BICEP2 result, we can hope to determine thermal history, in particular, the reheating temperature, TR, after inflation by space-based laser interferometers. It is shown that upgraded and upshifted versions of DECIGO may be able to determine TR if it lies in the range 6×106<TR <5×107GeV and 3×107<TR<2×108GeV, respectively. Although these ranges include predictions of some currently plausible inflation models, because each specification can probe TR of a range of at most a decade, we should determine the specifications of DECIGO taking full account of the constraints on inflation models to be obtained by near-future observations of temperature anisotropy and B-model polarization of the cosmic microwave background radiation.
Original language | English |
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Journal | Progress of Theoretical and Experimental Physics |
Volume | 2015 |
Issue number | 1 |
DOIs | |
Publication status | Published - 2014 Oct 10 |
Externally published | Yes |
Keywords
- E02
- E75
- E80
ASJC Scopus subject areas
- Physics and Astronomy(all)