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- W2769002299 abstract "Reheating after inflation can proceed even if the inflaton couples to Standard Model (SM) particles only gravitationally. However, particle production during the transition between de-Sitter expansion and a decelerating Universe is rather inefficient and the necessity to recover the visible Universe leads to a non-standard cosmological evolution initially dominated by remnants of the inflaton field. We remain agnostic to the specific dynamics of the inflaton field and discuss a generic scenario in which its remnants behave as a perfect fluid with a general barotropic parameter $w$. Using CMB and BBN constraints we derive the allowed range of inflationary scales. We also show that this scenario results in a characteristic primordial Gravitational Wave (GW) spectrum which gives hope for observation in upcoming runs of LIGO as well as in other planned experiments." @default.
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- W2769002299 date "2018-04-17" @default.
- W2769002299 modified "2023-10-03" @default.
- W2769002299 title "Gravitational wave signals and cosmological consequences of gravitational reheating" @default.
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- W2769002299 doi "https://doi.org/10.1088/1475-7516/2018/04/046" @default.
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