Built on

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Original
2002
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Original
2002
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2003
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Original
2004

Then

G. N. Remmen and S. M. Carroll, How Many e e -Folds Should We Expect from High-Scale Inflation? , Phys. Rev. D 90
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Later among the works it cites.
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2015
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Later among the works it cites.
J. L. Cook, E. Dimastrogiovanni, D. A. Easson and L. M. Krauss, Reheating predictions in single field inflation , JCAP 04
Original
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2020

Gravitational wave constraints on the observable inflation

Tanin, Erwin H., Tenkanen, Tommi

Understand

Gravitational waves (GW) produced in the early Universe contribute to the number of relativistic degrees of freedom, $N_{\rm eff}$, during Big Bang Nucleosynthesis (BBN).

By using the constraints on $N_{\rm eff}$, we present a new bound on how much the Universe could have expanded between horizon exit of the largest observable scales today and the end of inflation.
We discuss the implications on inflationary models and show how the new constraints affect model selection.
We also discuss the sensitivities of the current and planned GW observatories such as LIGO and LISA, and show that the constraints they could impose are always less stringent than the BBN bound.