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Post-inflationary behavior of adiabatic perturbations and tensor-to-scalar ratio

Andrei Linde·Viatcheslav Mukhanov·Misao Sasaki
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Abstract

We explain why it is so difficult and perhaps even impossible to increase the cosmological tensor-to-scalar perturbation ratio during the post-inflationary evolution of the universe. Nevertheless, contrary to some recent claims, tensor perturbations can be relatively large in the simplest inflationary models which do not violate any rules of modern quantum field theory.

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Andrei Linde, Viatcheslav Mukhanov, Misao Sasaki. 2005-09-12. Post-inflationary behavior of adiabatic perturbations and tensor-to-scalar ratio. https://doi.org/10.1088/1475-7516%2F2005%2F10%2F002

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