4.6 Article

Curing inflationary degeneracies using reheating predictions and relic gravitational waves

Journal

Publisher

IOP Publishing Ltd
DOI: 10.1088/1475-7516/2021/05/075

Keywords

gravitational waves / theory; inflation; physics of the early universe; primordial gravitational waves (theory)

Funding

  1. Council of Scientific and Industrial Research (CSIR), India
  2. J. C. Bose Fellowship of Department of Science and Technology, Government of India
  3. Russian Foundation for Basic Research [20-02-00411]

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In this study, the authors discuss degeneracies in inflationary cosmology predictions for CMB observables and demonstrate how constraints on post-inflationary reheating parameters can break this degeneracy in certain inflationary models. The study also shows how relic gravitational waves provide valuable information about the post-inflationary epoch and can be used to cure inflationary degeneracies in {n(S), r}. Through considering reheating parameters and relic gravitational waves, various inflationary degeneracies can be addressed and resolved.
It is well known that the inflationary scenario often displays different sets of degeneracies in its predictions for CMB observables. These degeneracies usually arise either because multiple inflationary models predict similar values for the scalar spectral index n(S) and the tensor-to-scalar ratio r, or because within the same model, the values of {n(S), r} are insensitive to some of the model parameters, making it difficult for CMB observations alone to constitute a unique probe of inflationary cosmology. We demonstrate that by taking into account constraints on the post-inflationary reheating parameters such as the duration of reheating Nre, its temperature T-re and especially its equation of state (EOS), w(re), it is possible to break this degeneracy in certain classes of inflationary models where identical values of {n(S), r} can correspond to different reheating wre. In particular, we show how reheating constraints can break inflationary degeneracies in the T-model and the E-model ff-attractors. Non-canonical inflation is also studied. The relic gravitational wave (GW) spectrum provides us with another tool to break inflationary degeneracies. This is because the GW spectrum is sensitive to the post-inflationary EOS of the universe. Indeed a stiff EOS during reheating (w(re) > 1/3) gives rise to a small scale blue tilt in the spectral index nGW = d log Omega GW/d log k > 0, while a soft EOS (w(re) < 1/3) results in a red tilt. Relic GWs therefore provide us with valuable information about the post-inflationary epoch, and their spectrum can be used to cure inflationary degeneracies in {n(S), r}.

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