English

Implications of the scalar tilt for the tensor-to-scalar ratio

Cosmology and Nongalactic Astrophysics 2016-01-20 v2 High Energy Physics - Theory

Abstract

We investigate the possible implications of the measured value of the scalar tilt nsn_s for the tensor-to-scalar ratio rr in slow-roll, single-field inflationary models. The measured value of the tilt satisfies ns11/Nn_s -1\sim 1/N_*, where N60N_* \sim 60 is the number of ee-folds for observationally relevant scales. If this is not a coincidence and the scaling holds for different values of NN, it strongly suggests that either rr is as big as 10110^{-1} (a possibility in tension with the recent data), or smaller than 10210^{-2} and exponentially dependent on nsn_s. A large region of the (nsn_s,rr) plane is not compatible with this scaling.

Keywords

Cite

@article{arxiv.1412.0678,
  title  = {Implications of the scalar tilt for the tensor-to-scalar ratio},
  author = {Paolo Creminelli and Sergei Dubovsky and Diana López Nacir and Marko Simonović and Gabriele Trevisan and Giovanni Villadoro and Matias Zaldarriaga},
  journal= {arXiv preprint arXiv:1412.0678},
  year   = {2016}
}

Comments

4 pages, 1 figure. Published version