English

On the Effective Field Theory for Quasi-Single Field Inflation

Cosmology and Nongalactic Astrophysics 2017-12-13 v2 General Relativity and Quantum Cosmology High Energy Physics - Theory

Abstract

We study the effective field theory (EFT) description of the virtual particle effects in quasi-single field inflation, which unifies the previous results on large mass and large mixing cases. By using a horizon crossing approximation and matching with known limits, approximate expressions for the power spectrum and the spectral index are obtained. The error of the approximate solution is within 10% in dominate parts of the parameter space, which corresponds to less-than-0.1% error in the nsn_s-rr diagram. The quasi-single field corrections on the nsn_s-rr diagram are plotted for a few inflation models. Especially, the quasi-single field correction drives m2ϕ2m^2\phi^2 inflation to the best fit region on the nsn_s-rr diagram, with an amount of equilateral non-Gaussianity which can be tested in future experiments.

Keywords

Cite

@article{arxiv.1708.01709,
  title  = {On the Effective Field Theory for Quasi-Single Field Inflation},
  author = {Xi Tong and Yi Wang and Siyi Zhou},
  journal= {arXiv preprint arXiv:1708.01709},
  year   = {2017}
}

Comments

12 pages, 5 figures. v2: references added