Effects of local features of the inflaton potential on the spectrum and bispectrum of primordial perturbations

The European Physical Journal C

Stefano Gariazzo¹  Antonio Enea Romano²  Alexander Gallego Cadavid³ 

[1] Department of Physics, University of Torino, Via P. Giuria 1, 10125, Torino, Italy;INFN, Sezione di Torino, Via P. Giuria 1, 10125, Torino, Italy;Instituto de Fisica, Universidad de Antioquia, A.A.1226, Medellin, Colombia;Department of Physics, University of Crete, 71003, Heraklion, Greece;Yukawa Institute for Theoretical Physics, Kyoto University, Kyoto, Japan;Department of Physics, University of Torino, Via P. Giuria 1, 10125, Torino, Italy;INFN, Sezione di Torino, Via P. Giuria 1, 10125, Torino, Italy;Instituto de Fisica, Universidad de Antioquia, A.A.1226, Medellin, Colombia;Yukawa Institute for Theoretical Physics, Kyoto University, Kyoto, Japan;

关键词: Cosmic Microwave Background;    Hubble Parameter;    Curvature Perturbation;    Cosmic Microwave Background Temperature;    Starobinsky Model;   

DOI  :  10.1140/epjc/s10052-016-4232-4

来源: Springer

【 授权许可】

CC BY