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Weak and Strong Warm Logamediate Anisotropic Inflationary Universe Model
Version 1
: Received: 24 June 2019 / Approved: 25 June 2019 / Online: 25 June 2019 (12:56:35 CEST)
A peer-reviewed article of this Preprint also exists.
Abstract
This paper is given to the investigation of warm inflation using Modified Chaplygin gas in the background of locally rotationally symmetric Bianchi Identity type I. We find out the field equations and perturbations parameters such as; scalar power spectrum, scalar spectral index, scalar potential and tensor to scalar ratio under slow roll approximation. We find out these parameters in directional of Hubble parameter during the Logamediate inflationary regime in weak and strong case. These comological parameters shows that the anisotropic model is also compatible WMAP$7$ with recent observational data Planck $2018$.
Keywords
warm inflation; slow roll approximation; scalar field
Subject
Physical Sciences, Particle and Field Physics
Copyright: This is an open access article distributed under the Creative Commons Attribution License which permits unrestricted use, distribution, and reproduction in any medium, provided the original work is properly cited.
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