Preprint Article Version 1 This version is not peer-reviewed

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)

How to cite: Javed, W.; Nawazish, I.; Khan, M.R.; Övgün, A. Weak and Strong Warm Logamediate Anisotropic Inflationary Universe Model. Preprints 2019, 2019060252 (doi: 10.20944/preprints201906.0252.v1). Javed, W.; Nawazish, I.; Khan, M.R.; Övgün, A. Weak and Strong Warm Logamediate Anisotropic Inflationary Universe Model. Preprints 2019, 2019060252 (doi: 10.20944/preprints201906.0252.v1).

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 $2018$.

Subject Areas

warm inflation; slow roll approximation; scalar field

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