Dynamics of single-field inflation in the framework of holographic f(T) gravity

Author:

Chattopadhyay Surajit1ORCID,Pasqua Antonio2,Radinschi Irina3,Beesham Aroonkumar4

Affiliation:

1. Department of Mathematics, Amity University, Kolkata, Major Arterial Road, Action Area II, Rajarhat, New Town, Kolkata, West Bengal 700135, India

2. Department of Physics, University of Trieste, Via Valerio 2 34127 Trieste, Italy

3. Department of Physics, “Gheorghe Asachi” Technical University, Iasi 700050, Romania

4. Department of Mathematical Sciences, University of Zululand, Private Bag X1001, Kwa-Dlangezwa 3886, South Africa

Abstract

In the work reported in the present paper, we have considered the inflationary dynamics inspired by holographic Ricci dark energy (HRDE) with the energy density [Formula: see text] in the framework of [Formula: see text] gravity. We have considered a [Formula: see text]-gravity model in linear form, which is sourced by a canonical scalar field due to the HRDE. We have investigated an inflationary Universe in this framework through slow-roll formalism. We also studied the scalar spectral index [Formula: see text] and tensor-to-scalar ratio [Formula: see text], which have come out to be in agreement with WMAP[Formula: see text]BAO[Formula: see text][Formula: see text] and Planck 2015 data.

Publisher

World Scientific Pub Co Pte Lt

Subject

Physics and Astronomy (miscellaneous)

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