Cosmological viscous fluid models describing infinite time singularities in f(T) gravity

Abstract In this paper we explore the state parameter behaviour of the interacting viscous dark energy in f(T) gravity. Using constant deceleration parameter we investigate the cosmological implications of the viscosity and interaction between the dark components (energy and matter) in terms of Reds...

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Main Authors: R. D. Boko, M. J. S. Houndjo
Format: Article
Language:English
Published: SpringerOpen 2020-09-01
Series:European Physical Journal C: Particles and Fields
Online Access:http://link.springer.com/article/10.1140/epjc/s10052-020-8252-8
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author R. D. Boko
M. J. S. Houndjo
author_facet R. D. Boko
M. J. S. Houndjo
author_sort R. D. Boko
collection DOAJ
description Abstract In this paper we explore the state parameter behaviour of the interacting viscous dark energy in f(T) gravity. Using constant deceleration parameter we investigate the cosmological implications of the viscosity and interaction between the dark components (energy and matter) in terms of Redshift. So doing, the viscosity and the interaction between the two fluids are parameterized by constants $$\delta $$ δ and $$\xi $$ ξ respectively. In the later part of the paper, we explore some bulk viscosity models describing Little Rip and Pseudo Rip future singularities within f(T) modified gravity. We obtain gravitational equations of motion for viscous dark energy coupled with dark matter. Solving these equations, we found analytic expressions for characteristic properties of these cosmological models.
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spelling doaj.art-e94f14bcb6de4a408a9d252cbf18b7592022-12-21T18:51:33ZengSpringerOpenEuropean Physical Journal C: Particles and Fields1434-60441434-60522020-09-018091810.1140/epjc/s10052-020-8252-8Cosmological viscous fluid models describing infinite time singularities in f(T) gravityR. D. Boko0M. J. S. Houndjo1Faculté des Sciences et Techniques de Natitingou, UNSTIMFaculté des Sciences et Techniques de Natitingou, UNSTIMAbstract In this paper we explore the state parameter behaviour of the interacting viscous dark energy in f(T) gravity. Using constant deceleration parameter we investigate the cosmological implications of the viscosity and interaction between the dark components (energy and matter) in terms of Redshift. So doing, the viscosity and the interaction between the two fluids are parameterized by constants $$\delta $$ δ and $$\xi $$ ξ respectively. In the later part of the paper, we explore some bulk viscosity models describing Little Rip and Pseudo Rip future singularities within f(T) modified gravity. We obtain gravitational equations of motion for viscous dark energy coupled with dark matter. Solving these equations, we found analytic expressions for characteristic properties of these cosmological models.http://link.springer.com/article/10.1140/epjc/s10052-020-8252-8
spellingShingle R. D. Boko
M. J. S. Houndjo
Cosmological viscous fluid models describing infinite time singularities in f(T) gravity
European Physical Journal C: Particles and Fields
title Cosmological viscous fluid models describing infinite time singularities in f(T) gravity
title_full Cosmological viscous fluid models describing infinite time singularities in f(T) gravity
title_fullStr Cosmological viscous fluid models describing infinite time singularities in f(T) gravity
title_full_unstemmed Cosmological viscous fluid models describing infinite time singularities in f(T) gravity
title_short Cosmological viscous fluid models describing infinite time singularities in f(T) gravity
title_sort cosmological viscous fluid models describing infinite time singularities in f t gravity
url http://link.springer.com/article/10.1140/epjc/s10052-020-8252-8
work_keys_str_mv AT rdboko cosmologicalviscousfluidmodelsdescribinginfinitetimesingularitiesinftgravity
AT mjshoundjo cosmologicalviscousfluidmodelsdescribinginfinitetimesingularitiesinftgravity