Dynamics of Bianchi type-V anisotropic dark energy cosmological model in a scale covariant theory of gravitation

International Journal of Mathematics and Systems Science

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Title Dynamics of Bianchi type-V anisotropic dark energy cosmological model in a scale covariant theory of gravitation
 
Creator Reddy, Dandala Radhakrishna
 
Subject Scale covariant theory; Bianchi type-V model; Dark energy model; cosmological model
 
Description This paper is devoted to the discussion of dynamical properties of anisotropic dark energy cosmological model of the universe in a Bianchi type-V space time in the framework of scale covariant theory of gravitation formulated by Canuto et al.(phys.Rev.Lett.39:429,1977).A  dark energy cosmological model is presented by solving the field equations of this theory by using some physically viable conditions. The dynamics of the model is  studied  by computing the cosmological parameters, dark energy density, equation of state(EoS) parameter, skewness parameters, deceleration parameter and the jerk parameter. This being a scalar field model gives us the quintessence model of the universe which describes a significant dark energy candidate of our accelerating universe. All the physical quantities discussed are in agreement with the recent cosmological observations.
 
Publisher EnPress Publisher LLC
 
Contributor No agencies
 
Date 2018-11-02
 
Type info:eu-repo/semantics/article
info:eu-repo/semantics/publishedVersion
Peer-reviewed Article
 
Format application/pdf
 
Identifier https://systems.enpress-publisher.com/index.php/IJMSS/article/view/560
10.24294/ijmss.v1i4.560
 
Source International Journal of Mathematics and Systems Science; Vol 1, No 4 (In publishing)
2578-1839
10.24294/ijmss.v1i4
 
Language eng
 
Relation https://systems.enpress-publisher.com/index.php/IJMSS/article/view/560/764
https://systems.enpress-publisher.com/index.php/IJMSS/article/downloadSuppFile/560/258
 
Rights Copyright (c) 2018 International Journal of Mathematics and Systems Science
http://creativecommons.org/licenses/by-nc/4.0
 

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