Study of growth matter index and cosmic implications in dynamical Chern–Simons modified gravity
Abstract In the framework of dynamical Chern–Simons theory of gravity, we study the recent cosmic expansion with acceleration of the universe. We take interacting scenario of dark energy and dark matter with three cutoffs like Granda–Oliveros, higher order derivative of Hubble parameter and generali...
Main Authors: | , , , |
---|---|
Format: | Article |
Language: | English |
Published: |
SpringerOpen
2021-08-01
|
Series: | European Physical Journal C: Particles and Fields |
Online Access: | https://doi.org/10.1140/epjc/s10052-021-09489-8 |
id |
doaj-85a0f737fbd941ee972f5feba760467e |
---|---|
record_format |
Article |
spelling |
doaj-85a0f737fbd941ee972f5feba760467e2021-08-15T11:14:16ZengSpringerOpenEuropean Physical Journal C: Particles and Fields1434-60441434-60522021-08-0181811210.1140/epjc/s10052-021-09489-8Study of growth matter index and cosmic implications in dynamical Chern–Simons modified gravityAbdul Jawad0Shamaila Rani1Saba Qummer2Amir Sharif3Department of Mathematics, COMSATS University IslamabadDepartment of Mathematics, COMSATS University IslamabadDepartment of Mathematics, COMSATS University IslamabadDepartment of Mathematics, COMSATS University IslamabadAbstract In the framework of dynamical Chern–Simons theory of gravity, we study the recent cosmic expansion with acceleration of the universe. We take interacting scenario of dark energy and dark matter with three cutoffs like Granda–Oliveros, higher order derivative of Hubble parameter and generalized holographic dark energy model. In the flat Friedmann–Robertson–Walker universe, well-known cosmological parameters have been calculated. We study the perturbation of matter density growth, growth factor and growth index behavior for the underlying framework. The cosmological parameters like equation of state parameter, deceleration parameter, and stability of each model are discussed. The outcomes of these models represent the cosmic expansion of the universe with acceleration.https://doi.org/10.1140/epjc/s10052-021-09489-8 |
collection |
DOAJ |
language |
English |
format |
Article |
sources |
DOAJ |
author |
Abdul Jawad Shamaila Rani Saba Qummer Amir Sharif |
spellingShingle |
Abdul Jawad Shamaila Rani Saba Qummer Amir Sharif Study of growth matter index and cosmic implications in dynamical Chern–Simons modified gravity European Physical Journal C: Particles and Fields |
author_facet |
Abdul Jawad Shamaila Rani Saba Qummer Amir Sharif |
author_sort |
Abdul Jawad |
title |
Study of growth matter index and cosmic implications in dynamical Chern–Simons modified gravity |
title_short |
Study of growth matter index and cosmic implications in dynamical Chern–Simons modified gravity |
title_full |
Study of growth matter index and cosmic implications in dynamical Chern–Simons modified gravity |
title_fullStr |
Study of growth matter index and cosmic implications in dynamical Chern–Simons modified gravity |
title_full_unstemmed |
Study of growth matter index and cosmic implications in dynamical Chern–Simons modified gravity |
title_sort |
study of growth matter index and cosmic implications in dynamical chern–simons modified gravity |
publisher |
SpringerOpen |
series |
European Physical Journal C: Particles and Fields |
issn |
1434-6044 1434-6052 |
publishDate |
2021-08-01 |
description |
Abstract In the framework of dynamical Chern–Simons theory of gravity, we study the recent cosmic expansion with acceleration of the universe. We take interacting scenario of dark energy and dark matter with three cutoffs like Granda–Oliveros, higher order derivative of Hubble parameter and generalized holographic dark energy model. In the flat Friedmann–Robertson–Walker universe, well-known cosmological parameters have been calculated. We study the perturbation of matter density growth, growth factor and growth index behavior for the underlying framework. The cosmological parameters like equation of state parameter, deceleration parameter, and stability of each model are discussed. The outcomes of these models represent the cosmic expansion of the universe with acceleration. |
url |
https://doi.org/10.1140/epjc/s10052-021-09489-8 |
work_keys_str_mv |
AT abduljawad studyofgrowthmatterindexandcosmicimplicationsindynamicalchernsimonsmodifiedgravity AT shamailarani studyofgrowthmatterindexandcosmicimplicationsindynamicalchernsimonsmodifiedgravity AT sabaqummer studyofgrowthmatterindexandcosmicimplicationsindynamicalchernsimonsmodifiedgravity AT amirsharif studyofgrowthmatterindexandcosmicimplicationsindynamicalchernsimonsmodifiedgravity |
_version_ |
1721206987065131008 |