Zobrazeno 1 - 10
of 24
pro vyhledávání: '"S. H. Shekh"'
Publikováno v:
European Physical Journal C: Particles and Fields, Vol 84, Iss 8, Pp 1-15 (2024)
Abstract In this paper, we present a cosmological model within the framework of symmetric teleparallel gravity, focusing on f(Q) gravity, where Q represents the non-metricity scalar. Utilizing cosmological datasets, we derive an accelerating cosmolog
Externí odkaz:
https://doaj.org/article/04df0aba9d0c46ed9f90f6806a0dbae0
Publikováno v:
Symmetry, Vol 15, Iss 10, p 1835 (2023)
The present analysis deals with the study of the f(Q,T) theory of gravity, which was recently considered by many cosmologists. In this theory of gravity, the action is taken as an arbitrary function f(Q,T), where Q is non-metricity and T is the trace
Externí odkaz:
https://doaj.org/article/09c83d6169574855a446466a5a80ea73
Publikováno v:
Frontiers in Astronomy and Space Sciences, Vol 9 (2022)
The existing analysis reports a reconstruction scheme of the newly proposed gravity say f(Q) gravity through the scale factor of the form a(t)=a0tn=11+z by describing the power-law cosmology. The reconstructed f(Q) gravity models disclosed how this m
Externí odkaz:
https://doaj.org/article/1b5c91c6ffc149c096dc23042d5d0116
Publikováno v:
International Journal of Geometric Methods in Modern Physics.
The paper presents Barrow holographic dark energy (infrared cut-off is the Hubble horizon) suggested by Barrow recently (Physics Letters B 808 (2020): 135643) in an anisotropic Bianchi type-I Universe within the framework of $% f\left( Q\right) $ sym
Externí odkaz:
https://explore.openaire.eu/search/publication?articleId=doi_dedup___::76453bb35f6dec62a3599db11ff4846f
http://arxiv.org/abs/2209.00341
http://arxiv.org/abs/2209.00341
In this paper, we investigate the homogeneous and isotropic flat FLRW Universe in the logarithmic form of $f\left( Q\right) $ gravity, where $% Q $ is the non-metricity scalar, specifically, $f\left( Q\right) =\alpha +\beta \log \left( Q\right) $, wh
Externí odkaz:
https://explore.openaire.eu/search/publication?articleId=doi_dedup___::39f78c3016ab455502cba166968f9c6e
In this work, we have discussed a spatially homogeneous and anisotropic Bianchi type-I space-time in the presence of Barrow holographic dark energy (infrared cut-off is the Hubble's horizon) proposed by Barrow recently (Physics Letters B 808 (2020):
Externí odkaz:
https://explore.openaire.eu/search/publication?articleId=doi_dedup___::d5b988de4b2e95dbc4de2ca70fc43dbb
Publikováno v:
Classical and Quantum Gravity. 40:055011
In this study, the non-metricity scalar Q, which characterizes the gravitational interaction, is used to analyze the Universe’s rapid expansion within the context of the f(Q) gravity theory. We suggest an emergent scale factor, which produces the d
Autor:
S. H. Shekh
Publikováno v:
Contemporary Mathematics. 1:49-57
We have investigated the dynamics of spatially homogeneous Bianchi type-I (LRS) space-time filled with two minimally interacting fields-matter and holographic dark energy components with volumetric power laws expansion towards the gravitational field
Publikováno v:
Journal of Scientific Research. 11:249-262
In this paper, we have investigated Kantowaski-Sachs cosmological model with bulk viscous and cosmic string in the framework of Teleparallel Gravity so called f(T) gravity, where T denotes the torsion scalar. The behavior of accelerating universe is