Models of holographic dark energy in f (Q) gravity
SH Shekh - Physics of the dark Universe, 2021 - Elsevier
Present analysis dedicated to the dynamical investigation of models of holographic dark
energy using FLRW cosmological model in the context of modified gravity in which …
energy using FLRW cosmological model in the context of modified gravity in which …
Cosmological solutions from induced matter model applied to 5D gravity and the shrinking of the extra coordinate
PHRS Moraes - The European Physical Journal C, 2015 - Springer
In this work, I present exact cosmological solutions from Wesson's induced matter model
applied to a general 5D metric in f (R, T) f (R, T) theory of gravity. The non-conservation of …
applied to a general 5D metric in f (R, T) f (R, T) theory of gravity. The non-conservation of …
Anisotropic cosmological models in gravity with variable deceleration parameter
The objective of this work enclosed with the study of spatially homogeneous anisotropic
Bianchi type-I universe in f (R, T) gravity (where R is the Ricci scalar and T is the trace of …
Bianchi type-I universe in f (R, T) gravity (where R is the Ricci scalar and T is the trace of …
LRS Bianchi type-I cosmological model in f(R,T) theory of gravity with Λ(T)
The locally rotationally symmetric (LRS) Bianchi type-I cosmological models have been
investigated in f (R, T) theory of gravity, where R is the Ricci scalar and T is the trace of the …
investigated in f (R, T) theory of gravity, where R is the Ricci scalar and T is the trace of the …
A measure of complexity for axial self-gravitating static fluids
U Farwa, Z Yousaf, MZ Bhatti - Physica Scripta, 2022 - iopscience.iop.org
One of the feasible potential candidates for illustrating the accelerating expansion of the
cosmos can be taken through the notion of modified gravity. Within the context of metric f (R) …
cosmos can be taken through the notion of modified gravity. Within the context of metric f (R) …
A transition from a decelerated to an accelerated phase of the universe expansion from the simplest non-trivial polynomial function of in the formalism
P Moraes, G Ribeiro, RAC Correa - Astrophysics and Space Science, 2016 - Springer
In this work we present cosmological solutions from the simplest non-trivial polynomial
function of TT in f (R, T) f(R,T) theory of gravity, with RR and TT standing for the Ricci scalar …
function of TT in f (R, T) f(R,T) theory of gravity, with RR and TT standing for the Ricci scalar …
Reheating and particle creation in unimodular f(R, T) gravity
We study cosmological inflation and reheating in the unimodular f (R, T) gravity. During the
reheating era, which takes place just after the end of inflation, the energy density of inflaton …
reheating era, which takes place just after the end of inflation, the energy density of inflaton …
Dynamical analysis with thermodynamic aspects of anisotropic dark energy bounce cosmological model in f (R, G) gravity
SH Shekh - New astronomy, 2021 - Elsevier
Present analysis dedicated to the dynamical investigation of anisotropic dark energy LRS
Bianchi type-I cosmological model in the context of modified gravity in which Langrangian …
Bianchi type-I cosmological model in the context of modified gravity in which Langrangian …
Kaluza–Klein cosmological model in f(R, T) gravity with Λ(T)
A class of Kaluza–Klein cosmological models in f (R, T) theory of gravity have been
investigated. In the work, we have considered the functional f (R, T) to be in the form f (R, T) …
investigated. In the work, we have considered the functional f (R, T) to be in the form f (R, T) …
Analysis of Reconstructed Modified Symmetric Teleparallel f(Q) Gravity
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)= a 0 tn= 1 1+ z by describing the power …
(Q) gravity through the scale factor of the form a (t)= a 0 tn= 1 1+ z by describing the power …