We generalize the result of Rindler-Ishak for the lensing deflection angle in a Schwarzschild– deSitter (SdS) space–time, to the case of a general spherically symmetric fluid beyond the …
We study the thermodynamics of galaxy clusters in a modified Newtonian potential motivated by a general solution to Newton's' sphere-point'equivalence theorem. We obtain …
We discuss the galaxy clustering based on thermodynamics and statistical mechanics in the expanding universe in a modified theory of gravity. The modified general relativity (MGR) is …
We study the clustering of galaxies in generalized uncertainty principle (GUP) modified Newtonian potential. We compute the corrected N-particle partition function which leads to …
We assume a modified (conformal) gravity theory, which produces a stronger interaction at large scale, in order to discuss the statistical distribution of the galaxy clusters based on …
We developed the functional form of the two-point correlation function under the approximation of fixed particle number density n (bar). We solved the quasi-linear partial …
HA Bagat, M Hameeda, PA Ganai - Physica Scripta, 2022 - iopscience.iop.org
In this manuscript, we have explored the large-scale structure (LSS) of the Universe using the halo approximation of galaxies and the mean-field (mean-field approximation) theory of …
We exploit a new theory of gravity proposed by Finzi, which gives stronger interaction at large scales, to study the thermodynamic description of galaxy clusters. We employ a …
We exploit a new theory of gravity proposed by Finzi, which gives stronger interaction at large scales, to study the thermodynamic description of galaxy clusters. We employ a …