K. Ghaderi
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View article: Phantom Dark Energy Behavior in Weyl Type f(Q,T) Gravity Models with Observational Constraints
Phantom Dark Energy Behavior in Weyl Type f(Q,T) Gravity Models with Observational Constraints Open
This study explores the behavior of phantom dark energy within the framework of Weyl-type f(Q,T) gravity, considering a spatially flat FLRW universe under observational constraints. The field equations are analytically solved for a dust-li…
View article: Phantom Dark Energy Behavior in Weyl Type f (Q, T) Gravity Models with Observational Constraints
Phantom Dark Energy Behavior in Weyl Type f (Q, T) Gravity Models with Observational Constraints Open
This study explores the behavior of phantom dark energy within the framework of Weyl-type $f(Q,T)$ gravity, considering a spatially flat FLRW universe under observational constraints. The field equations are analytically solved for a dust-…
View article: On new regular quadratic Gaussian black hole: Photon sphere, shadow and gravitational lensing
On new regular quadratic Gaussian black hole: Photon sphere, shadow and gravitational lensing Open
Gaussian black holes constitute an important class of regular black holes, characterized by their spherically symmetric and static nature. These solutions emerge from the framework of Einstein’s equations, particularly when incorporating t…
View article: Barrow Holographic Dark Energy in f (Q, T) gravity
Barrow Holographic Dark Energy in f (Q, T) gravity Open
In the present analysis, we explore a new version of dark energy called Barrow holographic dark energy within the framework modified gravity called $f(Q,T)$ gravity by adopting the simple homogeneous, isotropic, and spatially flat Friedman…
View article: Real particle geodesics and thermodynamics of a black hole in Regular Schwarzschild-Anti de Sitter space-time
Real particle geodesics and thermodynamics of a black hole in Regular Schwarzschild-Anti de Sitter space-time Open
Regular Schwarzschild Anti-de-Sitter (RSch-AdS) spacetime, which is a maximally symmetric and Lorentzian manifold of negative curvature, is a solution of Einstein's field equations with a negative cosmological constant and a matter source …
View article: Radiating Isotropic Homogeneous f(R,G) Gravity Model with Quark and Strange Quark Matter
Radiating Isotropic Homogeneous f(R,G) Gravity Model with Quark and Strange Quark Matter Open
Present analysis devoted to the dynamical investigation of radiating quark and strange quark matter in the framework of f(R, G) theory of gravity towards spatially homogeneous isotropic Friedman-Robertson-Walker line element filled with is…
View article: Using probabilistic neural network to analyze the binary starsSchulte 3, EY Cep, HD 101131, and Haro 1-14c
Using probabilistic neural network to analyze the binary starsSchulte 3, EY Cep, HD 101131, and Haro 1-14c Open
The use of artificial neural networks (ANNs) in physical sciences has increased recently. Determining the orbital elements of binary systems helps us to obtain fundamental information. In this paper, ANNs were used to find the correspondin…