collaborators

7 papers

gr-qc2025

Structure and Mass-Radius Stability of Charged Compact Objects in Symmetric Teleparallel Euler-Heisenberg Gravity

Allah Ditta, M. Yousaf, G. Mustafa +4

In this work, we develop a new relativistic model for a charged anisotropic compact star in the framework of modified symmetric teleparallel gravity, namely -Euler-Heisenberg…

astro-ph.HE2025

Magnetized particle motion and accretion process with shock cone morphology around a decoupled hairy black holes

G. Mustafa, Faisal Javed, S. K. Maurya +5

Relativistic accretion onto compact objects such as black holes and neutron stars is one of the most efficient known mechanisms for converting gravitational potential energy into r…

gr-qc2025

Analytical and numerical study of accretion processes around charged spherically symmetric black holes in scalar-tensor Gauss-Bonnet gravity

G. Mustafa, O. Donmez, A. Errehymy +5

We investigate the physical phenomena occurring around a spherically symmetric, non-rotating charged black hole (BH) to explore the effects of scalar-tensor Gauss-Bonnet gravity on…

gr-qc2025

Observational constraints on f(Q,T) gravity from the mass-radius relation and stability of compact stars

S. K. Maurya, Abdul Aziz, Ksh. Newton Singh +3

In this investigation we examine the astrophysical consequences of the influence of pressure anisotropy on the physical properties of observed pulsars within the background of $f(Q…

gr-qc2025

Relativistic massive compact stars supported by decoupled matter: Implications for mass-radius bounds

S. K. Maurya, A. Errehymy, Ksh. Newton Singh +2

The merger of binary neutron stars (BNSs) is a remarkable astrophysical event where all four fundamental forces interplay dynamically across multiple stages, producing a rich spect…

gr-qc2025

Testing Quantum-Corrected Black Holes with QPOs Observations: A Study of Particle Dynamics and Accretion Flow

G. Mustafa, Sushant G. Ghosh, Orhan Donmez +3

We study the epicyclic oscillations of test particles around rotating quantum-corrected black holes (QCBHs), characterized by mass , spin , and quantum deformation parameter…