The impact of anisotropic pressure models in neutron stars (NSs) is increasing their compactness. Therefore, for the relatively soft NS equation of state (EOS), we can still obtain …
One of the most common assumptions has been made that the pressure inside the star is isotropic in nature. However, the pressure is locally anisotropic in nature which is a more …
JMZ Pretel - The European Physical Journal C, 2023 - Springer
We construct dark energy stars with Chaplygin-type equation of state (EoS) in the presence of anisotropic pressure within the framework of Einstein gravity. From the classification …
L Baskey, S Ray, S Das, S Majumder, A Das - The European Physical …, 2023 - Springer
We present herein a new class of singularity-free interior solutions to describe realistic anisotropic compact stellar objects with spherically symmetric matter distribution. A specific …
S Kaur, SK Maurya, S Shukla - Physica Scripta, 2023 - iopscience.iop.org
This paper presents a study on a spherically symmetric anisotropic solution in f (Q) gravity in the framework of vanishing complexity formalism, which derives a relation between …
SK Maurya, A Ashraf, F Al Khayari, G Mustafa… - The European Physical …, 2024 - Springer
In the present article, A new class of singularity-free charged anisotropic stars is derived in f (Q)-gravity regime. To solve the field equations, we assume a particular form of anisotropy …
In this paper, we study the impact of anisotropy on neutron stars with different equations of state, which have been modeled by a piecewise polytropic function with continuous sound …
We have previously shown [R. Rizaldy, AR Alfarasyi, A. Sulaksono, and T. Sumaryada, Phys. Rev. C 100, 055804 (2019) 2469-9985 10.1103/PhysRevC. 100.055804] that Fermi …
Anisotropy in pressure within a star emerges from exotic internal processes. In this study, we incorporate pressure anisotropy using the Quasi-Local model. Macroscopic properties …