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Investigating physical existence of charged stellar models
This study aims at the detailed exploration of the internal structure of various anisotropic star
configurations interacting with an electromagnetic field within the framework of f (R, T, Q) …
configurations interacting with an electromagnetic field within the framework of f (R, T, Q) …
Compact stars in Rastall gravity: hydrostatic equilibrium and radial pulsations
JMZ Pretel, CE Mota - General Relativity and Gravitation, 2024 - Springer
Within the context of Rastall gravity, we investigate the hydrostatic equilibrium and
dynamical stability against radial pulsations of compact stars, where a free parameter β …
dynamical stability against radial pulsations of compact stars, where a free parameter β …
Interacting quark star with pressure anisotropy and recent astrophysical observations
This paper investigates the internal structure and equation of state (EoS) of quark stars (QS)
with pressure anisotropy, incorporating recent astrophysical observations. Utilizing …
with pressure anisotropy, incorporating recent astrophysical observations. Utilizing …
Non-Newtonian gravity in color-flavor locked strange stars and the 2.6 M⊙ component in GW190814
CM Pi, SH Yang - New Astronomy, 2025 - Elsevier
We investigate the effects of non-Newtonian gravity on the properties of the color-flavor
locked strange stars and constrain the parameters of the strange quark matter model using …
locked strange stars and constrain the parameters of the strange quark matter model using …
Anisotropic quark stars in gravity
Complete List of Authors: Tangphati, Takol; King Mongkut's University of Technology
Thonburi SAKALLI, İzzet; Dogu Akdeniz Universitesi, Fizik Banerjee, Ayan; University of …
Thonburi SAKALLI, İzzet; Dogu Akdeniz Universitesi, Fizik Banerjee, Ayan; University of …
Color flavor locked strange stars in de Rham–Gabadadze–Tolley like massive gravity
KP Das, A Karmakar, U Debnath - The European Physical Journal C, 2024 - Springer
Abstract We investigate Color Flavor Locked (CFL) Strange Stars using the most basic de
Rham–Gabadadze–Tolley massive gravity model, which explains the massive graviton in …
Rham–Gabadadze–Tolley massive gravity model, which explains the massive graviton in …
Quark stars in f (R, T) gravity: mass-to-radius profiles and observational data
Sakalli, Izzet; Dogu Akdeniz Universitesi, Fizik Dayanandan, Baiju; University of Nizwa,
Department of Mathematical & Physical Sciences; University of Nizwa, Pradhan, Anirudh; …
Department of Mathematical & Physical Sciences; University of Nizwa, Pradhan, Anirudh; …
Effect of rainbow function on radial oscillations and some other properties of Chaplygin dark star
KP Das, U Debnath - The European Physical Journal Plus, 2024 - Springer
In the present article, we have imagined a hypothetical spherically symmetric stellar
structure, made by an isotropic fluid satisfying dark energy equation of sate (EOS), named as …
structure, made by an isotropic fluid satisfying dark energy equation of sate (EOS), named as …
Constraint on the equation of state of strange quark star: Perturbative QCD along with a density-dependent bag constant
This study investigates the structural properties of strange quark stars (SQS) using a
Quantum Chromodynamics (QCD) perturbative model combined with the latest Particle Data …
Quantum Chromodynamics (QCD) perturbative model combined with the latest Particle Data …
Influence of dark matter on the structure of strange quark stars in one-fluid model
This work studies the influence of scalar dark matter on the structural properties of strange
quark stars (SQS) within a one-fluid framework, considering Yukawa interactions between …
quark stars (SQS) within a one-fluid framework, considering Yukawa interactions between …