Influence of pressure anisotropy on mass-radius relation and stability of millisecond pulsars in \(f(Q)\) gravity
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Publication:6618122
DOI10.1088/1475-7516/2024/09/048zbMATH Open1548.83115MaRDI QIDQ6618122
G. Mustafa, S. K. Maurya, Megandhren Govender, Abdul Aziz, Ksh. Newton Singh, Abdelghani Errehymy
Publication date: 14 October 2024
Published in: Journal of Cosmology and Astroparticle Physics (Search for Journal in Brave)
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Cites Work
- Title not available (Why is that?)
- \(f(R)\) theories
- Q-stars in anti de Sitter spacetime
- Extended gravity description for the GW190814 supermassive neutron star
- The large \(N\) limit of superconformal field theories and supergravity
- Boson stars with negative cosmological constant
- Baryons and branes in anti-de Sitter space
- Spinning gauged boson stars in anti-de Sitter spacetime
- Decoupling gravitational sources in general relativity: the extended case
- Quantum gravity slows inflation
- Trace-anomaly driven inflation in \(f(T)\) gravity and in minimal massive bigravity
- Model-independent reconstruction of \(f(Q)\) non-metric gravity
- Modified gravity theories on a nutshell: inflation, bounce and late-time evolution
- Compact objects in Horndeski gravity
- Stability of charged solitons and formation of boson stars in five-dimensional anti-de Sitter spacetime
- <mml:math xmlns:mml="http://www.w3.org/1998/Math/MathML" display="inline"><mml:mrow><mml:mi>f</mml:mi><mml:mrow><mml:mo>(</mml:mo><mml:mi>R</mml:mi><mml:mo>)</mml:mo></mml:mrow></mml:mrow></mml:math>theories of gravity
- Radial pulsations and stability of anisotropic stars with a quasi-local equation of state
- INTRODUCTION TO MODIFIED GRAVITY AND GRAVITATIONAL ALTERNATIVE FOR DARK ENERGY
- Some models of anisotropic spheres in general relativity
- Anisotropic stars in general relativity
- What if string theory has no de Sitter vacua?
- Strange stars inf(R,𝒯) gravity
- Generalized teleparallel cosmology and initial singularity crossing
- Exploring physical properties of minimally deformed strange star model and constraints on maximum mass limit in f(𝒬) gravity
- Study on charged strange stars in f(R, T) gravity
- Standard cosmology on the Anti-de Sitter boundary
- The Dynamical Instability of Gaseous Masses Approaching the Schwarzschild Limit in General Relativity.
- The Large Scale Structure of Space-Time
- Dynamical Instability of Gaseous Masses Approaching the Schwarzschild Limit in General Relativity
- Static Solutions of Einstein's Field Equations for Spheres of Fluid
- On Massive Neutron Cores
- Anti-de Sitter neutron stars in the theory of gravity with nonminimal derivative coupling
- On the viability of f(Q) gravity models
- Complexity‐Free Anisotropic Solution of Buchdahl's Model and Energy Exchange Between Relativistic Fluids by Extended Gravitational Decoupling
- Gravitational waves in \(f(Q)\) non-metric gravity via geodesic deviation
- Hamiltonian Analysis of f(Q)$f(\mathbb {Q})$ Gravity and the Failure of the Dirac–Bergmann Algorithm for Teleparallel Theories of Gravity
- Review on \(f(\mathbb{Q})\) gravity
- Impact of \(f(Q)\) gravity on anisotropic compact star model and stability analysis
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