Nuclear matter equation of state and stability of charged compact stars embedded in \(f(T)\) modified gravity, under cosmic acceleration
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Publication:6557307
DOI10.1142/S021988782450097XzbMATH Open1543.83032MaRDI QIDQ6557307
Mayukh Bandyopadhyay, Ritabrata Biswas
Publication date: 18 June 2024
Published in: International Journal of Geometric Methods in Modern Physics (Search for Journal in Brave)
Relativistic cosmology (83F05) Macroscopic interaction of the gravitational field with matter (hydrodynamics, etc.) (83C55)
Cites Work
- Extended gravity description for the GW190814 supermassive neutron star
- Stellar structure models in modified theories of gravity: lessons and challenges
- Static charged gas spheres in General Relativity
- <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
- Repulsive gravitational force and quintessence field in f(T) gravity: How anisotropic compact stars in strong energy condition behave
- Stability of motion and thermodynamics in charged black holes in f(T) gravity
- Rotating AdS black holes in Maxwell- f ( T ) gravity
- Radially symmetric distribution of matter
- Ultra-compact spherically symmetric dark matter charged star objects
- Charged stellar structure in Tolman–Kuchowicz spacetime
Related Items (2)
Isolated compact star \(RXJ 1856.5 - 3754\) in \(f(R, T)\) modified gravity in Tolman-Kuchowicz spacetime ⋮ Investigating the equation-of-state, stability and mass-radius relationship of anisotropic and massive neutron stars embedded in \(f(R, T)\) modified gravity
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