Investigating the equation-of-state, stability and mass-radius relationship of anisotropic and massive neutron stars embedded in \(f(R, T)\) modified gravity
From MaRDI portal
Publication:6625020
DOI10.1142/S0219887824502037MaRDI QIDQ6625020
Ritabrata Biswas, Mayukh Bandyopadhyay
Publication date: 28 October 2024
Published in: International Journal of Geometric Methods in Modern Physics (Search for Journal in Brave)
Macroscopic interaction of the gravitational field with matter (hydrodynamics, etc.) (83C55) Relativistic gravitational theories other than Einstein's, including asymmetric field theories (83D05)
Cites Work
- Cosmology from \(f(R,T)\) theory in a variant speed of light scenario
- Nonperturbative models of quark stars in \(f(R)\) gravity
- Some anisotropic cosmological models in a modified theory of gravitation
- Black holes, cosmological solutions, future singularities, and their thermodynamical properties in modified gravity theories
- \(f(R)\) theories
- Stellar structure models in modified theories of gravity: lessons and challenges
- Charged dilaton, energy, momentum and angular-momentum in teleparallel theory equivalent to general relativity
- Probes and tests of strong-field gravity with observations in the electromagnetic spectrum
- Anisotropic quintessence strange stars in \(f(T)\) gravity with modified Chaplygin gas
- Higher dimensional charged black hole solutions in \(f(R)\) gravitational theories
- On the use of the entropy principle in general relativity.
- Neutron stars in scalar-tensor gravity with quartic order scalar potential
- Modified gravity theories on a nutshell: inflation, bounce and late-time evolution
- <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
- REISSNER–NORDSTRÖM SOLUTIONS AND ENERGY IN TELEPARALLEL THEORY
- REISSNER–NORDSTRÖM SPACE–TIME IN THE TETRAD THEORY OF GRAVITATION
- A singularity-free solution for a charged fluid sphere in general relativity
- Exact Solutions of Einstein's Field Equations
- RECONSTRUCTION OF f(R, T) GRAVITY DESCRIBING MATTER DOMINATED AND ACCELERATED PHASES
- Repulsive gravitational force and quintessence field in f(T) gravity: How anisotropic compact stars in strong energy condition behave
- KERR–NEWMAN SOLUTION AND ENERGY IN TELEPARALLEL EQUIVALENT OF EINSTEIN THEORY
- On Massive Neutron Cores
- Charged rotating black holes coupled with nonlinear electrodynamics Maxwell field in the mimetic gravity
- Static neutron stars perspective of quadratic and induced inflationary attractor scalar-tensor theories
- The confrontation between general relativity and experiment
- Investigation on the stability and quantum phase transition of the charged rotating Kiselev black hole embedded in quintessence field with quantum fluctuation of entropy
- Tolman IV fluid sphere in \(f(R, T)\) gravity
- Nuclear matter equation of state and stability of charged compact stars embedded in \(f(T)\) modified gravity, under cosmic acceleration
This page was built for publication: Investigating the equation-of-state, stability and mass-radius relationship of anisotropic and massive neutron stars embedded in \(f(R, T)\) modified gravity
Report a bug (only for logged in users!)Click here to report a bug for this page (MaRDI item Q6625020)