Structure of Anisotropic Magnetized Neutron Stars in f(R,T) Gravity with Realistic Equation of State

arXiv:2607.05333 · gr-qc, astro-ph.SR, nucl-th · Submitted 2026-07-06 · Read on arXiv

M. Savari, G. H. Bordbar, J. Sedaghat, A. Sheykhi

gr-qc, astro-ph.SR, nucl-th

Submitted: 2026-07-06

Comments: 17 pages, 10 figures, 7 tables (Physics Letters B (2026) accepted for publication)

Journal ref: Physics Letters B 880 (2026) 140733

DOI: 10.1016/j.physletb.2026.140733

License: http://arxiv.org/licenses/nonexclusive-distrib/1.0/

Terminology

• Anisotropy — 35× in this paper · explained in 3 episodes
• Consistency — 3× in this paper · explained in 3 episodes
• Core — 3× in this paper · explained in 2 episodes
• Trace — 3× in this paper · explained in 2 episodes
• Equation of State (EoS) — 2× in this paper · explained in 4 episodes
• Cluster expansion — 1× in this paper · explained in 2 episodes
• Computational Tractability — 1× in this paper · explained in 2 episodes
• Degeneracy — 1× in this paper · explained in 3 episodes
• Magnetohydrodynamics (MHD) — 1× in this paper · explained in 3 episodes
• Momentum transfer — 1× in this paper · explained in 2 episodes
• Physical Constraints — 1× in this paper · explained in 7 episodes

Related papers

• Tests of General Relativity with Einstein Telescope
• Unitary quantum matter-bounce in a universe with a positive cosmological constant
• Quasi-pole quintessential inflation in metric-affine gravity
• Dynamical tidal response of neutron stars: From effective field theory to gravitational waveforms
• Limits of the Rastall--Einstein Equivalence: Matter-Action Compatibility, FLRW Dynamics, and Exceptional Sectors
• Boson star-black hole binaries: initial data and head-on collisions