Thermal evolution of neo-neutron stars. II. Temperature-dependent crusts

arXiv:2608.03732 · astro-ph.HE · Submitted 2026-08-04 · Read on arXiv

Sagnik Chatterjee, Mikhail V. Beznogov, Dany Page, Adriana R. Raduta

astro-ph.HE

Submitted: 2026-08-04

Comments: 10 pages, 11 figures, 1 table; submitted to A&A

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

Terminology

• Core — 27× in this paper · explained in 2 episodes
• Equation of State (EoS) — 3× in this paper · explained in 4 episodes
• Clustering — 1× in this paper · explained in 2 episodes

Related papers

• Numerical Studies of Accretion Flows onto a Neutron Star Engulfed in a Massive Star
• Collisionless Accretion of Finite-Angular-Momentum Plasma onto a Spinning Black Hole
• Impact of Magnetic Field Topology on Electromagnetic and Gravitational Waves from Binary Neutron Star Merger Remnants
• XRISM Resolve Spectroscopy of GX 5-1: Constraints on Iron Spectral Features in a Luminous Neutron-Star Binary
• SN 1006: A Cosmic Laboratory for Investigating Shock Acceleration Physics
• Neutrino Spectral Pinching in 3D Core-Collapse Supernovae: Late-Time Convergence, Failed-Explosion Signatures, and Viewing-Angle Dispersion