Thermal conduction and thermopower of a warm neutron star crust in magnetic fields

arXiv:2512.00874 · astro-ph.HE, astro-ph.SR, nucl-th · Submitted 2025-11-30 · Read on arXiv

astro-ph.HE, astro-ph.SR, nucl-th

Submitted: 2025-11-30

Updated: 2026-09-20

Comments: v2: 20 pages, 20 figures, matches published version

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

Terminology

• Boltzmann Equation — 6× in this paper · explained in 2 episodes
• Core — 5× in this paper · explained in 2 episodes
• Anisotropy — 3× in this paper · explained in 3 episodes
• Trace — 2× in this paper · explained in 2 episodes
• Momentum transfer — 1× in this paper · explained in 2 episodes
• Quantization — 1× in this paper · explained in 12 episodes

Sources

• The Second Born Corrections to the Electrical and Thermal Conductivities of Dense Matter in the Liquid Metal Phase
• Neutron stars - cooling and transport
• Electrical conductivity of warm neutron star crust in magnetic fields: Neutron-drip regime
• Thermal Conductivity and Thermal Hall Effect in Dense Electron-Ion Plasma
• Electron-neutron scattering and transport properties of neutron stars
• Revisiting thermoelectric effects in the crust of neutron stars
• Magnetothermal Evolution of Neutron Stars with Emphasis to Radio Pulsars
• 3D code for MAgneto-Thermal evolution in Isolated Neutron Stars, MATINS: The Magnetic Field Formalism
• 3D code for MAgneto-Thermal evolution in Isolated Neutron Stars, MATINS: thermal evolution and lightcurves
• Unified equations of state for cold non-accreting neutron stars with Brussels-Montreal functionals. I. Role of symmetry energy

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