Strong magnetic field inside degenerate relativistic plasma and the impacts on the neutrino transport in Core-Collapse Supernovae

arXiv:2405.11555 · astro-ph.HE, astro-ph.SR, hep-ph · Submitted 2024-05-19 · Read on arXiv

astro-ph.HE, astro-ph.SR, hep-ph

Submitted: 2024-05-19

Updated: 2026-09-15

Comments: 25 pages, 10 figures, published in Chin. Phys. C

Journal ref: Chin.Phys.C 50 (2026) 8, 084101

DOI: 10.1088/1674-1137/ae6b21

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

Terminology

• Core — 28× in this paper · explained in 2 episodes
• Abundance — 4× in this paper · explained in 1 episode
• Degeneracy — 4× in this paper · explained in 3 episodes
• Metallicity — 2× in this paper · explained in 3 episodes
• Quantization — 2× in this paper · explained in 12 episodes
• Absorption Cross Section — 1× in this paper · explained in 1 episode
• Accretion Shock — 1× in this paper · explained in 1 episode
• Accuracy — 1× in this paper · explained in 1 episode
• Chinese Academy of Sciences — 1× in this paper
• Equation of State (EoS) — 1× in this paper · explained in 4 episodes

Sources

• Neutrino-Neutron Scattering Opacities in Supernova Matter
• Coalescing Neutron Stars -- a Step Towards Physical Models. I. Hydrodynamic Evolution and Gravitational-Wave Emission

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