The swept-back multipolar magnetic field of neutron stars: Application to NICER MSP J0030+0451

arXiv:2604.19534 · astro-ph.HE · Submitted 2026-04-21 · Read on arXiv

astro-ph.HE

Submitted: 2026-04-21

Updated: 2026-09-17

Comments: The Astrophysical Journal, 2026, Volume 1008, Issue 2, id.215, 23 pp. Interactive figures are available in the published version

Journal ref: The Astrophysical Journal, 2026, Volume 1008, Issue 2, id.215, 23 pp

DOI: 10.3847/1538-4357/ae8e6f

Code: https://github.com/golmschenk/haplo

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

Terminology

Accuracy — 5× in this paper · explained in 1 episode
Benchmark — 2× in this paper · explained in 2 episodes
Consistency — 2× in this paper · explained in 3 episodes
Core — 2× in this paper · explained in 2 episodes
Fidelity — 2× in this paper · explained in 2 episodes
Interpretability — 2× in this paper · explained in 15 episodes
Anisotropy — 1× in this paper · explained in 3 episodes
Clustering — 1× in this paper · explained in 2 episodes
Degeneracy — 1× in this paper · explained in 3 episodes
Equation of State (EoS) — 1× in this paper · explained in 4 episodes
Fine-Tuning — 1× in this paper · explained in 5 episodes
Generalizability — 1× in this paper · explained in 6 episodes
Geodesic Integration in Kerr Spacetime — 1× in this paper
Loss Function — 1× in this paper · explained in 2 episodes
Robustness — 1× in this paper · explained in 5 episodes

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