Stationarity and angular momentum conservation in pulsar spin noise

arXiv:2610.01929 · astro-ph.HE, astro-ph.IM, cond-mat.stat-mech · Submitted 2026-10-01 · Read on arXiv

astro-ph.HE, astro-ph.IM, cond-mat.stat-mech

Submitted: 2026-10-01

Updated: 2026-10-01

Comments: 21 pages + refs, 12 figures, comments welcome

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

Terminology

• Core — 12× in this paper · explained in 2 episodes
• Bayesian Inference — 6× in this paper · explained in 5 episodes
• Regularization — 3× in this paper · explained in 3 episodes
• Consistency — 2× in this paper · explained in 3 episodes
• Calibration — 1× in this paper · explained in 7 episodes
• Entrainment — 1× in this paper · explained in 2 episodes
• Parameter Identifiability — 1× in this paper · explained in 2 episodes
• Vortex Pinning — 1× in this paper · explained in 2 episodes

Sources

• Stochastic problems in pulsar timing
• Gravitational waves from isolated neutron stars
• Radio Pulsars: The Neutron Star Population & Fundamental Physics
• Search for continuous gravitational waves from the pulsar J0435+3233
• Probing neutron stars with gravitational waves

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