Pulsar anti-glitches: starquakes driven by magnetism?

arXiv:2607.12285 · astro-ph.HE · Submitted 2026-07-14 · Read on arXiv

Hanyuan Long, Ruipeng Lu, Weiyang Wang, Shunshun Cao, Hao Tong, Han Yue, Renxin Xu

astro-ph.HE

Submitted: 2026-07-14

Comments: RAA sumbitted

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

Terminology

• Aperture — 1× in this paper · explained in 1 episode

Sources

• Discovery of the first anti-glitch event in the rotation-powered pulsar PSR B0540-69

Related papers

• Accreting Neutron Stars in Low-Mass X-ray Binaries
• 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