Pulsars: Cosmic Permanent 'Neutromagnets'?
Johan Hansson, Anna Ponga

TL;DR
The paper proposes that pulsars could be spin-polarized neutron stars acting as cosmic permanent magnets, potentially explaining key observational features like beam stability and magnetic field limits.
Contribution
It introduces a speculative model suggesting pulsars are neutron stars with permanent magnet-like properties, offering explanations for observed pulsar phenomena.
Findings
Explains the stability of pulsar beams
Accounts for the magnetic field upper limit
Proposes a new magnetic origin for pulsar behavior
Abstract
We argue that pulsars may be spin-polarized neutron stars, i.e. cosmic permanent magnets. This would simply explain several observational facts about pulsars, including the 'beacon effect' itself i.e. the static/stable misalignment of rotational and magnetic axes, the extreme temporal stability of the pulses and the existence of an upper limit for the magnetic field strength - coinciding with the one observed in "magnetars". Although our model admittedly is speculative, this latter fact seems to us unlikely to be pure coincidence.
Peer Reviews
No public reviews on file for this paper yet. If you reviewed it on a platform where reviews are public (OpenReview, ICLR, NeurIPS, ICML), you can paste yours below so the community can read it here.
Videos
No videos yet. Explain this paper in a talk, walkthrough, or lecture? Add one.
