Velocities of pulsars and neutrino oscillations

Alexander Kusenko; Gino Segre (University of Pennsylvania)

Velocities of pulsars and neutrino oscillations

Not yet reviewed by Pith; the record is open.

Re-run · record.json Download PDF Read on arXiv ↗

This paper has not been read by Pith yet. Machine review is queued; the pith claim, tier, and objections will appear here once it completes.

SPECIMEN: schema-true, not a live event

T0 review · schema-true

One-sentence machine reading of the paper's core claim.

pith:XXXXXXXX · record.json · timestamp

arxiv hep-ph/9606428 v2 pith:DT4WILPI submitted 1996-06-25 hep-ph astro-phgr-qc

Alexander Kusenko , Gino Segre (University of Pennsylvania) This is my paper · ORCID

classification hep-phastro-phgr-qc

keywords neutrinooscillationspulsarsvelocitiesalteranisotropybiasedcollapse

verification ladder T0 review T1 audit T2 compute T3 formal

0 comments

read the original abstract

Neutrino oscillations, biased by the magnetic field, alter the shape of the neutrinosphere in a cooling protoneutron star emerging from the supernova collapse. The resulting anisotropy in the momentum of outgoing neutrinos can be the origin of the observed proper motions of pulsars. The connection between the pulsars velocities and neutrino oscillations results in a prediction for the tau neutrino mass of order 100 eV.

Discussion (0). Continue with ORCID to comment.

Forward citations

Cited by 1 Pith paper

Reviewed papers in the Pith corpus that reference this work. Sorted by Pith novelty score. Full citation record

FCL-COD: Weakly Supervised Camouflaged Object Detection with Frequency-aware and Contrastive Learning
cs.CV 2026-03 unverdicted novelty 5.0 of 10

FCL-COD adapts SAM with frequency-aware LoRA and gradient-aware contrastive learning and claims to outperform both weakly and fully supervised camouflaged object detectors on three benchmarks.

Pith tools