Classification of pulsars into bimodal kick modes shows low-B objects overabundant in the low-velocity mode, with no high-velocity examples below 10^11 G.
URL https://link.aps.org/doi/10.1103/ PhysRevD.110.083025
2 Pith papers cite this work. Polarity classification is still indexing.
2
Pith papers citing it
fields
astro-ph.HE 2years
2026 2verdicts
UNVERDICTED 2representative citing papers
A minimalist analytic extension shows spin-kick alignment in the tug-boat mechanism arises either from fast rotation averaging out perpendicular asymmetries or from spin-aligned mass flux, but the former requires unrealistically high rotation unless magnetic angular-momentum transport is efficient.
citing papers explorer
-
Kick bimodality of neutron stars and mode dependence of their parameters
Classification of pulsars into bimodal kick modes shows low-B objects overabundant in the low-velocity mode, with no high-velocity examples below 10^11 G.
-
Effects of Rotation on the Gravitational Tug-Boat Mechanism for Neutron-Star Kicks and Implications for Spin-Kick Alignment
A minimalist analytic extension shows spin-kick alignment in the tug-boat mechanism arises either from fast rotation averaging out perpendicular asymmetries or from spin-aligned mass flux, but the former requires unrealistically high rotation unless magnetic angular-momentum transport is efficient.