arXiv (All)
open access
Effects of Rotation on the Gravitational Momentum Transfer in Neutron-Star Kicks and Implications for Spin-Kick Alignment
Neutron stars are often born with large recoil velocities, or natal kicks, whose physical origin remains an open question in core-collapse supernova theory. Observations suggest that the spin-kick angle distribution is not isotropic but skewed toward a spin-kick vector alignment. One possible kick m
Conceptio Open Archive
Analyze & explore related research in Conceptio
Connect this record directly into your research workflow or AI agent. Explore citations across open repositories, query full text, and export structured proof bundles.
This document is indexed with metadata only: full text is not available in the archive for this record. Open the official source ↗
Related documents
- Effects of Rotation on 3D Core-Collapse Supernova Models for Low-Mass Progenitors#1109099
- Radial differential rotation leading to dipole collapse in pre-main-sequence stars#624693
- GRMHD Simulations of Accreting Proto-Magnetars I. Implications for Gamma-Ray Burst Jets and Energetic Explosions#819642
- GRMHD Simulations of Accreting Proto-Magnetars I. Implications for Gamma-Ray Burst Jets and Energetic Explosions#809646
- STRONGLY DEFORMED NUCLEAR SHAPES AT ULTRA-HIGH SPIN AND SHAPE COEXISTENCE IN N ∼ 90 NUCLEI#611966
Record · ID 927350
Retrieved via Conceptio: every document is proof-bundled with source, license, and retrieval metadata.
Retrieved via Conceptio: every document is proof-bundled with source, license, and retrieval metadata.
Bring this data into your agent: Connect via MCP or API · 20 free credits to start · no card required
Read the Docs → · View CLI source on GitHub · Conceptio Open Knowledge Archive
Read the Docs → · View CLI source on GitHub · Conceptio Open Knowledge Archive