arXiv (OAI Expanded)
open access
Vortex pinning and the elastic response of neutron-star crusts II. Non-axisymmetric loading and Magnus mountains
Pinned superfluid vortices transmit a Magnus force to the neutron-star crust. A non-axisymmetric component of the superfluid-lattice lag can therefore support a persistent mass quadrupole. We calculate the l=m=2 response of self-gravitating, radially stratified spherical stars with SLy4 and BSk21 ba
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
- Vortex pinning and the elastic response of neutron-star crusts II. Non-axisymmetric loading and Magnus mountains#924981
- Spin effects in superfluidity, neutron matter and neutron stars#1048622
- Coherent spectroscopy of collective excitations in superfluid helium far from equilibrium#819373
- Coherent spectroscopy of collective excitations in superfluid helium far from equilibrium#809380
- The Magnetic Fields of the Universe and Their Origin#639379
Record · ID 920747
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