arXiv (All)
open access
Two sets of potential-density basis pairs for the study of radial perturbations in collisionless spherical stellar systems
The Kalnajs matrix method is a widely used framework for studying the global linear stability and possible Landau damping of collisionless stellar systems. However, for radial perturbations ($l=0$) in three-dimensional spherical models with infinite boundaries, standard biorthogonal sets such as the
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
- Steady-state density large deviations in driven diffusive systems#1105899
- Effects of resolution and local stability on galactic disks: Halo resolution and softening on bar formation#677511
- Effects of resolution and local stability on galactic disks: Halo resolution and softening on bar formation#674313
- The Ring Field Motif#170405
- Slowly rotating condensate dark stars beyond the mean-field approximation#662450
Record · ID 926864
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