arXiv (All)
open access
Modelling Dissipative Dynamics of r-mode Instability in Hybrid Stars
Compact star cores reach extreme densities and may contain exotic dense-matter phases. Information about the exotic interiors of rapidly rotating pulsars can be inferred from r-mode oscillations, whose stability is governed by viscous dissipation. In this work, we model a compact star containing a p
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
- The impact of spiral arms on the star formation life cycle#337510
- Experimental and Numerical Studies of the Collapse of Dense Clouds Induced by Herbig–Haro Stellar Jets#1066313
- Inefficient star formation in high Mach number environments II. Numerical simulations and comparison with analytical models#662015
- The CAVITY project - The spatially resolved star formation rate of galaxies in voids#284308
- Reconstructing the orbits of Milky Way dwarf galaxies: A Large Magellanic Cloud perspective#800072
Record · ID 1013196
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