arXiv (All)
open access
Axial Quasi-normal Modes of Boson-Fermion Stars
We study axial quasi-normal modes of boson-fermion stars composed of ordinary nuclear matter and a self-interacting bosonic dark matter component. The equilibrium configurations are obtained by solving the coupled two-fluid Tolman-Oppenheimer-Volkoff equations, where the neutron sector is modeled wi
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
- Reconstructing the Dark Matter Equation of State with Compact Object Inspirals#1070271
- Gravitational Imprints of Dark Energy in Neutron Stars#1061817
- Hyperon bulk viscosity effects in neutron-star inspirals#784771
- Hyperon bulk viscosity effects in neutron-star inspirals#783181
- Searching for quasinormal modes from Binary Black Hole mergers#173321
Record · ID 987670
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