arXiv (All)
open access
Milky Way White Dwarfs as Inelastic Dark Matter Detectors
We show that white dwarfs in the Galactic Center are a sensitive probe of inelastic dark matter (IDM) annihilation. IDM particles traversing a white dwarf may become gravitationally captured without fully settling in its interior if their energy drops below the kinematic threshold for inelastic scat
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
- Improved Heavy Dark Matter Annihilation Search from Dwarf Galaxies with HAWC#1070759
- Exploring spatially resolved metallicities, dynamics, and outflows in low-mass galaxies at z ∼ 7.6#1065846
- A study of transients from ground-based surveys reveals new ultra-compact accreting white dwarf binaries#206097
- Rotational Spectrum and First Interstellar Detection of 2-methoxyethanol Using ALMA Observations of NGC 6334I#612925
- Too small to fail: characterizing sub-solar mass black hole mergers with gravitational waves#986761
Record · ID 1115806
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