arXiv (All)
open access
21-cm Constraints on S-wave Dark Matter Annihilation with Subhalo-enhanced Effects
Observations of the 21-cm signal can probe energy injection into the intergalactic medium arising from dark matter annihilation during cosmic dawn and reionization. For s-wave annihilation, the annihilation rate depends on the squared dark matter density, making the 21-cm signal sensitive to dark ma
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
- Dynamical evolution of dark matter subhaloes in the Milky Way: role of the Galactic disc#987715
- Targeting cluster galaxies for the 4MOST CHANCES Low-z sub-survey with photometric redshifts#413247
- Electroweak Doublet Dark Matter for a Galactic Halo Gamma-Ray Excess#798840
- Electroweak Doublet Dark Matter for a Galactic Halo Gamma-Ray Excess#797426
- DESI DR2 Galaxy luminosity functions#495560
Record · ID 1035879
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