arXiv (All)
open access
Dark Photons in the Radio Sky: II. Resonant Conversions in the Intergalactic Medium
This is the second in a pair of papers forecasting the sensitivity of the Square Kilometre Array (SKA) to dark photons, a highly motivated, simple extension of the Standard Model. Through a kinetic mixing term, visible photons from the cosmic microwave background can resonantly convert into dark pho
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 Morphology, Color, and Gas Content of Low Surface Brightness Galaxies#639492
- Signature of Axion Dark Matter in Low-Frequency Terrestrial Electromagnetic Fields: Formulation and Predictions#433643
- Signature of Axion Dark Matter in Low-Frequency Terrestrial Electromagnetic Fields: Formulation and Predictions#433636
- Halo mass, star formation, and morphology in galaxies: A morphology-dependent connection between halo environment and star formation activity#972670
- Stellar masses of optically dark galaxies: uncertainty introduced by the attenuation law and star-formation histories#1063828
Record · ID 1014570
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