arXiv (All)
open access
Unveiling dark forces with measurements of the Large Scale Structure of the Universe
Cosmology offers opportunities to test Dark Matter independently of its interactions with the Standard Model. We study the imprints of long-range forces acting solely in the dark sector on the distribution of galaxies, the so-called Large Scale Structure (LSS). We derive the strongest constraint on
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
- Probing For Non-Gravitational Galactic-Range Dark Matter Interactions#1155056
- Dark Matter Science in the Era of LSST#798510
- Dark Matter Science in the Era of LSST#797097
- A New Dark Matter Model for Galaxies#639549
- Rubin LSST DP2 unveils almost-dark galaxies in the Virgo Cluster#1013844
Record · ID 1402883
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