arXiv (All)
open access
Probing Dense Nuclear Matter at Small-x: A workflow for a global analysis framework
The dipole model provides a powerful framework for describing high-energy nuclear interactions, particularly in the regime of dense gluonic matter. However, accurately evolving the dipole--nucleus scattering amplitude remains a major computational challenge because it is governed by nonlinear QCD ev
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
- Nuclear Deep Inelastic Scattering around $x=0.3$#1143220
- Finite Temperature NLO Corrections in Relativistic Scatterings: Implications for Dark Matter Freeze-In#1012168
- Search for dark matter production in association with a single top quark in proton-proton collisions at √s=13 TeV#231818
- Isospin dependence of the nuclear EMC effect from a global QCD analysis#679613
- The Seoul National University AGN Monitoring Project. III. Hβ Lag Measurements of 32 Luminous Active Galactic Nuclei and the High-luminosity End of the Size–Luminosity Relation#398473
Record · ID 999300
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