Dark-matter relay for ultra-high-energy cosmic rays
astro-ph.HE, hep-ph
Submitted: 2026-09-22
Updated: 2026-09-22
Comments: 6 pages, 2 figures
License: http://arxiv.org/licenses/nonexclusive-distrib/1.0/
Terminology
Sources
- An extremely energetic cosmic ray observed by a surface detector array
- Testing the correlations between ultra-high-energy cosmic rays and BL Lac type objects with HiRes stereoscopic data
- Search for Cross-Correlations of Ultra--High-Energy Cosmic Rays with BL Lacertae Objects
- Is astronomy possible with neutral ultra-high energy cosmic ray particles existing in the Standard Model?
- Anomalous cosmic-ray correlations revisited with a complete full-sky sample of BL Lac type objects
- Dark Sectors and New, Light, Weakly-Coupled Particles
- Search for Light Dark Matter with accelerator and direct detection experiments: comparison and complementarity of recent results
- Enhanced Cosmic-Ray Cooling in AGN from Dark Matter Deep Inelastic Scattering
- Search for Light Dark Matter with NA64 at CERN
- New parton distribution functions from a global analysis of quantum chromodynamics
- Implications of a Froissart bound saturation of $\gamma^*$-$p$ deep inelastic scattering. Part I. Quark distributions at ultra small $x$
- Implications of a Froissart bound saturation of $\gamma^*$-$p$ deep inelastic scattering. Part II. Ultra-high energy neutrino interactions
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