WIMPs with Enhanced Annihilation from a Feebly Interacting Unstable Partner
hep-ph, astro-ph.CO, astro-ph.HE, hep-ex
Submitted: 2026-09-15
Updated: 2026-09-15
Comments: 20 pages, 5 figures
License: http://arxiv.org/licenses/nonexclusive-distrib/1.0/
Terminology
Sources
- Precise Relic WIMP Abundance and its Impact on Searches for Dark Matter Annihilation
- Dark Matter Searches at Colliders
- Dark Matter Search Results from 4.2 Tonne-Years of Exposure of the LUX-ZEPLIN (LZ) Experiment
- WIMP Dark Matter Search using a 3.1 Tonne-Year Exposure of the XENONnT Experiment
- Searching for Dark Matter Annihilation in Recently Discovered Milky Way Satellites with Fermi-LAT
- Freeze-In Production of FIMP Dark Matter
- The Effects of Primordial Black Holes on Dark Matter Models
- Constraint on the Reheating Temperature from the Decay of the Polonyi Field
- Wino Cold Dark Matter from Anomaly-Mediated SUSY Breaking
- A Non-thermal WIMP Miracle
- Non-thermal WIMP baryogenesis
- Enhanced Dark Matter Abundance in First-Order Phase Transitions
- Origins of Hidden Sector Dark Matter I: Cosmology
- The Four Basic Ways of Creating Dark Matter Through a Portal
- Minimal Dark Matter Freeze-in with Low Reheating Temperatures and Implications for Direct Detection
- Revisiting Dark Matter Freeze-in and Freeze-out through Phase-Space Distribution
- Cosmological Histories in Neutrino Portal Dark Matter
- An Ultimate Target for Dark Matter Searches
- Planck 2015 results. XIII. Cosmological parameters
- GeV-Scale Thermal WIMPs: Not Even Slightly Dead
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