WIMPs with GUTs: Dark Matter Coannihilation with a Lighter Species
arXiv:1704.08256 · doi:10.1103/PhysRevLett.119.121801
Abstract
We propose a new thermal freeze-out mechanism for ultra-heavy dark matter. Dark matter coannihilates with a lighter unstable species, leading to an annihilation rate that is exponentially enhanced relative to standard WIMPs. This scenario destabilizes any potential dark matter candidate. In order to remain consistent with astrophysical observations, our proposal necessitates very long-lived states, motivating striking phenomenology associated with the late decays of ultra-heavy dark matter, potentially as massive as the scale of grand unified theories, GeV.
5 pages, 2 figures
References in corpus (13)
- Results from a search for dark matter in the complete LUX exposure
- Secluded WIMP Dark Matter
- Dark Matter Results from First 98.7-day Data of PandaX-II Experiment
- Reheating in Inflationary Cosmology: Theory and Applications
- Updated fit to three neutrino mixing: status of leptonic CP violation
- Reheating constraints to inflationary models
- Reheating predictions in single field inflation
- Gamma-ray Constraints on Decaying Dark Matter and Implications for IceCube
- Inflation and the Scale Dependent Spectral Index: Prospects and Strategies
- Thermal Dark Matter From A Highly Decoupled Sector
- Changes in Dark Matter Properties After Freeze-Out
- Superheavy Thermal Dark Matter and Primordial Asymmetries
- Light Dark Matter through Assisted Annihilation
Cited by in corpus (22)
- Proposal for gravitational direct detection of dark matter
- Super heavy thermal dark matter
- Heavy Thermal Relics from Zombie Collisions
- Testing Super-Heavy Dark Matter from Primordial Black Holes with Gravitational Waves
- Recycled Dark Matter
- Probing superheavy dark matter with gravitational waves
- Hunting super-heavy dark matter with ultra-high energy photons
- Dark matter produced from right-handed neutrinos
- Dark Matter from Exponential Growth
- Dark matter as a heavy thermal hot relic
- Annihilating Dark Matter Search with 12 Years of Fermi LAT Data in Nearby Galaxy Clusters
- Getting a THUMP from a WIMP
- Roadmap to Thermal Dark Matter Beyond the WIMP Unitarity Bound
- Sub-MeV Self Interacting Dark Matter
- Mass-varying Dark Matter from a Phase Transition
- Bouncing Dark Matter
- Probing Superheavy Dark Matter with Exoplanets
- Models of ultra-heavy dark matter visible to macroscopic mechanical sensing arrays
- Ultraheavy Atomic Dark Matter Freeze-Out through Rearrangement
- Mesotuned WIMPs and Avoided Deconfinement
- Producing and constraining self-interacting hidden sector dark matter
- Probing Heavy Dark Matter in Red Giants