E-Wimps
arXiv:hep-ph/0511003 · doi:10.1063/1.2149672
Abstract
Extremely weakly interacting massive particles (E-WIMPs) are intriguing candidates for cold dark matter in the Universe. We review two well motivated E-WIMPs, an axino and a gravitino, and point out their cosmological and phenomenological similarities and differences, the latter of which may allow one to distinguishing them in LHC searches for supersymmetry.
7 pages, plenary talk given by L. Roszkowski at PASCOS-05, Gyeongju, Korea
Cited by in corpus (57)
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- Dark matter production in the early Universe: beyond the thermal WIMP paradigm
- Dark Matter Candidates: A Ten-Point Test
- Extra-weakly Interacting Dark Matter
- The Effects of Primordial Black Holes on Dark Matter Models
- Theory and Phenomenology of Planckian Interacting Massive Particles as Dark Matter
- The singlet scalar as FIMP dark matter
- Neutralino dark matter from heavy axino decay
- Self-interacting Dark Matter from Primordial Black Holes
- Gravitational dark matter production: primordial black holes and UV freeze-in
- Warm and cold fermionic dark matter via freeze-in
- Reconstructing Non-standard Cosmologies with Dark Matter
- Ultraviolet Freeze-in with a Time-dependent Inflaton Decay
- WIMPs during Reheating
- From WIMPs to FIMPs with Low Reheating Temperatures
- Determining Reheating Temperature at Colliders with Axino or Gravitino Dark Matter
- Fermion Masses and Mixings and Dark Matter Constraints in a Model with Radiative Seesaw Mechanism
- Boosting Freeze-in through Thermalization
- Boosting Ultraviolet Freeze-in in NO Models
- A Two-Component Dark Matter Model and its Associated Gravitational Waves
- Dark Matter and Leptogenesis from Gravitational Production
- Naturally small Yukawa couplings from trans-Planckian asymptotic safety
- Quintessential Kination and Thermal Production of Gravitinos and Axinos
- Gauged Inverse Seesaw from Dark Matter
- Hidden strongly interacting massive particles
- Polynomial Inflation and Dark Matter
- Non-thermal production of Dark Matter after Inflation
- An intermediate framework between WIMP, FIMP, and EWIP dark matter
- A two-component vector WIMP -- fermion FIMP dark matter model with an extended seesaw mechanism
- Kaluza-Klein FIMP Dark Matter in Warped Extra-Dimensions
- Non-minimally Coupled Vector Boson Dark Matter
- From WIMPs to FIMPs: Impact of Early Matter Domination
- Constraints on solutions to the flavor anomalies with trans-Planckian asymptotic safety
- Matter Power Spectrum of Light Freeze-in Dark Matter: With or without Self-Interaction
- Freeze-in Axion-like Dark Matter
- Unitarity Bound on Dark Matter in Low-temperature Reheating Scenarios
- FIMP Dark Matter in Clockwork/Linear Dilaton Extra-Dimensions
- Inflection-point Inflation and Dark Matter Redux
- Tracking Quintessence and Cold Dark Matter Candidates
- FIMP dark matter mediated by massive gauge boson around the phase transition period and the gravitational waves production
- Baryogenesis and Dark Matter from Freeze-In
- Freeze-in, glaciation, and UV sensitivity from light mediators
- Sterile neutrino dark matter with dipole interaction
- Stau detection at neutrino telescopes in scenarios with supersymmetric dark matter
- Mass-varying Dark Matter from a Phase Transition
- Analysis of techni-dilaton as a dark matter candidate
- Frozen-in fermionic singlet dark matter in non-standard cosmology with a decaying fluid
- Phenomenological and cosmological implications of a scotogenic three-loop neutrino mass model
- Dark Matter in a bi-metric universe
- Stabilizing dark matter with quantum scale symmetry
- Unraveling particle dark matter with Physics-Informed Neural Networks
- Post-inflationary production of particle Dark Matter: Hilltop and Coleman-Weinberg inflation
- Dark matter production accompanied by gravitational wave signals during cosmological phase transitions
- Mesotuned WIMPs and Avoided Deconfinement
- Modified Supersymmetric Dark Sectors
- Oscillation Baryogenesis via Ultraviolet Dark Matter Freeze-In
- Freeze-in Leptogenesis via Dark-Matter Oscillations