Planck Mass Charged Gravitino Dark Matter
arXiv:1809.01441 · doi:10.1103/PhysRevD.100.035001
Abstract
Following up on our earlier work predicting fractionally charged supermassive gravitinos, we explain their potential relevance as novel candidates for Dark Matter and discuss possible signatures and ways to detect them.
Version accepted for publication in Phys. Rev. D
References in corpus (11)
- Dark Matter Search Results from a One TonneYear Exposure of XENON1T
- Results from a search for dark matter in the complete LUX exposure
- Turning off the Lights: How Dark is Dark Matter?
- First model independent results from DAMA/LIBRA-phase2
- Dark Matter Candidates: A Ten-Point Test
- Reopening the window on charged dark matter
- Theory and Phenomenology of Planckian Interacting Massive Particles as Dark Matter
- Saturated Overburden Scattering and the Multiscatter Frontier: Discovering Dark Matter at the Planck Mass and Beyond
- Trans-Planckian wimpzillas
- Standard Model Fermions and N=8 supergravity
- Standard Model Fermions and Infinite-Dimensional R-Symmetries
Cited by in corpus (13)
- Direct Detection Limits on Heavy Dark Matter
- Simulating the LOcal Web (SLOW) II: Properties of local galaxy clusters
- Inflation, Gravity Mediated Supersymmetry Breaking, and de Sitter Vacua in Supergravity with a Kähler-Invariant FI Term
- Asymmetric Dark Matter from Gravitational Waves
- Supermassive gravitinos and giant primordial black holes
- Superheavy Gravitinos and Ultra-High Energy Cosmic Rays
- Baryonic and Leptonic GeV Dark Matter
- A Realization of Slow Roll Inflation and the MSSM in Supergravity Theories with New Fayet-Iliopoulos Terms
- Charge transport in chiral solids as a possible tool in search of dark matter signals
- Shedding Light on Dark Sectors with Gravitational Waves
- Models of ultra-heavy dark matter visible to macroscopic mechanical sensing arrays
- Signatures of supermassive charged gravitinos in liquid scintillator detectors
- Charged topological geons with a self-gravitating scalar field