Neutrino As The Dark Force
arXiv:2106.08339 · doi:10.1103/PhysRevD.104.075010
Abstract
We point out a novel role for the Standard Model neutrino in dark matter phenomenology where the exchange of neutrinos generates a long-range potential between dark matter particles. The resulting dark matter self interaction could be sufficiently strong to impact small-scale structure formation, without the need of any dark force carrier. This is a generic feature of theories where dark matter couples to the visible sector through the neutrino portal. It is highly testable with improved decay rate measurements at future , Higgs, and factories, as well as precision cosmology.
6 pages, 2 figures; v2: added Lyman-alpha and references
References in corpus (19)
- The automated computation of tree-level and next-to-leading order differential cross sections, and their matching to parton shower simulations
- Constraints on the Self-Interaction Cross-Section of Dark Matter from Numerical Simulations of the Merging Galaxy Cluster 1E 0657-5
- New Fixed-Target Experiments to Search for Dark Gauge Forces
- The non-gravitational interactions of dark matter in colliding galaxy clusters
- Stellar Feedback in Dwarf Galaxy Formation
- Is dark matter with long-range interactions a solution to all small-scale problems of ΛCDM cosmology?
- Opening a new window for warm dark matter
- Searches for invisible decays of the Higgs boson in pp collisions at sqrt(s) = 7, 8, and 13 TeV
- BBN And The CMB Constrain Neutrino Coupled Light WIMPs
- Cosmological bounds on dark matter-neutrino interactions
- Interacting neutrinos in cosmology: exact description and constraints
- MDM: A Model for Sterile Neutrino and Dark Matter Reconciles Cosmological and Neutrino Oscillation Data after BICEP2
- Self-interacting inelastic dark matter: A viable solution to the small scale structure problems
- Constraining dark matter-neutrino interactions with IceCube-170922A
- Self-interacting Dark Matter Without Direct Detection Constraints
- Dark Matter and Neutrino Mass from the Smallest Non-Abelian Chiral Dark Sector
- Naturally Light Sterile Neutrinos from Theory of R-parity
- Long-lived Light Mediator to Dark Matter and Primordial Small Scale Spectrum
- Spin-Independent Two-Neutrino Exchange Potential with Mixing and -Violation