Z-portal Continuum Dark Matter
arXiv:2105.14023 · doi:10.1103/PhysRevLett.128.081807
Abstract
We examine the possibility that dark matter (DM) consists of a gapped continuum, rather than ordinary particles. A Weakly-Interacting Continuum (WIC) model, coupled to the Standard Model via a Z-portal, provides an explicit realization of this idea. The thermal DM relic density in this model is naturally consistent with observations, providing a continuum counterpart of the "WIMP miracle". Direct detection cross sections are strongly suppressed compared to ordinary Z-portal WIMP, thanks to a unique effect of the continuum kinematics. Continuum DM states decay throughout the history of the universe, and observations of cosmic microwave background place constraints on potential late decays. Production of WICs at colliders can provide a striking cascade-decay signature. We show that a simple Z-portal WIC model provides a fully viable DM candidate consistent with all current experimental constraints.
arXiv comment9 pages, 5 figures; Version published in PRL
References in corpus (40)
- Planck 2015 results. XIII. Cosmological parameters
- A Large Mass Hierarchy from a Small Extra Dimension
- Particle Dark Matter: Evidence, Candidates and Constraints
- Supersymmetric Dark Matter
- Dark Matter Search Results from a One TonneYear Exposure of XENON1T
- Results from a search for dark matter in the complete LUX exposure
- Dark Matter Results From 54-Ton-Day Exposure of PandaX-II Experiment
- Big-Bang Nucleosynthesis and Hadronic Decay of Long-Lived Massive Particles
- Unparticle Physics
- Excess Electronic Recoil Events in XENON1T
- Searching for Dark Matter Annihilation in Recently Discovered Milky Way Satellites with Fermi-LAT
- Indirect Dark Matter Signatures in the Cosmic Dark Ages I. Generalizing the Bound on s-wave Dark Matter Annihilation from Planck
- Updated Nucleosynthesis Constraints on Unstable Relic Particles
- General Constraints on Dark Matter Decay from the Cosmic Microwave Background
- Cosmological constraints on exotic injection of electromagnetic energy
- Experimental evidence of neutrinos produced in the CNO fusion cycle in the Sun
- Supernova Relic Neutrino Search at Super-Kamiokande
- Dynamical Dark Matter: I. Theoretical Overview
- Toward (Finally!) Ruling Out Z and Higgs Mediated Dark Matter Models
- Electromagnetic Cascade in the Early Universe and its Application to the Big-Bang Nucleosynthesis
- Dynamical Dark Matter: II. An Explicit Model
- Soft-Wall Stabilization
- Cosmic Rays from Dark Matter Annihilation and Big-Bang Nucleosynthesis
- A New Direction in Dark-Matter Complementarity: Dark-Matter Decay as a Complementary Probe of Multi-Component Dark Sectors
- Distinguishing Dynamical Dark Matter at the LHC
- Overcoming Velocity Suppression in Dark-Matter Direct-Detection Experiments
- Holographic Unhiggs
- The Unhiggs
- Direct Detection of Dynamical Dark Matter
- Lines and Boxes: Unmasking Dynamical Dark Matter through Correlations in the MeV Gamma-Ray Spectrum
- Continuum Naturalness
- Strategies for Probing Non-Minimal Dark Sectors at Colliders: The Interplay Between Cuts and Kinematic Distributions
- Continuum-Mediated Self-Interacting Dark Matter
- Dynamical Dark Matter, MATHUSLA, and the Lifetime Frontier
- Sensitivity to neutrinos from the solar CNO cycle in Borexino
- Secluded Dark Matter Coupled to a Hidden CFT
- Non-Minimal Dark Sectors: Mediator-Induced Decay Chains and Multi-Jet Collider Signatures
- Continuum-Mediated Dark Matter-Baryon Scattering
- The Quantum Critical Higgs
- Constraints on Light Dark Matter from Big Bang Nucleosynthesis