Dark Forces in the Sky: Signals from Z' and the Dark Higgs
arXiv:1605.09382 · doi:10.1088/1475-7516/2016/08/001
Abstract
We consider the indirect detection signals for a self-consistent hidden model containing a Majorana dark matter candidate, , a dark gauge boson, , and a dark Higgs, . Compared with a model containing only a dark matter candidate and mediator, the addition of the scalar provides a mass generation mechanism for the dark sector particles and is required in order to avoid unitarity violation at high energies. We find that the inclusion of the two mediators opens up a new two-body s-wave annihilation channel, . This new process, which is missed in the usual single-mediator simplified model approach, can be the dominant annihilation channel. This provides rich phenomenology for indirect detection searches, allows indirect searches to explore regions of parameter space not accessible with other commonly considered s-wave annihilation processes, and enables both the and scalar couplings to be probed. We examine the phenomenology of the sector with a focus on this new process, and determine the limits on the model parameter space from Fermi data on dwarf spheriodal galaxies and other relevant experiments.
17 pages, 7 figures. v2: cross section corrected, qualitative conclusions unchanged; references added
References in corpus (20)
- An Introduction to PYTHIA 8.2
- Big-Bang Nucleosynthesis
- Secluded WIMP Dark Matter
- Secluded U(1) below the weak scale
- The WIMPless Miracle: Dark Matter Particles without Weak-scale Masses or Weak Interactions
- Simplified Models for a First Characterization of New Physics at the LHC
- Scalar Simplified Models for Dark Matter
- Hidden On-Shell Mediators for the Galactic Center Gamma-Ray Excess
- Fitting the Galactic Center Gamma-Ray Excess with Cascade Annihilations
- On the Validity of the Effective Field Theory for Dark Matter Searches at the LHC Part III: Analysis for the -channel
- Higgs portal vector dark matter for scale -ray excess from galactic center
- The windows for kinetically mixed Z'-mediated dark matter and the galactic center gamma ray excess
- Nonabelian dark matter: models and constraints
- Dark Matter Signals from Cascade Annihilations
- A weighty interpretation of the Galactic Centre excess
- Hidden Sector Dark Matter Models for the Galactic Center Gamma-Ray Excess
- Multi-Step Cascade Annihilations of Dark Matter and the Galactic Center Excess
- Phenomenology of Dark Matter annihilation into a long-lived intermediate state
- Two-portal Dark Matter
- Lining up the Galactic Center Gamma-Ray Excess
Cited by in corpus (16)
- Residual Networks of Residual Networks: Multilevel Residual Networks
- Exoplanets as Sub-GeV Dark Matter Detectors
- Self-consistent Dark Matter Simplified Models with an s-channel scalar mediator
- Dark Higgs Bosons at Colliders
- Two Higgs Doublet Dark Matter Portal
- Exotic Higgs Decays
- Evaporation Barrier for Dark Matter in Celestial Bodies
- Hunting WIMPs with LISA: Correlating dark matter and gravitational wave signals
- Right-handed Neutrino Dark Matter in a U(1) Extension of the Standard Model
- Age Group and Gender Estimation in the Wild with Deep RoR Architecture
- Sub-GeV dark matter and nano-Hertz gravitational waves from a classically conformal dark sector
- Exploring dark sector parameters in light of neutron star temperatures
- Indirect Detection of Secluded Supersymmetric Dark Matter
- Bouncing Dark Matter
- SN1987A constraints to BSM models with extra neutral bosons near the trapping regime: model as an illustrative example
- A Radiative Model of Quark Masses with Binary Tetrahedral Symmetry