Published January 2019 | Version v1
Journal article

Global analyses of Higgs portal singlet dark matter models using GAMBIT

  • 1. Australian Research Council Centre of Excellence for Particle Physics at the Tera-scale, Melbourne (Australia)
  • 2. Monash University, School of Physics and Astronomy, Melbourne, VIC (Australia)
  • 3. Stockholm University, Department of Physics, Stockholm (Sweden)
  • 4. AlbaNova University Centre, Oskar Klein Centre for Cosmoparticle Physics, Stockholm (Sweden)
  • 5. University of Adelaide, Department of Physics, Adelaide, SA (Australia)
  • 6. Imperial College London, Blackett Laboratory, Department of Physics, London (United Kingdom)
  • 7. McGill University, Department of Physics, Montreal, QC (Canada)
  • 8. Nanjing Normal University, Department of Physics and Institute of Theoretical Physics, Nanjing, Jiangsu (China)
  • 9. University of Oslo, Department of Physics, Oslo (Norway)
  • 10. RWTH Aachen University, Institute for Theoretical Particle Physics and Cosmology (TTK), Aachen (Germany)
  • 11. University of California, Physics and Astronomy Department, Los Angeles, CA (United States)
  • 12. Queen's University, Arthur B. McDonald Canadian Astroparticle Physics Research Institute, Department of Physics, Engineering Physics and Astronomy, Kingston, ON (Canada)
  • 13. DESY, Hamburg (Germany)

Description

We present global analyses of effective Higgs portal dark matter models in the frequentist and Bayesian statistical frameworks. Complementing earlier studies of the scalar Higgs portal, we use GAMBIT to determine the preferred mass and coupling ranges for models with vector, Majorana and Dirac fermion dark matter. We also assess the relative plausibility of all four models using Bayesian model comparison. Our analysis includes up-to-date likelihood functions for the dark matter relic density, invisible Higgs decays, and direct and indirect searches for weakly-interacting dark matter including the latest XENON1T data. We also account for important uncertainties arising from the local density and velocity distribution of dark matter, nuclear matrix elements relevant to direct detection, and Standard Model masses and couplings. In all Higgs portal models, we find parameter regions that can explain all of dark matter and give a good fit to all data. The case of vector dark matter requires the most tuning and is therefore slightly disfavoured from a Bayesian point of view. In the case of fermionic dark matter, we find a strong preference for including a CP-violating phase that allows suppression of constraints from direct detection experiments, with odds in favour of CP violation of the order of 100:1. Finally, we present DDCalc 2.0.0, a tool for calculating direct detection observables and likelihoods for arbitrary non-relativistic effective operators. (orig.)

Availability note (English)

Available from: http://dx.doi.org/10.1140/epjc/s10052-018-6513-6

Additional details

Publishing Information

Journal Title
European Physical Journal. C, Particles and Fields (Online)
Journal Volume
79
Journal Issue
1
Journal Page Range
p. 1-28
ISSN
1434-6052

Optional Information

Collaborations
The GAMBIT Collaboration