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Title: Global constraints on vector-like WIMP effective interactions

Journal Article · · Journal of Cosmology and Astroparticle Physics
 [1];  [2];  [3];  [3];  [4]
  1. Royal Inst. Tech., Stockholm (Sweden)
  2. Virginia Polytechnic Inst. and State Univ. (Virginia Tech), Blacksburg, VA (United States); Fermi National Accelerator Lab. (FNAL), Batavia, IL (United States)
  3. Univ. Autonoma de Madrid, Madrid (Spain); Instituto de Fisica Teorica UAM/CSIC, Madrid (Spain)
  4. Univ. Libre de Bruxelles, Brussels (Belgium)

In this work we combine information from relic abundance, direct detection, cosmic microwave background, positron fraction, gamma rays, and colliders to explore the existing constraints on couplings between Dark Matter and Standard Model constituents when no underlying model or correlation is assumed. For definiteness, we include independent vector-like effective interactions for each Standard Model fermion. Our results show that low Dark Matter masses below 20 GeV are disfavoured at the 3 σ  level with respect to higher masses, due to the tension between the relic abundance requirement and upper constraints on the Dark Matter couplings. Lastly, large couplings are typically only allowed in combinations which avoid effective couplings to the nuclei used in direct detection experiments.

Research Organization:
Fermi National Accelerator Laboratory (FNAL), Batavia, IL (United States)
Sponsoring Organization:
USDOE Office of Science (SC), High Energy Physics (HEP)
Grant/Contract Number:
AC02-07CH11359
OSTI ID:
1253004
Report Number(s):
FERMILAB-PUB-15-374-T; arXiv:1509.01587; 1391960
Journal Information:
Journal of Cosmology and Astroparticle Physics, Vol. 2016, Issue 04; ISSN 1475-7516
Publisher:
Institute of Physics (IOP)Copyright Statement
Country of Publication:
United States
Language:
English
Citation Metrics:
Cited by: 4 works
Citation information provided by
Web of Science

References (5)

Freeze-in production of FIMP dark matter journal March 2010
Search for new phenomena in events with three or more charged leptons in pp collisions at s = 8 $$ \sqrt{s}=8 $$ TeV with the ATLAS detector journal August 2015
Bayesian Implications of Current LHC Supersymmetry and Dark Matter Detection Searches for the Constrained MSSM text January 2012
Dark matter annihilations and decays after the AMS-02 positron measurements text January 2013
Detecting Dark Matter Annihilation with CMB Polarization : Signatures and Experimental Prospects text January 2005

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