skip to main content
OSTI.GOV title logo U.S. Department of Energy
Office of Scientific and Technical Information

Title: Minimal semi-annihilating Z{sub N} scalar dark matter

Journal Article · · Journal of Cosmology and Astroparticle Physics
 [1]; ;  [2];  [3]
  1. LAPTH, Université de Savoie, CNRS, B.P.110, Annecy-le-Vieux Cedex, F-74941 France (France)
  2. National Institute of Chemical Physics and Biophysics, Rävala 10, Tallinn (Estonia)
  3. Skobeltsyn Institute of Nuclear Physics, Moscow State University, Moscow, 119991 (Russian Federation)

We study the dark matter from an inert doublet and a complex scalar singlet stabilized by Z{sub N} symmetries. This field content is the minimal one that allows dimensionless semi-annihilation couplings for N > 2. We consider explicitly the Z{sub 3} and Z{sub 4} cases and take into account constraints from perturbativity, unitarity, vacuum stability, necessity for the electroweak Z{sub N} preserving vacuum to be the global minimum, electroweak precision tests, upper limits from direct detection and properties of the Higgs boson. Co-annihilation and semi-annihilation of dark sector particles as well as dark matter conversion significantly modify the cosmic abundance and direct detection phenomenology.

OSTI ID:
22373538
Journal Information:
Journal of Cosmology and Astroparticle Physics, Vol. 2014, Issue 06; Other Information: Country of input: International Atomic Energy Agency (IAEA); ISSN 1475-7516
Country of Publication:
United States
Language:
English

Similar Records

Minimal semi-annihilating ℤ{sub N} scalar dark matter
Journal Article · Tue Jun 10 00:00:00 EDT 2014 · Journal of Cosmology and Astroparticle Physics · OSTI ID:22373538

Impact of semi-annihilations on dark matter phenomenology. An example of Z{sub N} symmetric scalar dark matter
Journal Article · Sun Apr 01 00:00:00 EDT 2012 · Journal of Cosmology and Astroparticle Physics · OSTI ID:22373538

ℤ{sub 3} scalar singlet dark matter
Journal Article · Tue Jan 01 00:00:00 EST 2013 · Journal of Cosmology and Astroparticle Physics · OSTI ID:22373538