Sterile neutrinos, dark matter, and the pulsar velocities in models with a Higgs singlet

dc.creatorKusenko, Alexander
dc.date2006-09-08
dc.date2006-12-06
dc.date.accessioned2026-07-07T07:35:56Z
dc.date.available2026-07-07T07:35:56Z
dc.descriptionWe identify the range of parameters for which the sterile neutrinos can simultaneously explain the cosmological dark matter and the observed velocities of pulsars. To satisfy all cosmological bounds, the relic sterile neutrinos must be produced sufficiently cold. This is possible in a class of models with a gauge-singlet Higgs boson coupled to the neutrinos. Sterile dark matter can be detected by the x-ray telescopes. The presence of the singlet in the Higgs sector can be tested at the Large Hadron Collider.
dc.description4 pages, one figure
dc.identifierhttps://arxiv.org/abs/hep-ph/0609081
dc.identifierhttp://arxiv.org/abs/hep-ph/0609081
dc.identifierPhys.Rev.Lett. 97 (2006) 241301
dc.identifierdoi:10.1103/PhysRevLett.97.241301
dc.identifier.urihttp://salesiana.dossiersoluciones.com/handle/123456789/120261
dc.subjectHigh Energy Physics - Phenomenology
dc.subjectAstrophysics
dc.titleSterile neutrinos, dark matter, and the pulsar velocities in models with a Higgs singlet
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