6533b7d9fe1ef96bd126d5ba
RESEARCH PRODUCT
Weakly interacting dark matter particle of a minimal technicolor theory
Jussi VirkajärviKimmo TuominenKimmo Kainulainensubject
PhysicsNuclear and High Energy PhysicsParticle physicsHypercharge010308 nuclear & particles physicsmedia_common.quotation_subjectHigh Energy Physics::PhenomenologyDark matterAdjoint representation01 natural sciencesUniverseStandard ModelGauge group0103 physical sciencesNeutrino010306 general physicsLeptonmedia_commondescription
We consider the possibility that a massive fourth family neutrino, predicted by a recently proposed minimal technicolor theory, could be the source of the dark matter in the Universe. The model has two techniflavors in the adjoint representation of a SU(2) techicolor gauge group and its consistency requires the existence of a fourth family of leptons. By a suitable hypercharge assignment the techniquarks together with the new leptons look like a conventional fourth standard model family. We show that the new (Majorana) neutrino N can be the dark matter particle if m{sub N}{approx}100-500 GeV and the expansion rate of the Universe at early times is dominated by an energy component scaling as {rho}{sub {phi}}{approx}a{sup -6} (kination), with {rho}{sub {phi}}/{rho}{sub rad}{approx}10{sup -6} during the nucleosynthesis era.
year | journal | country | edition | language |
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2007-04-12 | Physical Review D |