Origin of matter in the universe

dc.creatorGu, Pei-Hong
dc.date2007-06-13
dc.date2007-08-31
dc.date.accessioned2026-07-07T10:56:12Z
dc.date.available2026-07-07T10:56:12Z
dc.descriptionWe extend the standard model with two iso-singlet color triplet scalars, one singlet real scalar and one singlet fermion. The new fields are odd under an unbroken Z_2 discrete symmetry while the standard model particles are even. The decays of the singlet real scalar into three standard model quarks (antiquarks) with three singlet antifermions (fermions), which explicitly violate the baryon number, will become effective after the electroweak phase transition and then produce the observed baryon asymmetry in the universe through the loop diagram involving the exchange of the W gauge boson. The singlet fermion can serve as the candidate for cold dark matter. In our model, all new particles with masses below the TeV scale can be detected by the forthcoming collider experiments or the next generation experiments for neutron-antineutron oscillations.
dc.description6 pages, 7 figures. Comment on proton decay improved. Accepted by PLB
dc.identifierhttps://arxiv.org/abs/0706.1946
dc.identifierhttp://arxiv.org/abs/0706.1946
dc.identifierPhys.Lett.B657:103-106,2007
dc.identifierdoi:10.1016/j.physletb.2007.08.095
dc.identifier.urihttp://salesiana.dossiersoluciones.com/handle/123456789/186333
dc.subjectHigh Energy Physics - Phenomenology
dc.titleOrigin of matter in the universe
dc.typetext

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