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VOLUME 78 (2003) | ISSUE 11 |
PAGE 1203
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Dark matter from SU(4) model
G. E. Volovik
Low Temperature Laboratory, Helsinki University of Technology, FIN-02015 HUT, Finland L. D. Landau Institute for Theoretical Physics RAS, 117334 Moscow, Russia
PACS: 12.10.-g, 12.60.Rc, 95.35.+d
Abstract
The left-right symmetric Pati-Salam model of the
unification of quarks and leptons is based on SU(4) and SU(2)× SU(2)
symmetry groups. These groups are naturally extended to include the
classification
of families of quarks and leptons. We assume that the family group
(the group which
unites the families) is also the SU(4) group. The properties of
the fourth-generation of fermions are the same as that of the ordinary-matter
fermions in first three generations except for the family charge of the
SU(4)F group:
F=(1/3,1/3,1/3,-1), where F=1/3 for fermions of
ordinary matter and F=-1 for the fourth-generation fermions. The
difference in
F does not allow the mixing between ordinary and fourth-generation fermions.
Because of the conservation of the
F charge, the creation of baryons and leptons in the process of electroweak
baryogenesis must be accompanied by the creation of fermions of the 4-th
generation. As a result the
excess nB of baryons over antibaryons leads to the excess
of neutrinos over antineutrinos in the 4-th generation with
n4ν= nB.
This massive neutrino may form the non-baryonic dark matter. In
principle the mass density of the 4-th neutrino
n4ν mN in the Universe can give the main contribution to the dark
matter, since the lower bound on the neutrino mass mN from the
data on decay of
the
Z-bosons is
mN>mZ/2. The straightforward prediction of this model leads
to the amount of cold dark matter relative to baryons, which is an order of
magnitude bigger than allowed by observations. This inconsistency may
be avoided
by non-conservation of the
F-charge.
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