Abstract
Neutrinos with standard weak interactions are possible hot dark matter candidates, but they cannot provide an explanation for a cold dark matter scenario, because of constraints from relic abundance. It is shown here, however, that a stable ντ with a mass in the range 1–35 MeV and a magnetic moment of 10−6 Bohr magnetons is a possible candidate for a cold dark matter particle. This hypothesis can be experimentally tested in the near future.

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