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Large Extra Dimensions and Hot Dark Matter

2001
A neutrino mass-mixing scheme which explains qualitatively all present evidence for neutrino mass (the solar and atmospheric neutrino deficits, LSND, and significant hot dark matter) also successfully avoids the “alpha effect”, allowing r-process nucleosynthesis in the neutrino-heated ejecta of supernovae. The properties of neutrinos required to ensure
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Hot dark matter in the universe [PDF]

open access: possibleRussian Physics Journal, 2012
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Evidence for some hot dark matter?

Nature, 1992
Qaisar Shafi, Robert K. Schaefer
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STATUS OF HOT DARK MATTER

The Identification of Dark Matter, 2003
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