Astronomy and Astrophysics – Astrophysics
Scientific paper
1998-11-04
Astronomy and Astrophysics
Astrophysics
8 pages, 1 Figure, LaTeX, epsfig
Scientific paper
The paper "Big Bang Nucleosynthesis and Active-Sterile Neutrino Mixing: Evidence for Maximal $\nu_\mu \leftrightarrow \nu_\tau$ Mixing in Super Kamiokande?" by X. Shi and G. M. Fuller (astro-ph/9810075) discusses the cosmological implications of the $\nu_\mu \to \nu_s$ solution to the atmospheric neutrino anomaly. It incorrectly concludes that a lower bound on the $\nu_\tau$ mass of 15 eV is needed in order for the $\nu_\mu \to \nu_s$ oscillations to be consistent with a Big Bang Nucleosynthesis upper bound on the effective number of flavours of 3.3. Since such a large $\nu_\tau$ mass is disfavoured from large scale structure formation considerations, the strong, but incorrect, conclusion is made that cosmology favours the $\nu_\mu \to \nu_\tau$ solution to the atmospheric neutrino problem. We explain the nature of the error. We conclude that cosmology is, at present, consistent with both the $\nu_\mu \to \nu_s$ and $\nu_\mu \to \nu_\tau$ possibilities.
Foot Robert
Volkas Raymond R.
No associations
LandOfFree
Comment on "Big Bang Nucleosynthesis and Active-Sterile Neutrino Mixing: Evidence for Maximal $ν_μ\leftrightarrow ν_τ$ Mixing in Super Kamiokande?" does not yet have a rating. At this time, there are no reviews or comments for this scientific paper.
If you have personal experience with Comment on "Big Bang Nucleosynthesis and Active-Sterile Neutrino Mixing: Evidence for Maximal $ν_μ\leftrightarrow ν_τ$ Mixing in Super Kamiokande?", we encourage you to share that experience with our LandOfFree.com community. Your opinion is very important and Comment on "Big Bang Nucleosynthesis and Active-Sterile Neutrino Mixing: Evidence for Maximal $ν_μ\leftrightarrow ν_τ$ Mixing in Super Kamiokande?" will most certainly appreciate the feedback.
Profile ID: LFWR-SCP-O-610498