Astronomy and Astrophysics – Astrophysics
Scientific paper
2007-01-24
Phys.Rev.Lett.98:171301,2007
Astronomy and Astrophysics
Astrophysics
5 pages, 1 eps figure; clarifications and references added, improved discussion, conclusions unchanged. Matches version publis
Scientific paper
10.1103/PhysRevLett.98.171301
Future cosmological data may be sensitive to the effects of a finite sum of neutrino masses even as small as ~0.06 eV, the lower limit guaranteed by neutrino oscillation experiments. We show that a cosmological detection of neutrino mass at that level would improve by many orders of magnitude the existing limits on neutrino lifetime, and as a consequence on neutrino secret interactions with (quasi-)massless particles as in majoron models. On the other hand, neutrino decay may provide a way-out to explain a discrepancy <~ 0.1 eV between cosmic neutrino bounds and Lab data.
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