4 research outputs found
Planck-Scale Physics and Neutrino Masses
We discuss gravitationally induced masses and mass splittings of Majorana,
Zeldovich-Konopinski-Mahmoud and Dirac neutrinos. Among other implications,
these effects can provide a solution of the solar neutrino puzzle. In
particular, we show how this may work in the 17 keV neutrino picture.Comment: 10 pages, IC/92/79, SISSA-83/92/EP, LMU-04/92 (the preprint number
has been corrected; no other changes
Planck scale effects in neutrino physics
We study the phenomenology and cosmology of the Majoron (flavon) models of
three active and one inert neutrino paying special attention to the possible
(almost) conserved generalization of the Zeldovich-Konopinski-Mahmoud lepton
charge. Using Planck scale physics effects which provide the breaking of the
lepton charge, we show how in this picture one can incorporate the solutions to
some of the central issues in neutrino physics such as the solar and
atmospheric neutrino puzzles, dark matter and a 17 keV neutrino. These
gravitational effects induce tiny Majorana mass terms for neutrinos and
considerable masses for flavons. The cosmological demand for the sufficiently
fast decay of flavons implies a lower limit on the electron neutrino mass in
the range of 0.1-1 eV.Comment: 24 pages, 1 figure (not included but available upon request), LaTex,
IC/92/196, SISSA-140/92/EP, LMU-09/9
Gallium Solar Neutrino Experiments: Absorption Cross sections, Neutrino spectra, and Predicted Event Rates
Neutrino absorption cross sections for 71Ga are calculated for all solar
neutrino sources with standard energy spectra, and for laboratory sources of
51Cr and 37Ar; the calculations include, where appropriate, the thermal energy
of fusing solar ions and use improved nuclear and atomic data. The ratio, R, of
measured (in GALLEX and SAGE) to calculated 51Cr capture rate is R = 0.95 +/-
0.07 (exp)} + ^{+0.04}_{-0.03} (theory). Cross sections are also calculated for
specific neutrino energies chosen so that a spline fit determines accurately
the event rates in a gallium detector even if new physics changes the energy
spectrum of solar neutrinos. Theoretical uncertainties are estimated for cross
sections at specific energies and for standard neutrino energy spectra.
Standard energy spectra are presented for pp and CNO neutrino sources in the
appendices. Neutrino fluxes predicted by standard solar models, corrected for
diffusion, have been in the range 120 SNU to 141 SNU since 1968.Comment: 57 pages, ReVTeX file. Accepted for publication in Phys. Rev. C.
Viewgraphs and numerical tables of neutrino spectra and cross sections at
http://www.sns.ias.edu/~jn