4 research outputs found
The Cr neutrino source and Borexino: a desirable marriage
Exposure to a Cr neutrino source as that used in Gallex will provide
an excellent overall performance test of Borexino, which should collect about
1400 source induced events, with an initial rate of about 35 counts per day.
This will be particularly important if MSW-small-angle turns out to be the
solution of the solar neutrino problem. In addition, if an independent,
accurate calibration is available, one will have an interesting experiment on
neutrino properties: as an example, a neutrino magnetic moment of the order
could be detected/excluded at the 90\% C.L.Comment: 7 pages, RevTeX, plus 3 postscripts figures, tarred, compresse
Solar opacity, neutrino signals and helioseismology
In connection with the recent suggestion by Tsytovich et al. that opacity in
the solar core could be overestimated, we consider the following questions: i)
What would a 10\% opacity reduction imply for the solar neutrino puzzle? ii) Is
there any hope of solving the solar neutrino puzzle by changing opacity? iii)
Is a 10\% opacity reduction testable with helioseismological data?Comment: revtex file of 3 pages + 2 postscipt figures, in a uuencoded
compressed tarred file, send any offprint request to [email protected]
Where are the beryllium neutrinos?
We show that present experiments imply that neutrinos are nonstandard at the
87\% C.L., independently of solar or nuclear physics. Moreover, if neutrinos
are standard, the Be flux must be almost zero. Even if we arbitrarily
disregard one of the experiments, the neutrino flux must still be less than
half of the value predicted by standard solar models.Comment: 8 pages in RevTeX 3.0 plus 2 figures in uuencoded postscript files.
Full postscript version available via anonymous ftp from
risc0.ca.infn.it:/pub/private/lissia/infnfe-10-94.ps (192.84.132.4) Submitted
to Physics Letters
The MSW solution to the solar neutrino problem for non-standard solar models
The difficulties for non-standard solar models (NSSM) in resolving the solar
neutrino problem are discussed stressing the incompatibility of the
gallium--Kamiokande data, and of the gallium--chlorine data. We conclude that
NSSM's cannot explain simultaneously the results of any two of the solar
neutrino data (chlorine, Kamiokande and gallium). We address further the
question whether the MSW solution exists for NSSM's (e.g. models with B
neutrino flux much lower than the standard one and/or central temperature
very different from ). We demonstrate that the MSW solution
exists and is very stable relative to changes of (-factor for +
Be reaction) and . In particular, is almost constant
while depends on the exact values of (or
B-neutrino flux) and .Comment: 13 pages in RevTeX 3.0 plus 3 figures in uuencoded postscript files.
Full postscript version available via anonymous ftp from
risc0.ca.infn.it:/pub/private/lissia/lngs-94-104.ps (192.84.132.4) Submitted
to Physics Letters