My Master's thesis examined various
numerical calculations and approximations for calculating the flux of
solar neutrinos in three flavours. The main motivation was to examine
the possible dependence on theta_13, and it was shown that low energy
solar neutrinos would be the most sensitive to this parameter.
I also wrote a fairly complete C++ library to carry out the calculation
numerically and using the various approximations discussed in the
thesis. The code is available here, but you will have to contact me if
you want to run it, as there is no help manual, although it is quite
straightforward once one gets the jist of it.
The Thesis (pdf) (Password Protected for now...)
The Code (Password Protected)
A tarball with the source, Makefile and required data for the solar and
PREM models. Basically untar everything in a directory, modify the
makefile and call me when it doesn't work.
Some help for the Code
(Password Protected)
The usual ROOT generated html pages, quite helpful when the code is
actually installed.