Data and Results from hep-ph/0506298
If using the data here provided,
please cite
M.Cirelli, N.Fornengo, T.Montaruli, I.Sokalski,
A.Strumia, F.Vissani, ``Spectra of neutrinos from dark matter
annihilations'', Nucl. Phys. B727:99-138, 2005, hep-ph/0506298v5.
This is
Release 4: A bug in the production of the fluxes of
anti-neutrinos after propagation from the Sun has been fixed. All other fluxes are unchanged. So in particular there are
no
changes for: all fluxes before production (neutrinos and
anti-neutrinos), all fluxes after propagation from the Earth (neutrinos
and anti-neutrinos),
neutrino fluxes after propagation from the Sun.
Fluxes of neutrinos before propagation (i.e. at production from DM
annihilations):
Fluxes of neutrinos after propagation (oscillations, absorptions,
regeneration):
Fluxes of neutrinos after propagation (oscillations, absorptions,
regeneration) given in
Mathematica
format:
This page is mirrored at:
http://www.to.infn.it/~fornengoDMnu.html
http://www.cern.ch/astrumia/DMnu.html
http://www.marcocirelli.net/DMnu.html
Further information, different (reasonable) data formats, copies of the
figures in the paper, files from the previous release for comparisons
and so on can be obtained upon request:
fornengo@to.infn.it,
marco.cirelli@cea.fr .
Last updated: 18 february 2010