This page contains simulated fluxes of solar atmopsheric neutrinos accompanying the work:
"Solar Atmospheric Neutrinos and the Sensitivity Floor for Solar Dark Matter Annihilation Searches"
C.A. Arguelles, G. de Wasseige, A. Fedynitch, B.J.P. Jones
https://arxiv.org/abs/1703.07798
We present a limited simulation release in two folders:
Pre-propagation
Solar atmospheric neutrino fluxes predicted at each impact parameter for a variety of primary cosmic ray models and for each neutrino flavor.
Post-propagation
Solar atmopsheric neutrino fluxes after propagation through the Sun and between Sun and Earth, aggregated over impact factors.
Both folders contain a README with format information, as well as summary plots and scripts with which they were generated, in jupyter notebook format.
The complete set of fluxes can be found in the .tar file:
Comlete archive
Any questions about these fluxes should be directed to the authors:
caad@mit.edu, gdewasse@vub.ac.be, anatoli.fedynitch@desy.de, ben.jones@uta.edu
Last update:
Tuesday June 27, 2018.
Figures show example fluxes for nu_mu flavor. Left: at production in the solar atmopshere for impact parameter b=0. Right: After propagation through the solar core and to the Earth.