Speaker
Dafne Guetta
(Ariel University)
Description
The recently discovered 100GeV- TeV emission from Novae hints towards a possible hadronic origin of this radiation component. To investigate such scenario, I developed a tailored Monte Carlo (MC) simulation that reproduces the kinematics of proton-proton interactions occurring in the nova wind. As a result, I find that sub-TeV observations of Novae can be reproduced by an hadronic scenario. I also estimate the neutrino flux from these sources, the constraints that come from the lack of observation of IceCube and the prediction for KM3 Net and ANTARES
Primary author
Dafne Guetta
(Ariel University)
