Speaker
Mr
Mattias Blennow
(Royal Institute of Technology)
Description
We make an improved analysis on the flow of neutrinos originating from
WIMP annihilations inside the Sun and the Earth. We treat both
neutrino interaction and oscillation effects in a consistent
framework. Our numerical simulations are performed in an event based
setting, which is useful for both theoretical studies and for creating
neutrino telescope Monte Carlos. We find that the flow of muon-type
neutrinos is enhanced or suppressed depending on the dominant WIMP
annihilation channel.
Author
Mr
Mattias Blennow
(Royal Institute of Technology)
Co-authors
Dr
Joakim Edsjö
(Stockholm University)
Dr
Tommy Ohlsson
(Royal Institute of Technology)