Speaker
Nora Valtonen-Mattila
Description
Large-scale neutrino telescopes like IceCube monitor for supernovae using low energy neutrinos O(10 MeV), with a detection horizon out to the Magellanic Clouds. However, some models predict the emission of high-energy neutrinos O(>TeV) in core-collapse supernovae through the interaction of the ejecta with the circumstellar material or through choked jets. In this talk, I will explore the detection horizon of high-energy neutrinos emitted from core-collapse supernovae for the IceCube telescope, demonstrating that the reach for these objects can be pushed past the LMC and out to the neighboring galaxies in the Mpc range.
Author
Nora Valtonen-Mattila
