Interplay of energy dependent astrophysical neutrino flavor ratios and new physics effects

Abstract

We discuss the importance of flavor ratio measurements in neutrino telescopes, such as bymeasuring the ratio between muon tracks to cascades, for the purpose of extracting new physics signals encountered by astrophysical neutrinos during propagation from the source to the detector. The detected flavor ratios not only carry the energy information of specific new physics scenarios which alter the transition probabilities in distinctive ways, but also the energy dependent flavor composition at the source. In the present work, we discuss the interplay of these two energy dependent effects and identify which new physics scenarios can be distinguished from the detected flavor ratios as a function of astrophysical parameters.We use a recently developed self-consistent neutrino production model as our toy model to generate energydependent source flavor ratios and discuss (invisible) neutrino decay and quantum decoherence as specific newphysics examples. Furthermore, we identify potentially interesting classes of sources on the Hillas plot for the purpose of new physics searches. We find that sourceswith substantial magnetic fields 103 Gauss≲B≲106 Gauss, such as Active Galactic Nuclei (AGN) cores,white dwarfs, or maybe gamma-ray bursts, have, in principle, the best discrimination power for the considered new physics scenarios, whereas AGN jets, which typically perform as pion beam sources, can only discriminate few sub cases in the new physics effects. The optimal parameter region somewhatdepends on the class of new physics effect considered.