Analytic treatment of neutrino oscillation and decay in matter

Abstract

We analyze invisible decay of neutrinos in the presence of oscillation and matter effects. The inclusion of decay can be accommodated by a non-Hermitian effective Hamiltonian, with the Hermitian component giving rise to oscillations, and the anti-Hermitian component leading to the invisible decay of neutrinos. We consider the possibility that the oscillation and decay matrix may not commute; in fact, in matter, they will invariably become non-commuting. This would lead to a mismatch between the effective mass eigenstates and the decay eigenstates. Employing a resummation of the Zassenhaus expansion, we develop a formalism for calculating the neutrino oscillation probabilities in the two-flavor scenario. This technique can easily be extended to three flavors.

Summary of Session III: Multimessenger astrophysics

“…Finally, S. Goswami suggested an alternative approach for analytic treatment of neutrino decay and oscillation in matter [53,54]. It is emphasized that in the presence of decay the Hamiltonian is non-hermitian, hence decay eigenstates and mass eigenstates are not simultaneously diagonalisable by Unitary transformations [55].…”

“…It is emphasized that in the presence of decay the Hamiltonian is non-hermitian, hence decay eigenstates and mass eigenstates are not simultaneously diagonalisable by Unitary transformations [55]. Subsequently, a formalism is developed for the two-flavor [53] and three-flavor [54] neutrino propagation through matter of uniform density with invisible neutrino decay. Neutrino oscillation probabilities are derived as perturbative expansions for different decay scenarios.…”