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Precise analytical description of the Earth matter effect on oscillations of low energy neutrinos
Phys. Rev. D 71, 033006 – Published 23 February, 2005
DOI: https://doi.org/10.1103/PhysRevD.71.033006
Abstract
We present a formalism for the matter effects in the Earth on low energy neutrino fluxes which is both accurate and has all the advantages of a full analytic treatment. The oscillation probabilities are calculated up to the second order term in , where is the neutrino potential at position . We show the absence of large undamped phases which makes the expansion in well behaved. An improved expansion is presented in terms of the variation of around a suitable mean value which allows one to treat energies up to those relevant for supernova neutrinos. We discuss also the case of three-neutrino mixing.
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This result may be obtained via ordinary perturbation theory with the Hamiltonian , where is the diagonalized Hamiltonian (MSW solution) at point (). We stress that only that separation of the Hamiltonian into a nonperturbative () and a perturbative () part leads to results where terms proportional to the full distance traveled by neutrinos in matter are absent; this is, in fact, guaranteed by the existence of the MSW solution.
It is important to recall that enters both through and through the adiabatic phase .
Even more general would be an expansion around a suitable potential for which there is a closed analytic form.
When , then and .