An approximate solution for solar and supernova neutrino oscillation in matter

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dc.creatorLuo, Rui
dc.date2005-06-03
dc.date.accessioned2026-07-07T03:55:00Z
dc.date.available2026-07-07T03:55:00Z
dc.descriptionBy using Laplace transformation we developed an approximate solution to describe neutrino oscillation probabilities in arbitrary density matter. We show that this approximation solution is valid when matter potential V satisfy $V< Δm^2/2E$ and $\int VL<1$, where $L$ is the length of the neutrino oscillation . Thus, the formula is useful for propagation of the solar or supernova neutrinos with terrestrial matter effect.
dc.description15 pages, 3 figures
dc.identifierhttps://arxiv.org/abs/hep-ph/0506020
dc.identifierhttp://arxiv.org/abs/hep-ph/0506020
dc.identifier.urihttp://salesiana.dossiersoluciones.com/handle/123456789/44412
dc.subjectHigh Energy Physics - Phenomenology
dc.titleAn approximate solution for solar and supernova neutrino oscillation in matter
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