Abstract
The conversion of electron neutrinos into either a tan or muon neutrino in a dense plasma, such as in the solar interior, is shown to be described by the Weber equation. We show that the problem is related to propagation through a potential barrier and is identical to classical mode conversion problems in inhomogeneous fluids and plasmas, (C) 1997 Elsevier Science B,V.
Original language | English |
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Pages (from-to) | 257-259 |
Number of pages | 3 |
Journal | Physics Letters A |
Volume | 232 |
Issue number | 3-4 |
DOIs | |
Publication status | Published - 28 Jul 1997 |
Keywords
- OSCILLATIONS
- MODE