NEUTRINO ENERGY EIGENSTATES IN MATTER WITH VARYING DENSITY

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We consider the energy eigenstates of neutrino in matter with varying density. From this consideration we calculate the transition probability of P(v(e) --> v(e)) as a function of ratio of neutrino energy to neutrino mass difference squared E/Delta(o) in salar neutrino We show that our results are consistent with those results obtained by considering the effective mass eigenstates and level crossing.
Publisher
WORLD SCIENTIFIC PUBL CO PTE LTD
Issue Date
1995-05
Language
English
Article Type
Article
Keywords

3-NEUTRINO OSCILLATIONS; SOLAR NEUTRINOS; SPECTROSCOPY; SEARCH; FLUX

Citation

MODERN PHYSICS LETTERS A, v.10, no.13-14, pp.1035 - 1040

ISSN
0217-7323
DOI
10.1142/S0217732395001149
URI
http://hdl.handle.net/10203/67834
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