Analytic approximations for three neutrino oscillation parameters and probabilities in matter
- 19 July 2001
- journal article
- research article
- Published by American Physical Society (APS) in Physical Review D
- Vol. 64 (5) , 053003
- https://doi.org/10.1103/physrevd.64.053003
Abstract
The corrections to neutrino mixing parameters in the presence of matter of constant density are calculated systematically as series expansions in terms of the mass hierarchy The parameter mapping obtained is then used to find simple, but nevertheless accurate formulas for oscillation probabilities in matter including effects. Expressions with one to one correspondence to the vacuum case are derived, which are valid for neutrino energies above the solar resonance energy. Two applications are given to show that these results are a useful and powerful tool for analytical studies of neutrino beams passing through the Earth mantle or core: First, the “disentanglement problem” of matter and effects in asymmetry is discussed and second, estimations of the statistical sensitivity to the terms of the oscillation probabilities in neutrino factory experiments are presented.
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This publication has 30 references indexed in Scilit:
- ErratumPhysics Letters B, 2000
- Three flavor neutrino oscillations in matterJournal of Mathematical Physics, 2000
- Neutrino oscillations with three flavors in matter: Applications to neutrinos traversing the EarthPhysics Letters B, 2000
- The mixing angles in matter for three generations of neutrinos and the MSW mechanismThe European Physical Journal C, 1988
- Analytic conditions for three-neutrino resonant oscillations in matterPhysical Review D, 1988
- ErrataPhysics Letters B, 1987
- Adiabatic resonant oscillations of solar neutrinos in three generationsPhysical Review D, 1987
- Resonant amplification of three-neutrino oscillations in matterPhysics Letters B, 1987
- Solar-Neutrino Problem and Three-Neutrino OscillationsPhysical Review Letters, 1986
- Matter effects on three-neutrino oscillationsPhysical Review D, 1980