Title: Matter Effects on Neutrino Oscillations
1Matter Effects on Neutrino Oscillations
Nov. 20, 04 AS
2Outline
- Matter effects and Solar Neutrinos
- The world with ?13 and matter enhancement to ?13
- Very Long Baseline Neutrino Oscillation
Experiments and the Determination of ?13 and
?23work in progress with Y. Umeda
3The Neutrino Mixing Matrix
The world without ?13 and ? CHOOZ bound sin22?13lt
0.1
4Neutrino-electron coherent scattering
5Solar Neutrino Oscillations and Matter
Enhancement
Diagonalization ?12??12m
6Wolfenstein, 1978 Mikheyev and Smirnov, 1986
Varying electron density in the
Sun Adiabaticity
7Combine Solar Neutrino and KamLAND experiments
Y.-F. Wang in ICHEP04
8The World with ?13
new mixing!
new mixing!
The ?e ??? oscillation length
For an experiment with the terrestrial beam E??
a few GeV, one drops
9?? does not evolve, while ?e ?? induced by ?13
and Ae.
Diagonalization ?13??13m
10Barger et al., 99 Banuls, Barenboim, Bernabeu, 01
Earth mantle ?5 g/cm3, Eres?6.4 GeV Earth
core ?12 g/cm3, Eres?2.7 GeV
11Stacey, Physics of the Earth, 77
?m5 g/cm3 ?c12 g/cm3
Freund and Ohlsson 99
12Very Long Baseline Neutrino Oscillation
Experiments
In progress with Y. Umeda
Still treat ?0
The solution the equation in the constant-density
approximation
13Use actual Earth density profile for calculation
14How long is the very long baseline?
Banuls, Barenboim, Bernabeu, 01
Gandhi et al., hep-ph/0408361
?Optimized for P(????e) ?1-P(?????) also peaks at
E?? Eres
15?Simultaneous measurements of P(????e) and
P(?????) sensitive to ?13 and ?23. Are they
really Independent? ?P(????e) studied for L9300
km Fermilab to Kamioka.
F. DeJongh, hep-ex/0203005
Consider L9300 km case for P(????e)? P?e and
P(?????) ? P??
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17In progress with Y. Umeda
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23w.r.t resonant energy
lt 0.03
gt0.03
24Issues to be considered ?The effect of CPV phase
? (?10, Gandhi et al., hep-ph/0408361
) ?Convoluting with the ?? spectrum from the
accelerator
25. DeJongh, hep-ex/0203005
?? CC events before and after oscillations
Sharp cutoff to avoid background
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28From the mixing matrix, one derives
29Studying GeV neutrinos on Earth