The merits (and de-merits)
- f the Silver Channel at the Neutrino Factory
Andrea Donini I.F.T.-U.A.M. Madrid with thanks to Enrique - - PowerPoint PPT Presentation
The merits (and de-merits) of the Silver Channel at the Neutrino Factory Andrea Donini I.F.T.-U.A.M. Madrid with thanks to Enrique Fernndez-Martnez, Patrick Huber, Jacobo Lpez-Pavn, Davide Meloni, Pasquale Migliozzi, Stefano Riglin
The Golden Channel: νe→νμ The degeneracy problem The Silver Channel: νe→ντ Limitations of the Silver Channel How to improve the Silver Channel The νμ→ντ Channel νe→ντ and νμ→ντ for other means:
unitarity of the PMNS matrix sterile neutrinos ...
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What we already know (at 2σ)
Solar sector Atm. sector
What we still don’t know
sin2θ13 < 0.031 δ Mass hierarchy θ23 octant
G.L. Fogli hep-ph/0608060
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−0.7 × 10−5eV2
−0.05
|∆m2
23|
= 2.6+0.4
−0.4 × 10−3eV2
sin2 θ23 = 0.45+0.16
−0.09
23)
The νe →νμ oscillation probability in matter 4
eµ = X± µ sin2 2θ13+Y ± µ sin 2θ13 cos
There is a curve of
Black square = input
If we add antineutrinos
Two other unknown
2 Intersections each
G.L.Fogli et al. hep-ph/9604415
There are 4 different sets
The νe →ντ oscillation probability in matter
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eτ = X± τ sin2 2θ13−Y ± τ sin 2θ13 cos
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9
10 8
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The main limitation is STATISTICS. 13
2000 4000 6000 8000 LMID km 101 102 103 104 sin22Θ13 sensitivity limit Golden only Golden Silver Golden Platinum All three channels
3Σ
GLoBES 2006
LECC LMID 2000 4000 6000 8000 LMID km 101 102 103 104 sin22Θ13 sensitivity limit 2000 4000 6000 8000 LMID km 101 102 103 104 True value of sin22Θ13 Mass hierarchy for ∆CP3Π2 3Σ
Golden only GoldenSilver GoldenPlatinum All three channels GLoBES 2006
LECC LMID 2000 4000 6000 8000 LMID km 101 102 103 104 True value of sin22Θ13 Mass hierarchy for ∆CP3Π2 3Σ
Difficult:
increase the mass?
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Difficult:
Increase the mass? Magnetize the detector to use more τ decay channels?
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Difficult:
Increase the mass? Magnetize the detector to use more τ decay channels?
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Limited impact at the Neutrino Factory for the
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1 2 3 4 5 6 7 8 9 10 Θ13 0.0021 0.0023 0.0025 0.0027 0.0029 m223 36 38 40 42 44 46 48 50 52 54 Θ23 0.0021 0.0023 0.0025 0.0027 0.0029 m223
Crucial beyond the three-family oscillation scenario
to test unitarity of the PMNS matrix
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19 Crucial beyond the three-family oscillation scenario
to test unitarity of the PMNS matrix
104 103 102 101 ΗeΤ 180 90 90 180 ∆eΤ 104 103 102 101 ΗΜΤ 180 90 90 180 ∆ΜΤ
Crucial beyond the three-family oscillation scenario
to test unitarity of the PMNS matrix to look for sterile neutrinos
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20 40 60 80
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solid lines = including matter effects dashed lines = no matter effects 20 40 60 80
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Different cross-sections can
Comparison of LIPARI (black)
We used the LIPARI cross-
The cross-sections will be