Sterile neutrino oscillation Sterile neutrino oscillation
at a neutrino factoryy
Ken-ichi Fuki Ken ichi Fuki
(Tokyo Metropolitan University )
Andrea Donini (IFT Madrid (UAM/CSIC)) Work in collaboration with
Andrea Donini (IFT, Madrid (UAM/CSIC)),
Davide Meloni (Rome III U. & INFN, Rome3 ),
Jacobo Lopez-Pavon (IFT, Madrid (UAM/CSIC)),
Osamu Yasuda (TMU)
1 1 Four flavor neutrino with LSND 1. Four flavor neutrino
1.1. Four flavor neutrino with LSND
(2+2) scheme
Maltoni et al, hep-ph/0405172(2+2) scheme
m32 m42
Excluded by solar ν
m 2
Excluded by solar ν and atm ν (4.9σ)
(3+1) scheme
m12 m2
m42 Strongly disfavored by SBL disappearance
m322
pp data (3.1σ)
m12 m22
1.2.1. Four flavor neutrino without LSND
Large θ
34is allowed θ
14and θ
24are small.
In contrast, g
34Donini-Maltoni-Meloni-Migliozzi-Terranova arXiv:0704.0388v2
,
14 16 18 20
30 35 40
8 10 12 14
θ 14 20
25
θ 34
2 4 6 8
5 10 15
0 2 4 6 8 10 12 14 16 18 20
θ13
0 2
0 2 4 6 8 10 12 14 16 18 20
θ24
0 5
1.2.2. Sensitivity limit at the CNGS/OPERA
Large g θ
3434is still allowed
Nominal intensity of 4.5 x 1019 pot/yr
14 θ23 = 45°, δ3 = 0°
1 2 3× 5
10 35
40
θ23 = 45°, δ3 = 0°
p y
8 10 12
4 × 1× 2××× 1
25 30
4
× 1
99%CL 99%CL
4 6 θ 14 8
10 15
θ 34 20 1
× 2
× 3
× 10× 5
0 2 4 6 8 10 12 14
0 2 4
0 2 4 6 8 10 12 14
0 5 10
0 2 4 6 8 10 12 14
θ13 0 2 4 6 θ248 10 12 14
Donini-Maltoni-Meloni-Migliozzi-Terranova arXiv:0704.0388v2
2 1 1st order expansion of probabilities in matter
2. (3+1)scheme at Neutrino Factory
2.1. 1st order expansion of probabilities in matter
ν e decouples !!
2.2. Set up
P ( ν μ →ν μ )
P ( ν μ →ν τ )
P ( ν μ →ν μ )
Set up:
relevant
I t 2 x 1020 muon decay / yr x 4 yr / baseline
L=3000km, 7500km
Input:
Δm241 > 0.1eV2
Hybrid-emulsion / Magnetized iron calorimeter of 50 kton
“HYBRID MIND”
A maximal muon energy = 50 GeV No CP phases
“HYBRID-MIND”
No background / No systematic errors Ref. Cervera @ GOLDEN’07 for HYBRID-MIND;
100 % efficiency for both εμ and ετ
~90% ~25%
De Lellis @ GOLDEN’07 for MAGNETIZED ECC
In reality 90% 25%
VERY PRELIMINAR ANALYSIS
In reality
2.3. Sensitivity in θ 13 , θ 14 ,θ 24 and θ 34
Very low sensitivity to θ13 and θ14 High sensitivity in θ24 and θ34
1) Highest sensitivity in θ34 from the 7500km
2). Highest sensitivity in θ24 from the 3000km baseline
1). Highest sensitivity in θ34 from the 7500km baseline
baseline
10
8
6
θ 14 3000km+7500km
90%CL
4
2
90%CL
θ
θ θ 0
0
10 8
6 4
2
0 θ13
ν e decouples !!
However, similar results marginalizing on θ13 and θ14θ13=θ14=0
2.4. Contribution of P(ν
μ→ν
μ) and P(ν
μ→ν
τ)
at 3000km at 3000km
Sensitive to both θ24 and θ34
3-flavor
4-flavor Θ24=10°
Θ34=25°
Pμτ
90%CL
No sensitivity to θ34, only to θ24
4-flavor 3-flavor
Θ24=10°
Pμμ
Θ34=25°
2.5. Contribution of P(ν
μ→ν
μ) and P(ν
μ→ν
τ)
at 7500km at 7500km
Sensitivity to both θ24y and θ34
Θ34=25°
Θ24=10°
τ
90%CL 3-flavor
4 flavor
Pμτ
4-flavor
Sensitivity to both θ24 and θ34
3-flavor 4-flavor
Θ24=10° Θ34=25°
Pμμ
Θ34=25
3. Summary
• Golden and Silver channels are not optimal to study 3+1Golden and Silver channels are not optimal to study 3 1 sterile neutrinos.
νμ→ νμ and νμ→ ντ are the relevant channels.
• We have performed a preliminary analysis at a two-baseline (L=3000km+7500km) 50GeV nufact with ideal HYBRID-MIND detectors (no background and 100% efficiency)
detectors (no background and 100% efficiency).
θ34 sensitivity down to 〜 4°and θ24 sensitivity down to 〜 1°at 90%CL.
1 at 90%CL.
Highest sensitivity in θ34 from the 7500km baseline and Highest sensitivity in θ24 from the 3000km baseline.
Hi h t iti it i θ f th d h l t
Highest sensitivity in θ24 from the νμ→ νμ and νμ→ ντchannels at 3000km.
Highest sensitivity in θ34 from the νμ→ νμ and νμ→ ντchannels at 7500km.
Th h l h hi h iti it i θ d θ t b th 3000k
The channel νμ→ ντ has a high sensitivity in θ34 and θ24 at both 3000km and 7500km, even though the event number is not large .
The νμμ→ νμμ channel alone gives g θ2424
< 1
°and θ3434< 5
°at 90%CL.It is very important to have a reasonable efficiency for
τ
to improve on θ24 , θ34 combination.