SPL-Fréjus Collection partkirkmcd/mumu/target/...+ ATM ν:see Th. Schwetz Machines R. Garoby & M....
Transcript of SPL-Fréjus Collection partkirkmcd/mumu/target/...+ ATM ν:see Th. Schwetz Machines R. Garoby & M....
ISS-CERN 22-24/9/05
SPL-Fréjus
Collection part
J.E Campagne
Thanks to S. Gilardoni, A. Cazes
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New optimization questioned @ MMW04*
Particle production
Horn design optimisation
Decay tunnel parameter optimisation
Flux computation at Fréjus
θ13 and δCP sensitivity.LAL – 04-102 submitted to EPJC
p
π,Κ
π,Κ ν
*: Multi MegaWatt Workshop at CERN 26-28 May 04
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Particle productionProton beam :
1. Pencil like2. Ek=2.2GeV, 3.5GeV,…, 8GeV
Target : 1. 30cm long cylinder, ∅15mm in Liq. Hg2. FLUKA 2002.4
Normalized to 4MW beam power:1.10 1023 pot/yr @ 2.2GeV0.69 1023 pot/yr @ 3.5GeV0.30 1023 pot/yr @ 8.0GeV
Pion+ production
0,25
0,26
0,27
0,28
0,29
0,30
0,31
0,32
0,00 2,00 4,00 6,00 8,00 10,00
Beam Energy
yiel
d (1
e23)
Max. π yield ≠
Max. Phys. sensitivity
5GeV
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SuperBeam vs νFact Optics
px/pz
x20 mrad
2 m
Super Beam
Spot size @ 130kmDecay tunnel size
px/pz
x
½ rad
30cm
νFact
Decay channel solenoidsAperture and B strength
Thanks S. Gilardoni
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Pion production p (2.2GeV)π+
Hg
νFact SB
at the exit of the target
Horn optimisation by S. Gilardoni
This new optimisation
2 105 pot
Rule of thumb: Eπ/3~ Eν (MeV) > 2.L(km)
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Kaon production?
at 2.2GeV : 0.26 π+/s 0.8 10-3 K+/s
see BENE meeting 11/09/03
at 3.5GeV : 0.29 π+/s 2.8 10-3 K+/s
at 4.5GeV : 0.32 π+/s 5.2 10-3 K+/s
Ep(GeV) Ep(GeV)
π+
π-
K+
K-
K0Not physical dip !!!Not Used…
3.52.2
For
500
000
pot
Rate x 1016
New Fluka will be tested
HARP ???
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Horn style of collection
Bφ(r) ∝ Icur/rIcur ~ (300 ÷ 600) kA
rmin limited by Target size π+
IN
OUT
“Ideal”
shape
20cm
4cm1m 2m
40cm
The wrong sign pionsare eliminated locally
JEC NuFact-Note-138
Fixed momentum focalisation~800 MeV/c
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Comparison Solenoid vs Horn
S. Gilardoni thesis
capt
ure
Dec
ay s
olen
oid
~3m
20T →1.2
5T30cm
0,3m ~1m
The collection yield is identical ~1.4 10-3 π/pot
νFact
Solenoid
Horn x 2MARS
Cut : 1.5 cm.rad
In µRLA
Dec
ay s
olen
oid
~0.5m~1m ~1m
E
Horn ≈ Solenoid
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Horn design parameter for Super Beam
140 cm 220 cm
80 cm
140cmtotal length
220cmtotal length40cmouter radius
REFLECTOR
20.5cmouter radius40cmneck length3.4cminner radius
HORNHORN
Eν~300MeVEπ~800MeV
Conductor thickness : 3mmhorn : 300kAmps
reflector : 600kAmpsChallenging!!!
Using Geant 3.2.1NuFact-Note 138
Drawing from the horn built at CERNOptimized for Super Beam
+ or - focusing
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Decay Tunnel Parameters
• Lengths: 1. Modify beam purity2. Tested: 10m …→ 40m …→ 60m3. Optimum @ 40m
• Radius: 1. modify acceptance2. 1m …→ 2m3. No optimum found: larger is better (we just keep
“reasonable” radius)
This results have been checked on sensitivity to θ13 and δCP
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Fluxes comparison @ 130km
<Eν> ~ 275 MeV, 4.5 1011/m2/yrOld νFact optimum
<Eν> ~ 300 MeV, 1.2 1012/m2/yr3.5GeV SPL optimum
~95 νµCC/kT/yr*
*: Lipari x-sect. (see later)Reflector: 50% of the Flux
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π+π−
~1/2 µ− & 1/2 K0e3
µ+
Flux @ 130km: compositionhttp://opera.web.lal.in2p3.fr/horn/Simu/index.htm
3.5GeV Kinetic p beam~800MeVπ focusing40m decay tunnel length2m decay tunnel radius
+ Focusing
− Focusingπ−π+
~1/3 µ+ & 1/3 K0e3 & 1/3 K+
e3
µ−
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The X-sections
βB is an ideal tool to measure these cross-sections and a 2% systematic error on both signal and background are used.
---: Lipari et al.PRL74(95)4384
on H20
νµ SPL
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Some physics performances440kT water Č, 4MW SPL, GLoBES
2% syst. on signal & bkg
(χ2(2dof)=4.6 or 11.83)*: 5 bins [0.08,1.08] GeV
Sin22θ13(90%CL) = 610-3 (0.7°)
5yrs (+)δCP=0
preliminary
90%CL
New Opt.Old Opt.
True values: (∆m23, sin22θ13)
sin22θ12=0.82, θ23=π/4, ∆m221=8.1 10-5eV2
5% external precision on θ12 and ∆m221 and
use SPL disappearance channel and spectrum analysis*
sizeable improvement
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Beam Energy comparison
hep-ex/0411062 with an early version of analysis
10-310-4 10-310-4
5y+ 2y+8y-
2.2GeV3.5GeV4.5GeV8GeV
-100
-50
0
50
-150
3.5GeV is an optimum
Eν~260MeV
δCP = 010-3 sin22θ13
10-3
∆m
2 23 (e
V2)
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CNGS vs SB/νFact HORN
SB/νFact CERN proto
CNGS Horn
Pbeam = 4MW / 2÷3GeV, Target inside300÷600kA/50Hz/100µs200 M pulses/6 weeks
Neck: PJ = 7kW, PB = 63kW (8mm eq. Alu)1022 fast neutron/cm2/6 months
Pbeam = 0,4MW / 400GeV, Target outside150kA/2pulses 10µs-6s20 M 2pulses/5 years
IC: PJ = 13kW, PB = 5kW (2mm Alu)
Every parameter is critical
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CERN prototype (2001-2002)
Neck
Inner Cond. Double skin
S. GilardoniS.Rangod, J.M Mauguin…
1 m
42 c
m
Water cooling
(NUFACT-NOTE : 4, 28, 42, 80, 81, 126, 129)
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Energy deposition in the horn (induced by protons)
34.0 kW47kW
A. Cazes + JECNufact-Note-134
4MW, 2GeV proton beam
+7kW fromJoule effect
13.6kW
Solution ?: reduce Al thickness (3mm Al) + strength rings
63kW(8mm Al)
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Horn cooling (CERN schema)
Round shape thread inside the waist
The gain in surface exchange is somewhatlost by the thickness increase and then the heat load increase…
Double skin 20kW/surface exchange275kW/m2
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R&D: water cooling is still ok?
Aluminum alloy cylinder80 mm ext. diameter300 mm length
Heat load ~ 30 kW
Water curtainor other water jets
configuration
At LAL
Sprinkler
Contact me if you plan to do it
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Power Supply (basic)
500 (180 Horn) µΩR1500µFC
0.6 (0.4 Horn)µHL
100µsτo
300kA (14,5 rms)IM
7kVUo
50Hz thyristors
50Hz: 20 x « µ life time »
The main trouble
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Power Supply
• CERN had successfully tested the Horn at 100kA/(0.5)Hz• mid-June 03: a schedule of conditions have been written by LAL
(13p) for a (300kA/100µs/50Hz) power supply.• 1st industrial price feed back:
1. Main power supply (7kV/130A): HAZEMEYER co.: ~ 160k€2. Switches (300kA/100µs/50Hz): ABB co: ~ 3x2x50k€* = 300k€
But we think that a 300kA/1Hz may be a good next step to push the present CERN power supply prototype..
A solution exists for ~ 460k€ (700kCH)
*: factor 2 for # of switches, factor 3 for 1Hz -> 50Hz
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Al alloy property modifications
6082 (CNGS) or 6061 (MiniBOONE)
Précipitation (Mg2Si) par nThermique
Défauts par nRapide
Flux (n/cm2)
Rp ou Rm
1021 61022
Cavités
(n,p) et (n,α) reactions produce hydrogen and helium cavities
J.E.C NuFact-Note-130
Non irradiated Al can stand more than 108 pulses
And also MiniBOONE…
108 pulses
Max. stress ~ 14MPa to be confirmed
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Other problems…
• Integration of the Target• Compatibility with Hg• Radioactive water cooling treatment • Water Cooled Striplines• Fabrication cost issues if the life time of
a horn is < 1y• Fast Coupling (cooling & electric) remotely
controlled (see US/Japan example)
• Nuclear waste management...
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Summary
An optimized version of the Horn-like collection/focusing and SuperBeam energy is availablewith the present knowledge of the π/K production x-sections and the detector performances.The Horn R&D has been interrupted more or less in 2002 at CERN and not revived yet elsewhere.The Horn-like collection has been demonstrated in the past to be equivalent to a Solenoid-like collection for a NuFact. The SB-Horn and the NF-Horn are different simply because they have different purposes, but they share a lot of design parameters, so a SB-Horn is a prototype for a NF-Horn.
Thank you
ISS-CERN 22-24/9/05
END
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A possible schema
+ BetaBeam: see M. Mezzetto+ ATM ν: see Th. Schwetz
MachinesR. Garoby & M. Lindroos
TRE
CERN SPLLSM-Fréjus
Near detector
130km
Related talks
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SPL block diagram (CDR 1)Characteristics (Conceptual Design Report 1):
are “optimized” for a neutrino factoryassume the use of LEP cavities & klystrons up to the
highest energy
2.2GeV
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Gradients at 700 MHz
Last test performed in CryHoLab (July 04):5-cells 700 MHz ß=0.65 Nb cavity A5-01from CEA/Saclay and IPN-Orsay
from Stephane Chel, HIPPI04, Frankfurt, sep04
LEP cavities may have worked 350MHz & 3.6MV/m effective gradientNuFact Note 040
1E+08
1E+09
1E+10
1E+11
0 2 4 6 8 10 12 14 16 18 20Eacc ( MV/m )
Q0
Vertical Cryostat (Fast Cooling)
Horizontal Test in CryHoLab (B1)
quench
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Choice of the EnergyNeglecting Matter effect (Ok CERN-Frejus), for δCP = 0°
Maximum of probability is obtained for
2famillies formula
∆m221=810-5eV2, ∆m2
31=2.410-3eV2, L=130km
Eν = 250MeV
c23=s23=1/√2,tan2θ12=0.4
sin22θ13=10-2, Eν =320MeV sin22θ13=10-3, Eν =390MeV
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Decay Tunnel ParametersLengthLength
1. modify purity2. L=10m, 20m, 40m and
60m have been tested.
3. 10m→40mνµ , νµ + 50% to 70%νe , νe + 50% to 100%
4. 40m→60mνµ , νµ + 5%νe , νe + 20%
40m seems better40m seems better
RadiusRadius1. modify acceptance2. R=1m, 1.5m and 2m
have been Tested3. 1m →2m (L=40)
νµ , νµ +50%νe , νe +50% to 70%
Larger is better (2m)…Larger is better (2m)…
This results have been checked on sensitivity to θ13 and δCP