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XXIst International Conference on Neutrino Physics and Astrophysics
NEUTRINO 2004
A. Bueno University of Granada
The ICARUS ProjectThe ICARUS Project
A. Bueno (Granada University), ICARUS Collab. Neutrino 2004
The ICARUS CollaborationThe ICARUS CollaborationResearch project jointly approved by INFN and Research project jointly approved by INFN and CERN CERN
CERN/SPSC 2002CERN/SPSC 2002--027 (SPSC027 (SPSC--PP--323) LNGS323) LNGS--EXP 13/89 EXP 13/89
–– CNGS Physics Program: ICARUS is an official CERN CNGS Physics Program: ICARUS is an official CERN experiment known as CNGS2 (April 2003)experiment known as CNGS2 (April 2003)
ICARUS COLLABORATION25 INSTITUTIONS, 150 PHYSICISTS
CIEMATGranada
UCLA
ETHZ
INR
IHEP
Katowice KrakowWarsaw, Wroclaw
L’Aquila, LNGS, Milano, Napoli, Padova, Pavia,
Pisa, LNF
Liquid Argon Detector : Why?Liquid Argon Detector : Why?Easy to obtain with very high purity by specialized Easy to obtain with very high purity by specialized industriesindustries–– Concentration on atmosphere ~ 0.9%Concentration on atmosphere ~ 0.9%–– Cheap: 1 liter cost below 1 Cheap: 1 liter cost below 1 €€
Homogeneous medium simultaneously acting as target Homogeneous medium simultaneously acting as target and detectorand detectorInteresting physical properties for a tracking device: Interesting physical properties for a tracking device: –– Boiling point = 87.3 K at 1 bar; not flammableBoiling point = 87.3 K at 1 bar; not flammable–– Density = 1.4 g/cmDensity = 1.4 g/cm33
–– Radiation length = 14 cm; interaction length = 80 cmRadiation length = 14 cm; interaction length = 80 cm–– Electron mobility = 500 cmElectron mobility = 500 cm22/Vs/Vs–– dE/dxdE/dx = 2.1 MeV/cm= 2.1 MeV/cm
Propagation of charged particles inducePropagation of charged particles induce……–– Ionization Ionization
Minimum ionizing track: 88000 electron-ion pairs per cmAfter recombination @ 500 V/cm: 55000 pairs/cm
–– Scintillation Scintillation UV Spectrum UV Spectrum λλ=128 nm=128 nm
–– ČČerenkoverenkov light (given that light (given that ββ > 1/n)> 1/n)
A. Bueno (Granada University), ICARUS Collab. Neutrino 2004
A. Bueno (Granada University), ICARUS Collab. Neutrino 2004
After many years of R&D at lab scaleAfter many years of R&D at lab scale……
The road for construction of The road for construction of very massivevery massiveLArLAr TPC detectors is now open!TPC detectors is now open!
ElectronicElectronic BubbleBubble ChamberChamber
cathode
Anode: 3 wire planes (at ±60o and 0o)
EE
µµArgon(87K)
EE
ee−−
33--dimensional imagesdimensional images
LAr acts as target and detector Real EventsReal Real EventsEvents
µµ→→ee
EM EM ShowerShower
HadronicHadronic InteractionInteraction
Energymeasured in each point:
bubble size ≈3 x 3 x 0.2 mm3
ee−−
ee−−
ee−−
ee−−
ee−−
ee−−
ee−−
T600detector
A. Bueno (Granada University), ICARUS Collab. Neutrino 2004
T600 Detector: Cosmic Ray DataT600 Detector: Cosmic Ray DataMore than 27000 triggers collected during More than 27000 triggers collected during technical run on surface (summer 2001)technical run on surface (summer 2001)–– Detector performed according to expectationsDetector performed according to expectations–– Testing 3D reconstruction, particle ID capabilities, Testing 3D reconstruction, particle ID capabilities, ……Publications so farPublications so far……
Design, construction and tests of the ICARUS T600 Design, construction and tests of the ICARUS T600 detector, detector, accepted for publication by NIM A on 31/12/03accepted for publication by NIM A on 31/12/03..Measurement of the muon decay spectrum with the ICARUS Measurement of the muon decay spectrum with the ICARUS T600 liquid Argon TPC, T600 liquid Argon TPC, EurEur. Phys. Journal C33 (2004) 233. Phys. Journal C33 (2004) 233--241.241.Study of electron recombination in liquid Argon with the Study of electron recombination in liquid Argon with the ICARUS TPC, ICARUS TPC, NuclNucl. Inst. . Inst. MethMeth. A523 (2004) 275. A523 (2004) 275--283283..Analysis of Liquid Argon Purity in the ICARUS T600 TPCAnalysis of Liquid Argon Purity in the ICARUS T600 TPC, , Nucl. Inst. Meth. A516 (2004) 68Nucl. Inst. Meth. A516 (2004) 68--7979. . Observation of long ionizing tracks with the ICARUS T600 Observation of long ionizing tracks with the ICARUS T600 first halffirst half--module,module, Nucl. Inst. Meth. A508 (2003) 287Nucl. Inst. Meth. A508 (2003) 287--294294. .
A. Bueno (Granada University), ICARUS Collab. Neutrino 2004
Liquid Argon PurityLiquid Argon Purity
Long drift distances demand ultra Long drift distances demand ultra pure Argonpure Argon– Impurities: 0.1 ppb Oxygen-
equivalentTwo independent and complementary methods to measure the LAr purity:– Purity Monitors : on-line
information on a fixed position of the chamber (punctualmeasurement).
– Muon tracks: off-line analysis measuring the collected charge attenuation from crossing muon tracks (average measurement).
For future modules, the present technology would allow to expand drift distances up to 3m
0
250
500
750
1000
1250
1500
1750
2000
2250
2500
0 10 20 30 40 50 60 70 80
from long tracks
from purity monitors
LA
r re
-cir
cula
tion
OF
F
Elapsed Time (Days)
Lif
etim
e (µ
s)
ICARUS T600
Vdrift= 1.56 mm / µs @ 0.5 kV/cm
drift ≈ 2.3 m
Liquid Argon TPCis a mature
detection technique
A. Bueno (Granada University), ICARUS Collab. Neutrino 2004
Michel Electron SpectrumMichel Electron Spectrum
Study of stopping muon Study of stopping muon sample sample –– 3000 events analyzed and 3000 events analyzed and
fully reconstructed in 3Dfully reconstructed in 3Dρρ parameter parameter
measurementmeasurement
Standard Model Standard Model ρρ = 0.75 = 0.75
Energy resolution for Energy resolution for electrons below ~50 MeVelectrons below ~50 MeV
)(08.0)(06.072.0 sysstat ±±=ρ
%2%11)(⊕=
EEEσ
A. Bueno (Granada University), ICARUS Collab. Neutrino 2004
Momentum measurement: Multiple ScatteringMomentum measurement: Multiple ScatteringEssential to measure kinematics Essential to measure kinematics properties of nonproperties of non--contained eventscontained events–– Interest focused on atmospheric eventsInterest focused on atmospheric events
Full simulation of muon events for a broad Full simulation of muon events for a broad momentum range momentum range –– Include all detector effectsInclude all detector effects
Split track into segments. Measured Split track into segments. Measured angles have two contributions:angles have two contributions:
Momentum extracted from fit over a Momentum extracted from fit over a sample of different segment lengthssample of different segment lengthsResolutions Resolutions ≈≈2020--25%25%Future analysisFuture analysis……–– Resolution improvement with alternative Resolution improvement with alternative
methods (e.g. methods (e.g. KalmanKalman Filter)?Filter)?–– Validate conclusions with real data: large Validate conclusions with real data: large
sample of stopping muonssample of stopping muonsMC Momentum (GeV)
0 1 2 3 4 5 6MC Momentum (GeV)
0 1 2 3 4 5 6
∆
p/p
(%)
0
5
10
15
20
25
30
35
40
MC Momentum (GeV)0 1 2 3 4 5 6
MC Momentum (GeV)0 1 2 3 4 5 6
0
5
10
15
20
25
30
35
40MUON MOMENTUM RESOLUTION
Preliminary
( ) ( ) ( ) 2/30
220
2 ;/; −∝∝+= segRMSnoiseseg
RMSRMSnoise
RMSRMSmeas LpL ϑϑϑϑϑ
3 GeV muon
A. Bueno (Granada University), ICARUS Collab. Neutrino 2004
ParticleParticle IdentificationIdentification
210
215
2201170
1172
1174
1176
1178
1180
290
295
300
305
310
315
320
y(cm)z (cm)
x (c
m)
K+
µ+
e+
AB
BC
K+
µ+
Run 939 Event 46
A
BC
DK+
µ+
e+
CollectionK+[AB] → µ+[BC] → e+[CD]
wire
drift
tim
e
µ+
e+
K+
Induction I
K+ µ+e+
3D reconstruction
allows tocompute dE/dx
and range
A. Bueno (Granada University), ICARUS Collab. Neutrino 2004
Particle Identification: Neural NetworkParticle Identification: Neural Network
0
1000
2000
muons
81.20 %
K p
18.71 %
K p
0.09 %
K p
0 %
K p
02505007501000
pions
7.72 %
K p
91.78 %
K p
0.50 %
K p
0 %
K p
0
1000
2000
3000kaons
0.11 %
K p
0.62 %
K p
99.02 %
K p
0.25 %
K p
0
1000
2000
3000
protons
0 %
K p
0 %
K p
0.035 %
K p
99.965 %
K p
π
π
π
π
µ
µ
µ
µ
Muon Event Classification
1
10
102
103
0 0.2 0.4 0.6 0.8 1
Neural Net Out
Events
µ
π
k
p
Kaon Event Classification
1
10
102
103
0 0.2 0.4 0.6 0.8 1
Neural Net Out
Events
µ
π
k
p
Full generation and 3D Full generation and 3D reconstruction of muons, reconstruction of muons, pionspions, , protons and protons and kaonskaonsAnalysis based on neural Analysis based on neural network. Discrimination given by: network. Discrimination given by: –– Different stopping power for each Different stopping power for each
particle type particle type –– Difference on secondary particle Difference on secondary particle
production after decay/interaction production after decay/interaction of parent trackof parent track
–– Key issuesKey issues: : Accurate energy measurementAccurate energy measurementGood spatial resolution for Good spatial resolution for precise tracking reconstructionprecise tracking reconstruction
Very high identification Very high identification efficiencies efficiencies (>90%)(>90%) while low while low contamination levels contamination levels (few %)(few %) are are expected expected
Preliminary
A. Bueno (Granada University), ICARUS Collab. Neutrino 2004
T600 at LNGST600 at LNGS
Following LNGS DirectorFollowing LNGS Director’’s mandate, a s mandate, a working group of experts was set up to working group of experts was set up to review: review: –– ICARUS T600 (cryogenics, safety, installation, ICARUS T600 (cryogenics, safety, installation,
commissioning, operation)commissioning, operation)–– Risk Analysis: simulation of possible major Risk Analysis: simulation of possible major
failuresfailures–– Technical infrastructure and human resources Technical infrastructure and human resources
at LNGS to cope with ICARUS needsat LNGS to cope with ICARUS needs
A. Bueno (Granada University), ICARUS Collab. Neutrino 2004
Working Group Conclusions (Nov 2003)Working Group Conclusions (Nov 2003)
The ICARUS project is sound and innovativeThe ICARUS project is sound and innovativeRecommended improvements concerning the Recommended improvements concerning the cryogenic system will be implemented by our cryogenic system will be implemented by our collaboration collaboration –– Overall risk linked to LNGS activities is not increased Overall risk linked to LNGS activities is not increased
when T600 becomes operationalwhen T600 becomes operationalA significant amount of work should be carried out A significant amount of work should be carried out at LNGS to upgrade Hall B infrastructure and at LNGS to upgrade Hall B infrastructure and technical utilitiestechnical utilitiesT600 can be installed right now underground: T600 can be installed right now underground: allowed to enter hall B (summer 2004)allowed to enter hall B (summer 2004)
A. Bueno (Granada University), ICARUS Collab. Neutrino 2004
The T600 Installation RoadmapThe T600 Installation RoadmapMilestonesMilestones Estimated start/end datesEstimated start/end dates
LNGS DirectorLNGS Director’’s permission to place cryostat s permission to place cryostat undergroundunderground
End of May End of May
Works on Hall B pavement refurbishingWorks on Hall B pavement refurbishing 11--0606--04/1004/10--0909--0404
Control System & Liquid Nitrogen ReControl System & Liquid Nitrogen Re--LiquifierLiquifier Deadline: 30Deadline: 30--0909--0505
T600 Transportation to LNGS T600 Transportation to LNGS ““parking lotparking lot””positionposition (adjudicated contract)(adjudicated contract)
JulyJuly--04/04/
Control Room Building and SetControl Room Building and Set--up up (contract (contract adjudication 30/6/04)adjudication 30/6/04)
66--1010--04/1304/13--0909--0505
Supporting structure for N2 Utilities & Supporting structure for N2 Utilities & Purification System Purification System (adjudicated contract)(adjudicated contract)
1414--1010--04/3004/30--0808--0505
Thermal Insulation & Mechanics Installation Thermal Insulation & Mechanics Installation (adjudicated contract)(adjudicated contract)
3030--0808--04/1304/13--0707--0505
Piping Works Installation & Control System Piping Works Installation & Control System (INFN approval needed)(INFN approval needed)
1414--0707--05/1305/13--0909--0505
DRY TESTDRY TEST 1414--0909--05/405/4--1010--0505Upgrade human resources & ventilation, Upgrade human resources & ventilation, cooling, power distribution systems (LNGS cooling, power distribution systems (LNGS responsibility)responsibility) Deadline: 3Deadline: 3--1010--0505
LAr Supply, Filling & CommissioningLAr Supply, Filling & Commissioning October 2005October 2005
A. Bueno (Granada University), ICARUS Collab. Neutrino 2004
A Rich Physics ProgrammeA Rich Physics Programme
Atmospheric, Solar Atmospheric, Solar and Supernova and Supernova neutrinos neutrinos Long Baseline Long Baseline Neutrino Experiment:Neutrino Experiment:–– Explicit search for Explicit search for
ννµµ→→ννττ and and ννµµ→→ννee
BackgroundBackground--free free proton decay proton decay searches searches
uud
e+
dd
pπ0
I
C
A
R
U
S
Physics Prospects
A. Bueno (Granada University), ICARUS Collab. Neutrino 2004
CONCLUSIONSCONCLUSIONS
The Liquid Argon detection technique is now The Liquid Argon detection technique is now mature mature –– Matches the requirements imposed, to second Matches the requirements imposed, to second
generation detectors, by neutrino physics and proton generation detectors, by neutrino physics and proton decay searchesdecay searches
–– Ability to build very massive detectors Ability to build very massive detectors –– It has been demonstrated that It has been demonstrated that drift distancesdrift distances
amounting amounting up to several metersup to several meters are feasibleare feasibleThe T600 is being moved to LNGS The T600 is being moved to LNGS –– Physics run will start in Autumn, 2005Physics run will start in Autumn, 2005
The collaboration plans to clone the T600 The collaboration plans to clone the T600 module in order to reach a final mass of 3 module in order to reach a final mass of 3 KtonKton–– Address fundamental questions related to the Physics Address fundamental questions related to the Physics
Beyond the Standard ModelBeyond the Standard Model
A. Bueno (Granada University), ICARUS Collab. Neutrino 2004
ICARUS T3000 + Muon SpectrometerICARUS T3000 + Muon SpectrometerA SecondA Second--Generation Proton Decay Experiment and Neutrino Observatory at Generation Proton Decay Experiment and Neutrino Observatory at
Gran Sasso LaboratoryGran Sasso Laboratory
T600
T1200
T1200
Muon Spectrometer
LNGS-EXP 13/89 Add. 3/03
CERN/SPSC 2003-030
SPSC-P-323-Add. 1
Construction strategy:Construction strategy:““CloningCloning”” the successfully the successfully operated T600 module operated T600 module
A. Bueno (Granada University), ICARUS Collab. Neutrino 2004
CNGS: CNGS: ννµµ→→ννττ OscillationsOscillations
Main reaction Main reaction
–– Search based on Search based on kinematical criteriakinematical criteria–– Natural Natural ννττ contamination below 10contamination below 10--77 w.r.t. w.r.t. ννµµ
componentcomponent–– Several decay modes investigated (electron decay is Several decay modes investigated (electron decay is
the the ““goldengolden”” channel)channel)
–– 5 years of CNGS operation 5 years of CNGS operation (4.5 x 10(4.5 x 101919 p.o.t.)p.o.t.)–– T3000 detector T3000 detector (2.35 kton active LAr, 1.5 kton (2.35 kton active LAr, 1.5 kton
fiducial)fiducial)
Super-Kamiokande: 1.6 < ∆m2 < 3.0 at 90% C.L.
eννµνν
h−nh0ν
h−h+h−nh0ν
⎧
⎨ ⎪
⎩ ⎪ ⎪
18%18%50%14%
τ→ντ+Ar→τ+jet;
A. Bueno (Granada University), ICARUS Collab. Neutrino 2004
Main reactionMain reaction
Natural Natural ννee contamination contamination 1%1%Limited by CNGS Limited by CNGS statistics statistics
Three Neutrino Mixing10-1
10-110-210-3 1
10-3
10-2
10-4
sin 2Θ213
∆m
(
eV ) 2
2 23
ν νµ e
MINOS, 10 KT-YEARICARUS, 2.35 KT, 5 YEARS CNGS, + 4.6JHF+SK, 22.5 KT, 5 YEARS
min2χ
oMINOS
oCHOOZ
oCNGS
or
or
or
706.0)2(sin
1114.0)2(sin
604.0)2(sin
13132
13132
13,132
<<
<<
<<
θθ
θθ
θθ τ
CNGS: CNGS: ννµµ→→ννee OscillationsOscillations
For ∆m223 = 2.5 x 10-3 eV2For ∆m2
23 = 2.5 x 10-3 eV2
νe+Ar→e−+jet;