overview of the kopio detector 2005 rhic & ags users ’ meeting brookhaven national laboratory...
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Overview of the KOPIO Detector
2005 RHIC & AGS Users’ MeetingBrookhaven National Laboratory
June 20, 2005David E. Jaffe
June 20, 2005 David E. Jaffe 2005 RHIC & AGS Users’ meeting 2
• Poor kinematic signature: 3-body decay
• Neutral initial and final states
• Only outgoing 0 is observable
• SM prediction Br(KL0) = 3x10-11
• Main background is KL0 0 with
Br=9.3x10-4 which implies a need for suppression of >7x107
Observing KL0
“Experimentally, the problems are perhaps best represented by the statement that nobody has shown that a measurement of this decay is absolutely impossible” F.J.Gilman, “CP violation in Rare K Decays”, Blois CP Violations 1989:481-496
June 20, 2005 David E. Jaffe 2005 RHIC & AGS Users’ meeting 3
Experimental Search for KL0
E391a using same technique and
is the first dedicated experiment
to search for KL0
KTeV Results using ‘pencil’ beam
PL B447(1999)240.
June 20, 2005 David E. Jaffe 2005 RHIC & AGS Users’ meeting 4
KOPIO technique: work in KL CMS
Measure everything possible
Microbunched KL beam
Measure directions in PR
Measure energy in CAL
Reconstruct 0 from Measure KL velocity from TOF
Photon Veto (PV)
Charged Particle Veto (CPV)
Kinematic veto
June 20, 2005 David E. Jaffe 2005 RHIC & AGS Users’ meeting 5
June 20, 2005 David E. Jaffe 2005 RHIC & AGS Users’ meeting 6
KOPIO technique: work in KL CMS
Measure everything possible
Microbunched KL beam
Measure directions in PR
Measure energy in CAL
Reconstruct 0 from Measure KL velocity from TOF
Photon Veto (PV)
Charged Particle Veto (CPV)
Kinematic veto
June 20, 2005 David E. Jaffe 2005 RHIC & AGS Users’ meeting 7
Microbunch Width
93 MHz cavity at 22 kV gave= 240 ps
Microbunch time, in ns
93 MHz cavity at 22 kV gave217 ps
Microbunch time, in ns
Data Simulation
SimulationData
Simulations predict = 180ps utilizing
new 25 and 100MHz cavities
June 20, 2005 David E. Jaffe 2005 RHIC & AGS Users’ meeting 8
Interbunch ExtinctionInterbunch Extinction
4.5 MHz cavity at 130 kV gave= 8 (+/- 6) x 10-6
Microbunch time, in ns Microbunch time, in ns
Data Simulation
4.5 MHz cavity at 130 kV gave= 1.7 (+/- 0.9) x 10-3.
Data Simulation
Interbunch events
Interbunch events
Extinction performance at high AGS intensities last
remaining issue to be verified
June 20, 2005 David E. Jaffe 2005 RHIC & AGS Users’ meeting 9
KOPIO technique: work in KL CMS
Measure everything possible
Microbunched KL beam
Measure directions in PR
Measure energy in CAL
Reconstruct 0 from Measure KL velocity from TOF
Photon Veto (PV)
Charged Particle Veto (CPV)
Kinematic veto
June 20, 2005 David E. Jaffe 2005 RHIC & AGS Users’ meeting 10
ExtrudedScintillator &WLS fibers
Cathode strip drift chambers
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e+
e-
Preradiator – convert & measure properties
64 Layers (4% X0/layer, 2.7 X0) 256 Chambers 288 Scintillator Plates (1200 m2) 150,000 Channels Readout
4m
June 20, 2005 David E. Jaffe 2005 RHIC & AGS Users’ meeting 11
KOPIO technique: work in KL CMS
Measure everything possible
Microbunched KL beam
Measure directions in PR
Measure energy in CAL
Reconstruct 0 from Measure KL velocity from TOF
Photon Veto (PV)
Charged Particle Veto (CPV)
Kinematic veto
June 20, 2005 David E. Jaffe 2005 RHIC & AGS Users’ meeting 12
Shashlyk Photon Calorimeter
APD
Shashlyk modules prototyped and tested in beams. Requiredspecs have all been met
June 20, 2005 David E. Jaffe 2005 RHIC & AGS Users’ meeting 13
KOPIO technique: work in KL CMS
Measure everything possible
Microbunched KL beam
Measure directions in PR
Measure energy in CAL
Reconstruct 0 from Measure KL velocity from TOF
Photon Veto (PV)
Charged Particle Veto (CPV)
Kinematic veto
June 20, 2005 David E. Jaffe 2005 RHIC & AGS Users’ meeting 14
Every detector is a photon veto!
Fine-sampling lead/scintillator-basedshower counters of shashlyk & bar geometry. All thick enough so punch-through not an issue.
KOPIO PV estimates and simulations based on
BNL E949 measurements supplemented by FLUKA
calculations
1 MeV Visible Energy Threshold
June 20, 2005 David E. Jaffe 2005 RHIC & AGS Users’ meeting 15
Catcher: Hadron Blind Beam Veto
beam
420 modules ofPb-Aerogel counter
June 20, 2005 David E. Jaffe 2005 RHIC & AGS Users’ meeting 16
KOPIO technique: work in KL CMS
Measure everything possible
Microbunched KL beam
Measure directions in PR
Measure energy in CAL
Reconstruct 0 from Measure KL velocity from TOF
Photon Veto (PV)
Charged Particle Veto (CPV)
Kinematic veto
June 20, 2005 David E. Jaffe 2005 RHIC & AGS Users’ meeting 17
Plastic Scintillator – backed up by vetoes!
185 290
10-5
10-4
10-3
Data
MC
Charged Particle Veto Performance
10-6
June 20, 2005 David E. Jaffe 2005 RHIC & AGS Users’ meeting 18
KOPIO technique: work in KL CMS
Measure everything possible
Microbunched KL beam
Measure directions in PR
Measure energy in CAL
Reconstruct 0 from Measure KL velocity from TOF
Photon Veto (PV)
Charged Particle Veto (CPV)
Kinematic veto
June 20, 2005 David E. Jaffe 2005 RHIC & AGS Users’ meeting 19
Kinematic Separation of Signal &Backgrounds
Signal BackgroundsPion kinetic energy squared (T*2) vs Ln(Missing Energy)
June 20, 2005 David E. Jaffe 2005 RHIC & AGS Users’ meeting 20
Discovering/Constraining New Physics
1st yr2nd yr
3rd yr
KOPIO Proposal
June 20, 2005 David E. Jaffe 2005 RHIC & AGS Users’ meeting 21
• Only approved experiment sensitive enough reach the SM level
• Uses a robust innovative technique to suppress background
• Only experiment that measures the area of the unitarity triangle
• Excellent discovery potential for non-SM physics
KOPIO is Unique
June 20, 2005 David E. Jaffe 2005 RHIC & AGS Users’ meeting 22
Extras
June 20, 2005 David E. Jaffe 2005 RHIC & AGS Users’ meeting 23
BNL scientists and KOPIO
BNL physics dept scientists currently participating on KOPIOD.Beavis: Integration SSM,Vacuum,CDRJ.Frank : CPV STL, CPV constructionD.Jaffe : Sim. SSM, Parameters STL, CDR, 2 students/2004,1
student/2005S.Kettell: Trig/DAQ/Offline/FEE STL, TriggerL.Littenberg: Spokesman,CDR,1student/2004,1student/2005G.Redlinger: DAQ SSM,CDR,PV ineff’y,1student/2004C.Scarlett:CDR,1student/2004,2students/2005M.Sivertz:AGS SSM,CAL/PV STL, CDR, CPVconstruction,
microbunch testbeam,2students/2004,1student/2005STL=Scrub Team Leader for Apr05 NSF reviewCDR=author of chapter(s) in KOPIO Conceptual Design Report for
Apr05 NSF review
June 20, 2005 David E. Jaffe 2005 RHIC & AGS Users’ meeting 24
The Challenge of KOPIO
• B(KL0) ~ 310-11, need huge flux of K’s– rates inevitably rather high
• Kinematic signature weak (2 particles undetectable)• Backgrounds with 0 up to 1010 times larger• Veto inefficiency on extra particles must be 10-4
• Huge flux of neutrons in beam– can make 0 off residual gas – require high vacuum
– halo must be very small
– hermeticity requires photon veto in this beam
• Need convincing measurement of background
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June 20, 2005 David E. Jaffe 2005 RHIC & AGS Users’ meeting 25
KOPIO Technique
• High intensity micro-bunched beam from the AGS• Measure everything! (energy, position, angle, time)• Eliminate extra charged particles or photons
– KOPIO: 0 inefficiency < 10-8
• Suppress backgrounds– Predict backgrounds from data:dual cuts– Use “blind” analysis techniques– Test predictions “outside the box”
• Weight candidate events with S/N likelihood function
June 20, 2005 David E. Jaffe 2005 RHIC & AGS Users’ meeting 26
• Proton Beam
• 100TP/spill (upgraded from present 70TP)• ~5s spill, 2.3s interspill• Microbunching
• Extract debunched beam resonantly between empty buckets• 25MHz frequency• 200ps bunch width• 10-3 interbunch extinction
• Kaon Beam• 42.5o take-off angle• Soft momentum spectrum
• 0.5-1.5 GeV/c
• 3108 KL/spill• 8% decay
• 10 GHz neutrons
Need AGS to provide
40 ns between microbunches=200 ps
June 20, 2005 David E. Jaffe 2005 RHIC & AGS Users’ meeting 27
ExtrudedScintillator &WLS fibers
Cathode strip drift chambers
.
.
.
.
.
.
.
.
.
.
.
.
.
.
.
.
e+
e-
Preradiator – convert & measure properties
64 Layers (4% X0/layer, 2.7 X0) 256 Chambers 288 Scintillator Plates (1200 m2) 150,000 Channels Readout
4m
June 20, 2005 David E. Jaffe 2005 RHIC & AGS Users’ meeting 28
Preradiator Angular resolution: 25 mr at 250 MeV/c
Simulations agree with measurements.
KOPIO Prototype Measurements – BNL LEGS Tagged Photon Beams
June 20, 2005 David E. Jaffe 2005 RHIC & AGS Users’ meeting 29
Shashlyk Photon Calorimeter
APD
Shashlyk modules prototyped and tested in beams. Requiredspecs have all been met
June 20, 2005 David E. Jaffe 2005 RHIC & AGS Users’ meeting 30
Beam test of Calorimeter modulesBeam test of Calorimeter modules
Simulation: Combined PR +CAL Energy Resolution
2.7%
( )E GeV
June 20, 2005 David E. Jaffe 2005 RHIC & AGS Users’ meeting 31
Charged Particle Veto in vacuum
June 20, 2005 David E. Jaffe 2005 RHIC & AGS Users’ meeting 32
Plastic Scintillator – backed up by vetoes!
185 290
10-5
10-4
10-3
Data
MC
Charged Particle Veto Performance
10-6
June 20, 2005 David E. Jaffe 2005 RHIC & AGS Users’ meeting 33
Every detector is a photon veto!
US Wall
Barrel veto
Preradiator
Prerad outer veto
Calorimeter
vetoes in D4 sweeping magnet
vetoes in DS vacuum pipe
Fine-sampling lead/scintillator-based shower counters of shashlyk & bar geometry. All thick enough so punch-through not an issue. All with sufficient efficiency
June 20, 2005 David E. Jaffe 2005 RHIC & AGS Users’ meeting 34
E949 Single Ineff’y Measurement
+
2
1
K2 Decay
June 20, 2005 David E. Jaffe 2005 RHIC & AGS Users’ meeting 35
KOPIO PV Estimates and Simulations based on improved BNL E949 Measurements supplemented by FLUKA calculations
1 MeV Visible Energy Threshold
Photon Veto Inefficiency
June 20, 2005 David E. Jaffe 2005 RHIC & AGS Users’ meeting 36
Catcher: Hadron Blind Beam Veto
Aerogel Counterbeam
420 modules ofPb-Aerogel counter
June 20, 2005 David E. Jaffe 2005 RHIC & AGS Users’ meeting 37
Catcher R&D results
Modules prototyped and tested in beams.
June 20, 2005 David E. Jaffe 2005 RHIC & AGS Users’ meeting 38
KL modes simulated for bkgnd studies
Largest back-grounds
June 20, 2005 David E. Jaffe 2005 RHIC & AGS Users’ meeting 39
Other Backgrounds
• K+ contamination of beam: <0.001 of signal rate
• KLK+e-, K-e+: ~ 0.001 of signal rate
• nN N: negligible production from residual gas in decay volume if pressure<10-6 Torr. Requirements on reconstructed ZV(KL) suppress rate from US wall to <0.01 of signal rate
• n: far smaller than neutron background
• Hyperons: <10-5 of signal rate
• Fake photons < 0.05 of signal rate assuming ~10-3 10-3 suppression from (vetoing) (/n discrimination)
• Two KL giving single candidate: negligible due to vetoes
• (KL X) (e ): ~0.01 of signal rate
• KS 10-4 of KL background rate
_
June 20, 2005 David E. Jaffe 2005 RHIC & AGS Users’ meeting 40
Kinematic Separation of Signal &Backgrounds
Signal Backgrounds
Pion kinetic energy squared (T*2) vs Ln(Missing Energy)
June 20, 2005 David E. Jaffe 2005 RHIC & AGS Users’ meeting 41
*
ew physics could be revealed K .
:
*
New flavor physics in the sector may be very different from that in the secto b r:
s-d
If B - physics is consistent with the SM
I
N
K would add crucial additional information;
the complexity of the flavor sector beyond the SM
:
is
f deviations from the SM are indicated
foreseen in many models.
Roles of K Measurements in Flavor Physics
Results from will be needed to interpret
non-SM physics discoveries at BABAR, BELLE,
CDF/D0, and the
K
LHC.
June 20, 2005 David E. Jaffe 2005 RHIC & AGS Users’ meeting 42
• KTeV (FNAL): B(KL0) < 5.910-7 (90% CL)• KEK E391a >10-9 ?? J-PARC LOI • KOPIO (BNL): single event sensitivity <10-12
– Discovery (5) for B(KL0)>510-11 or <1.8 10-11
– If nothing new, ~300 SM events• Rule out BRs outside of (10.17)BRSM @ 95%CL• Bound operators, B-system can’t access
[ , ] 9Limit based on via iso 1.4 10spin : Grossman NirK x
0 0Experiments Seeking LK 0 0 11LSM: B(K ) (3.0 0.6) 10x
_
_
June 20, 2005 David E. Jaffe 2005 RHIC & AGS Users’ meeting 43
KOPIO Parameters
bunch width (extinction) 200ps (10-3)• Beam halo 10-4
• Vacuum 10-7 Torr resolution @ 250MeV 25 mr
• E resolution 2.7%/ E(GeV)
• t resolution 90ps/ E(GeV)
veto inefficiency(outside beam) E949 or better veto efficiency(inside beam) >99% at 300 MeV• n efficiency (inside beam) <0.3% at 800 MeV• Charged particle inefficiency 210-5(+), 1.210-4(-)
June 20, 2005 David E. Jaffe 2005 RHIC & AGS Users’ meeting 44
Preradiator
64 Layers (4% X0/layer, 2.7 X0)256 Chambers288 Scintillator Plates (1200 m2)
150,000 Channels Readout
4m
June 20, 2005 David E. Jaffe 2005 RHIC & AGS Users’ meeting 45
Primary detection mode: Secondary mode:2 photons covert in preradiator 1 photon in preradiator, 1 in BV
Reconstruct 1st e+e- in “Preradiator”,
Point to K decay vertex in vacuum
June 20, 2005 David E. Jaffe 2005 RHIC & AGS Users’ meeting 46
Simulation: Combined PR+ CAL Energy Resolution
2.7%
( )E GeV
Shashlyk Beam Measurements
June 20, 2005 David E. Jaffe 2005 RHIC & AGS Users’ meeting 47
Barrel Veto/Calorimeter
• Cylindrical array of 840 modules with 2.5m ID
• Both signal detection and vetoing functions– 1 in prerad + 1 in BV/C
• Modified version of calorimeter shashlyk technology, pmt readout– Energy resolution calculated
to be almost as good as calorimeter
– Time resolution should be comparable
• B V/C lined with thin, high-efficiency, charged particle veto scintillators
US end of barrel sealed by wall of plate shower-counter vetoes
June 20, 2005 David E. Jaffe 2005 RHIC & AGS Users’ meeting 48
D4 & downstream vetoes
• Charged & vetoes in D4 sweeping magnet– Field sweeps vertically
• DS vetoes detect ’s emerging from the beam
• Lead/scintillator plate sandwich counters
• Hermeticity completed by catcher veto at the back
June 20, 2005 David E. Jaffe 2005 RHIC & AGS Users’ meeting 49
Primary Backgrounds
K * PV2
K * C2 * PV
K * C2
K * PV4
Rejections0 0 0 3L
0 2L
0 0L
0 0 0 0L
10
10
0.93
0.36
0.1255
10Background suppression factor needed: 10
Mode Branching Ratio
K
K
K
K
0 0
Primary Backgrounds
Measurement
x
xe
LK
0.2105
Others
Worst backgrounds are from KL decay
June 20, 2005 David E. Jaffe 2005 RHIC & AGS Users’ meeting 50
Simulation Tools
• GEANT3– FLUKA, GCALOR, GHEISHA hadronic packages
• GEANT4
• FLUKA
• MCNPX
• MARS
• KOPTICs – custom optics simulator
• FastMC– uses input from detailed simulators + input from experiments
• Critical parameters directly measured – Either in prototype tests or experiments
June 20, 2005 David E. Jaffe 2005 RHIC & AGS Users’ meeting 51
Alternative Display of Results
June 20, 2005 David E. Jaffe 2005 RHIC & AGS Users’ meeting 52
KOPIO Operations Plan
• 2010 Test Run – partial detector
• 2011 Engineering Run
“Discovery phase”: Sensitivity goal:~10-10
• 2012-16 Data Acquisition
June 20, 2005 David E. Jaffe 2005 RHIC & AGS Users’ meeting 53
Branching Ratio Measurement Precision
• Precision at B(KL0) = 310-11 Using probability likelihood method employing all observed events (approximately 300) 10%
• (Statistical) Precision on Im t: 5%