[email protected] – binp, novosibirsk – march 1 st, 20081 tpc review david attié 10-th...
TRANSCRIPT
INSTR08 – BINP, Novosibirsk – March 1st, 2008 1
TPC ReviewTPC Review
David Attié
10-th INTERNATIONAL CONFERENCEON INSTRUMENTATION
FOR COLLIDING BEAM PHYSICS
Novosibirsk, March 1st, 2008
INSTR08 – BINP, Novosibirsk – March 1st, 2008 2
Outline
1. The Time Projection Chamber
• Description
• Characteristics
2. Examples of TPCs
• TPCs for High Energy Physics: Particle Physics and ions Physics
• TPCs for rare event detection: neutrinos, dark matter
3. TPC R&D
• Readout for TPC: Micro Pattern Gaseous Detector (GEM, Micromegas)
• Gas studies
• Spatial resolution measurements and techniques
4. The LC-TPC collaboration
• The Large Prototype
INSTR08 – BINP, Novosibirsk – March 1st, 2008 3
• TPCs have been operated often as the main tracker in a wide range of physics experiments:
– particle physics– heavy ion collision– underground experiments
• Need for Physics measurements:– momentum resolution– pattern recognition– low material budget to preserve good jet energy resolution
• Physics knowledge depend on the sensitivity and the performance of the instrument
Introduction
INSTR08 – BINP, Novosibirsk – March 1st, 2008 5
TPC description
Gas volumeReadout
z
x
y
gas system
field cage for the E field
magnet for the B field
amplification system at the anode
gating grid to suppress the ion feedback
laser calibration system
readout electronics
trigger
• Ingredients:
• The TPC is a gas-filled cylindrical chamber with one or two endplates
• Particle detector invented by D. R. Nygren in 1974
INSTR08 – BINP, Novosibirsk – March 1st, 2008 6
• Track point recorded in 3-D
(2-D channels in x-y) x (1-D channel in z = vdrift x tdrift)
• Low occupancy large track densities possible
• Particle identification by dE/dx
long ionization track, segmented in 100-200 measurements
STAR ion TPC BNL-RHIC
ALICE simulation
events
- LBL STAR TPC - at BNL RHIC ion collider
Characteristics of a TPC
INSTR08 – BINP, Novosibirsk – March 1st, 2008 8
Experiments with a TPC
TPC Reference PEP4 PEP-PROPOSAL-004, Dec 1976 TOPAZ Nucl. I nstr. and Meth. A252 (1986) 423 ALEPH Nucl. I nstr. and Meth. A294 (1990) 121 DELPHI Nucl. I nstr. and Meth. A323 (1992) 209-212 NA49 Nucl. I nstr. and Meth. A430 (1999) 210 STAR I EEE Trans. on Nucl. Sci. Vol. 44, No. 3 (1997)
TOPAZ (KEK)
ALEPH (CERN)
DELPHI (CERN)
PEP4 (SLAC) STAR (LBL)Some detectors in Particle and ions Physics using a TPC
INSTR08 – BINP, Novosibirsk – March 1st, 2008 9
Today: ALICE at LHC
• ALICE (A Large Ion Collider Experiment)
• search for a quark-gluon plasma
• in heavy ion collisions Pb-Pb
• at a centre of mass energy of 5.5 TeV per nucleon
INSTR08 – BINP, Novosibirsk – March 1st, 2008 10
First cosmic-rays events in ALICE TPC
• 3-dimensional view of a shower induced by cosmic rays
L. Musa et al.January 2008
INSTR08 – BINP, Novosibirsk – March 1st, 2008 11
Performance needed for the ILC-TPC
• LC-TPC should provide a good resolution on the momentum measurement
Precise and model-independent measurement of the Higgs-Mass in the Zμμ recoil
• Momentum: σ1/p ~ 5x10-5/GeV(1/10 x LEP)
- Z mass reconstruction from charged leptons
- Higgs-Strahlung:
• Need to support high density of tracks and/or final states with 6+ jets:
– high granularity
– good two tracks separation
– track identification
e+,μ+e–,μ–
INSTR08 – BINP, Novosibirsk – March 1st, 2008 12
ILC-TPC simulations
Simulation GEANT4 of LC-TPC, A. Vogel
• TPC for the International Linear Collider, e+e- collisions at 500 GeV
• Includes beam background
INSTR08 – BINP, Novosibirsk – March 1st, 2008 13
Future TPC for rare events detection
• Rare events topics:– neutrinos physics (double-beta decay, T2K long baseline
experiment)– Dark Matter search, WIMPs, axions
• TPC medium can also be used as the target
• Main TPC characteristics for this physics:– a large volume and/or a dense medium: pressurized gas or liquid– a “quiet” TPC (for example, no needs for gating gate)– generally underground experiments with low activity materials
• Examples :– ICARUS: Imaging Cosmic And Rare Underground Signals– GLACIER: Giant Liquid Argon Charge Imaging ExpeRiment – DRIFT project: Directional Recoil Identification From Tracks– T2K: Tokai to Kamiokande
INSTR08 – BINP, Novosibirsk – March 1st, 2008 14
• ICARUS (Imaging Cosmic And Rare Underground Signals) at Gran Sasso
• the biggest one ever build
• Observation:- high energy neutrinos (17 GeV) from CERN- solar ν (5-14 MeV)- supernovae ν (10-100 MeV)- atmospheric ν (1GeV)
• 300t of Liquid Argon (idea from C. Rubbia, 1977): -Argon is not electronegative: electrons may drift over very long distances- many e- are produced (60000/cm for a MIP particle) - + scintillation in Ar (50000 ph./cm for a MIP particle)- Argon is inexpensive (1% in the atmosphere)
• future: 100kT GLACIER LAr detector?
ICARUS for neutrinos Physics
INSTR08 – BINP, Novosibirsk – March 1st, 2008 16
GLACIER TPC• Giant Liquid Argon Charge Imaging ExpeRiment (A. Rubbia, hep-ph/0402110)
A scalable design:
10 kton
Ø = 70 m
h = 20 m
Passive perlite insulation
100 ktonElectronics crates
• Two phases Argon TPC
• LEM (Large Electron Multiplier) = thick macroscopicGEM readout, very long drift
• Single module cryo-tanker based on industrial Liquefied Natural Gas (LNG) technology
• Could potentially be magnetized
INSTR08 – BINP, Novosibirsk – March 1st, 2008 17
• DRIFT (Directional Recoil Identification From Tracks)
• negative ion TPC (C. Martoff, N. Spooner et al.)
• the most exotic !
• For detection:- WIMP- Axion
• electronegative gas additive (CS2) captures primary e- negative ions
• Excellent background discrimination
• future: large underground observatory
4m
8m
DRIFT for Dark Matter
INSTR08 – BINP, Novosibirsk – March 1st, 2008 18
T2K : Tokai to Kamiokande
• Long Baseline neutrino experiment with an intense beam (0.75MW)
• Aiming at 13 , and “atmospheric oscillation” measurements
• 2 detectors: far (SK) and near at 280 m from target • Off-axis beam• JPARC currently under construction first beam 2009
The 280 m detector is used to check the initial beam composition, it includes 3 largeMicromegas TPCs
B = 0.2 TB = 0.2 T
INSTR08 – BINP, Novosibirsk – March 1st, 2008 20
Plan of TPC R&D
• Develop the readout technologies– Tests with small prototypes
• Studies of the gas mixtures– Limit the diffusion– Find a stable state
• Improve the spatial resolution: resistive or digital anode– Resolution with short drift length is dominated by
• Readout pad pitch• Width of induced charge on pad plane
– To decrease pad pitch• Digital TPC• Increase signal width
Resistive anode pad readout, but two track separation might be less good
• Built and test a larger prototype to make the technology choice
• Design and produce the final TPC for the specific experiment
INSTR08 – BINP, Novosibirsk – March 1st, 2008 21
Micromegas & GEMs (MPGD)
50 µm
40 kV/cm
~1000 µm
1 kV/cm
GEM
~50 µm
80 kV/cm
Micromegas
Technology choice for TPC readout: Micro Pattern Gaseous Detector
• more robust than wires
• no E×B effect
• better ageing properties
• easier to manufacture
Avalanche
• fast signal & high gain
• low ion backdrift
• Gas Electron Multiplier (F. Sauli, 1997)
• 2 copper foils separated by kapton
• multiplication takes place in holes
• use of 2 or 3 stages
• MICROMEsh GAseous Structure(Y. Giomataris et al., 1996)
• metallic micromesh (typical pitch 50μm)
• sustained by 50μm pillars, multiplication between anode and mesh, high gain
• Gas Electron Multiplier (F. Sauli, 1997)
• 2 copper foils separated by kapton
• multiplication takes place in holes
• low gain
INSTR08 – BINP, Novosibirsk – March 1st, 2008 22
Micromegas & GEMs (MPGD)
• 2- or 3- stage amplification
• easy operation
• low field above the electronics
• low discharge probability
• simplicity
• single stage of amplification
• natural ion feedback suppression
• discharges non destructive
GEMMicromegas
Technology choice for TPC readout: Micro Pattern Gaseous Detector
• more robust than wires
• no E×B effect
• better ageing properties
• easier to manufacture
• fast signal & high gain
• low ion backdrift
INSTR08 – BINP, Novosibirsk – March 1st, 2008 23
Bulk Micromegas technology
Copper segmented anode
Lamination of Vacrel
Positioning of Mesh
Encapsulation
Development
FR4
Photo-imageablepolyamide film
Stainless steelwoven mesh
Border frame
Spacer
Contact to Mesh
Base Material
I. Giomataris et.al., NIM A560 (2006) 405
• Process to have an encapsulated mesh on a PCB
(mesh = stretched wires)
• Motivations for using bulk Micromegas
– the mesh is held everywhere:
no dead space, no frame
– robustness because it is closed to dust
– can be segmented
– repairable
INSTR08 – BINP, Novosibirsk – March 1st, 2008 24
Bulk-Micromegas prototypes of TPC for T2K
Geneva-Barcelona test bench
Test of a T2K module with a 55Fe source
Micromegas prototypes: • Bulk: 34x36 cm2, 128 m gap • 1728 pads of 6.9x9 mm²
HARP test at CERN (PS/T9)
MM1 detector + FEE + Cooling system
HARP solenoid (0.7 T)
Field cage1.5 m drift length
• Sep. 19th – Oct. 3rd 2007 (Analysis in progress)• Electronics: AFTER ASIC from Saclay
By T2K/TPC-Europe
INSTR08 – BINP, Novosibirsk – March 1st, 2008 25
Bulk-Micromegas prototypes for T2K
Signal from 55Fe source
= 8.5% rms @ 5.9 keV
= ~8% rms @ 5.9 keV
Lab Test HARP test at CERN (PS/T9)
Energy resolution consistent with lab. test results
• E = 160 V/cm, B = 0.2 T• Source located at 1.54 m from MM detector
INSTR08 – BINP, Novosibirsk – March 1st, 2008 26
Bulk-Micromegas prototypes for T2K
15 GeV/c p-Pb interactions in front of the TPCCosmic rays in the
TPCY
X
T
Y
55Fe source
HARP test: events display
INSTR08 – BINP, Novosibirsk – March 1st, 2008 27
Ion feedback measurements
Gain ~ 200σt = 9.5 μm
• 20 μm pitchp1 = 1.01
• 32 μm pitchp1 = 0.90
• 45 μm pitchp1 = 0.96
• 58 μm pitchp1 = 1.19
BF = p0/FRp1
• Measurements with a 45 μm gap InGrids
• Backflow fraction (BF) down to 1 permil at low picth and high field ratio
M. Chefdeville et al. IEEE/NSS 2007
INSTR08 – BINP, Novosibirsk – March 1st, 2008 28
Gating for ILC
• If natural ion backflow suppression is not sufficient, gating can reduce the number ions feeding back in the drift space
• Time structure: one ms train every 200 ms
• Gating can be done with wires or a GEM operated at unit gain
Wire gating GEM gating
Gate Open
Gate Closed
50mm/ms
- -
- -
- -
- -
- -
- -
- -
+ +
+ +
+ +
+ +
+ +
+ +
+ +
Previous beam train x-ings
INSTR08 – BINP, Novosibirsk – March 1st, 2008 30
100
1000
10000
100000
50 55 60 65 70 75 80 85 90 95 100
Field (kV/cm/atm)
Ga
in
Iso : 1%
Iso : 2%
Iso : 3%
Iso : 4%
Iso : 5%
CF4 : 3%, Iso : 1%
CF4 : 3%, Iso : 2%
CF4 : 3%, Iso : 3%
CH4 : 6%
CH4 : 7,5%
CH4 : 9%
CH4 : 10%
CH4 : 5%, CF4 : 3%
CH4 : 5%, CF4 : 5%
CH4 : 5%, CF4: 10%
CH4 : 10%, CF4 : 3%
CH4 : 5%, CO2 : 3%
CH4 : 10%, CO2 : 10%
CO2 : 10%
CO2 : 20%
CO2 : 30%
CO2 : 10%, Iso 2%
CO2 : 10%, Iso 5%
CO2 : 10%, Iso 10%
CF4 : 3%, CO2 : 1%
CF4 : 3%, CO2 : 3%
CF4 : 3%, CO2 : 5%
Iso : 2%, CH4 : 10%
Iso : 5%, CH4 : 10%
Iso : 10%, CH4 : 10%
Ethane 10%
Ethane 5%
Ethane 3,5%
Ethane 2%
Ethane 3,5% - CO2 10%
Ethane 3,5% - CF4 3%
Ethane 3,5% - CF4 10%
Ethane 3,5% - Iso 2%
Mixtures of gases containing argon: gain curves
iC4H10
CO2, CH4C2H6
Micromegas Mesh : 50 m gap of 10x10 cm² size
INSTR08 – BINP, Novosibirsk – March 1st, 2008 31
5%
10%
15%
20%
25%
30%
35%
40%
100 1000 10000 100000 1000000
Gain
RM
S
Iso : 1%
Iso : 2%
Iso : 3%
Iso : 4%
Iso : 5%
Energy resolution vs. gain
Argon/Isobutane
• Best RMS for a gain between 3.103 & 6.103
• Degradation increase in inverse proportion to the quencher
INSTR08 – BINP, Novosibirsk – March 1st, 2008 33
Spatial resolution: 5 T cosmic-ray test at DESY
5T magnet at DESY + COSMo TPC
Resistive anode
Micromegas
COSMo TPC
resistive foilgluepads
PCB
mesh
(r,t) integral over pads
(r)
r (mm)
Q(t)
t (ns)
M.S.Dixit et.al., NIM A518 (2004) 721
• COSMo (Carleton Ottawa Saclay Montréal) TPC+ 10 x 10 cm² Micromegas (50 μm gap) + resistive anode used to disperse the charge(126 pads of 2x6 mm²size)
INSTR08 – BINP, Novosibirsk – March 1st, 2008 34
Spatial resolution at 0.5T vs. gain
• B = 0.5 T, resolution fit by where Neff number of effective e-
• Resolution 0 ( at z = 0) ~ 50 µm still good at low gain (will minimize ion feedback)
• Mean of Neff = 27
Gain = 4700 Gain = 2500
Neff=25.2±2.1 Neff=28.8±2.2
x 02 Cd2 zNeff
0 = 1/40 of the pad pitch
INSTR08 – BINP, Novosibirsk – March 1st, 2008 35
Spatial resolution at 5T vs. gas mixtures
Ar Iso (95:5)
B = 5T
Ar Iso (95:5)
B = 5T
50 m
At high magnetic field (5T) ~ 50 µm independent of the drift distance
Dixit, Attié, et al., NIMA 581, 254 (2007)
Extrapolate to B = 4T with T2K gas for 2x6 mm² pads:
• DTr = 23.3 µm/cm, • Neff ~ 27,• 2 m drift distance,
Resolution of Tr 80 m will be possible !!!
INSTR08 – BINP, Novosibirsk – March 1st, 2008 36
Tsinghua: TPC prototype with GEM Readout
INSTR08 – BINP, Novosibirsk – March 1st, 2008 37
Tsinghua: 1 T cosmic-ray test at KEK
Test in Dec. 2007
Preliminary results !
INSTR08 – BINP, Novosibirsk – March 1st, 2008 39
• Chip (CMOS ASIC) upgraded in the EUDET framework from the Medipix chip developed first formedical applications
• IBM technology 0.25 µm
• Characteristics:– surface: 1.4 x 1.6 cm2
– Matrix of 256 x 256– pixel size: 55 x 55 µm2
• For each pixel:– preamp/shaper– threshold discriminator– register for configuration– TimePix synchronization logic– 14-bit counter
55 m
55 m
Description of the TimePix chip
INSTR08 – BINP, Novosibirsk – March 1st, 2008 40
TimePix/Micromegas chambers
• NIKHEF– Next-1,2 & 3– standard Micromegas– amorphous-Silicon protection
against discharges– Ingrid: Integrated Micromegas
using post-processing
• Saclay– Micro-TPC– standard Micromegas– amorphous-Silicon
protectionagainst discharges
– 6 cm height field cage
INSTR08 – BINP, Novosibirsk – March 1st, 2008 41
Cosmic-ray
time
• Chamber Next-1 at NIKHEF
• TimePix chip + SiProt + Ingrid
• Gas mixture : He/Iso (80:20)
• Maximum drift: 10 mm
• Amplification gap: 50 μm
• Cosmic-ray track:– Length : ~ 18 mm– Width : ~ 200 μm
• Before SiProt chips used to die due tosparking but now …
NIKHEF
INSTR08 – BINP, Novosibirsk – March 1st, 2008 42
• Image of discharges are being recorded
• Round-shaped pattern of some 100 overflow pixels
• Perturbations in the concerned column pixels
– Threshold?– Power?
Chip keeps working !!
Discharges are observed
• Provoke discharges by introducing small amount of Thorium in the Ar gas
- Thorium decays to Radon 222 which emits 2 alphas of 6.3 & 6.8 MeV- Depose on average 2.5.105 & 2.7.105 e- in Ar/iC4H10 80/20- at -420 V on the grid, likely to trigger discharges
INSTR08 – BINP, Novosibirsk – March 1st, 2008 43
TimePix/Micromegas Micro-TPC of Saclay
• Micro-TPC
• Timepix chip+ SiProt 20 μm+ Micromegas
• 90Sr
• Ar/Iso (95:5)
• Time Mode
• z ~ 40 mm
• Vmesh = -340 V
INSTR08 – BINP, Novosibirsk – March 1st, 2008 44
TimePix & GEMs
Freiburg (+Bonn)
Beam DESY II
Trigger (scint.) &Si-telescope
- Standard GEMs 100x100 mm2 with 140 μm of hole pitch
- News GEMs 24x28 mm2 with 50μm of hole pitch
puce TimePix :14 mm
• Test beam at DESY in 2007• Several gas mixture and two GEM systems were tested
Time
TOT
INSTR08 – BINP, Novosibirsk – March 1st, 2008 45
ILC-TPC collaboration
41 institutes
120 physicists
INSTR08 – BINP, Novosibirsk – March 1st, 2008 47
Large Prototype for ILC• Endplate of 7 panels, ø = 80 cm
• Two readout technology : GEM & MICROMEGAS (bulk)
• anode, resistive anode, pixels
80 cm
INSTR08 – BINP, Novosibirsk – March 1st, 2008 48
EUDET/LCTPC setup at DESY
• Field cage (DESY)
• 1 T magnet (KEK)
INSTR08 – BINP, Novosibirsk – March 1st, 2008 49
Conclusions
• Gaseous detectors have a long history behind them andthey, especially TPCs, have a promising future
• The new MPGD technologies are now mature unite in world-wide RD51 collaboration
• Physicists working on TPC R&D are now inside a huge collaboration over the world towards the future Linear Collider
• The ALICE TPC is getting ready for data taking at LHC
• T2K experiment will commission a large new generation TPC in 2009
• TPCs will permit a large development of many applications, not only in particle tracking, as usually in high energy and heavy ions physics,but also in rare event detection