Title: Detection Techniques
1Detection Techniques
2Liquid Argon TPC (ICARUS)
- Electronic Bubble chamber
- Planes of wires (3mm pitch) widely separated
(1.5m) 55K readout channels! - Very Pure Liquid Argon
- Density 1.4, Xo14cm lINT 83cm
- 3.6x3.9x19.1m3 600 ton module (480fid)
3Half Module of ICARUS
View of the inner detector
4Liquid Argon TPC
Raw Data to Reconstructed Event
- Because electrons can drift a long time (gt1m!) in
very pure liquid argon, this can be used to
create an electronic bubble chamber
5dE/dx in Materials
- Bethe-Block Equation
- x in units of g/cm2
- Energy Loss Only f(b)
- Can be used for Particle ID in range of momentum
6Full 2D View from the Collection Wire Plane
2
Drift coord. (m)
2
1
3
2
Wire coord. (m)
2
4
6
18
12
1
El.m. shower
2
Zoom views
m stop and decay in e
Detail of a long (14 m) m track with d-ray spots
3
El.m. shower
T600 test _at_ Pv Run 201 - Evt 12
7Full 2D view from the Collection Wire Plane
2
Drift Coord. (m)
Wire coord. (m)
2
6
4
18
12
Zoom View
3.9 m
1.3 m
T600 test _at_ Pv Run 308 - Evt 7
Large el.m. shower
8Events with Hadrons
2D view
2D view
- Trk. 1 - m.i.p.
- Edep 31 MeV
- Ltrk 18 cm
- Trk. 2 heavily i.p.
- Edep 191 MeV
- Ltrk 53 cm
- Trk. 3 - m.i.p.
- Edep 105 MeV
- Ltrk 60 cm
- Trk. 4 - heavily i.p.
- Edep 42 MeV
- Ltrk 16 cm
- Trk. 5 - m.i.p.
- Edep 111 MeV
- Ltrk 60 cm
vertex
vertex
Preliminary analysis
10 m3 test _at_ LNGS Run 641 - Evt 14 (Apr. 14th,
2000)
Monte Carlo ne Charged Current Event
9Steel/Scintillator Detector (MINOS)
- 8m octagon steel scintillator calorimeter
- Sampling every 2.54 cm
- 4cm wide strips of scintillator
- 5.4 kton total mass
- 55/?E for hadrons, 23/?E for electrons
- 486 planes of scintillator
- 95,000 strips
10MINOS in Soudan
- 5.4 kton total mass
- 55/?E for hadrons
- 23/?E for electrons
- 486 planes of scintillator
- 95,000 strips
May 14, 2002
11Events at MINOS
2.4GeV nmCC
25GeV nmCC
8.5GeV neCC
10GeV nNC
12MINI-MINOS beam test (at CERN)
- Mini detector with sixty 1 m2 planes
- Ran last summer with FD electronics
- ND electronics and higher energies this year
- Tested with hadrons, electrons, and protons
Expected resolution, 23/?E constant term lt5
Preliminary
13Backgrounds in Neutrino Factories
14Detector-Dependent Backgrounds
- The denser the detector, the more likely the
meson in the hadronic shower will interact before
decaying
15LOw DENsity Calorimeter
- Low z absorber to maximize detector mass for a
given X0 sampling recycled plastic pellets?
Other? - Cheap, reliable detector glass RPC
- Two-dimensional information per sample
- Simple, understood technology
- Can start detector construction with minimal
delay -
16ne Charged Current
17n Neutral Current Event
18LoDensity Energy Resolution
- ne Charged Current Events (ylt.5)
19Cerenkov Light
As particles move faster than the speed of light
in that medium, they emit a shock wave of light
- For water, n(280-580nm)1.33-6
- Threshold Angle 42o
20Event Reconstruction in Cerenkov Detector
- Vertex Point fit time of flight should be as
sharp as possible - Define set of in-time tubes
- Use Hough Transform to find rings
- Look for rings until youre done
- Particle ID
- Corrections to Vertex
- Energy Reconstruction
- Decay Electron Finding
21Particle ID Using Cerenkov Light
22Super-Kamiokande detector
50,000 ton water Cherenkov detector (22.5 kton
fiducial volume) 1000m underground (2700
m.w.e.) 11,146 20-inch PMTs for inner
detector 1,885 8-inch PMTs for outer detector
23Inside the Super-K Experiment
24(No Transcript)
25Single-Ring Energy Resolution
26Charged or Neutral Current?
27Charged or Neutral Current?
28MiniBooNE detector Cerenkov with Mineral Oil
total volume 800 tons (6 m radius) fiducial
volume 445 tons (5m radius)
1280 PMTs in detector at 5.5 m radius
10 photocathode coverage 240 PMTs in veto
Phototube support structure provides opaque
barrier between veto and main volumes
29Differences Between Oil and Water Cerenkov
30NuTeV Coarse-Grained Calorimeter
31Coarse-Grained Detector
32Neutral and Charged Current Events..what about
nes?
33NuTeV Energy Resolution
- Calibration Beams of p and e
34nt detection (OPERA)
- Challenge making a Fine-grained and massive
detector to see kink when tau decays to something
plus nt
35nt detection (OPERA)
36nt backgrounds
- Cut on invariant mass of primary tracks
37nt events expected (OPERA)
- Comparison 4 nt events over 0.34 background at
DONUT .27kton