november 4, 2004carl bromberg, fnal lar exp. workshop nov. 4-6, 20041 liquid argon as an active...
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November 4, 2004Carl Bromberg, FNAL LAr Exp. Workshop Nov. 4-6, Liquid Argon basics W ion (1 MeV e – )23.6 eV Radiation Length19.55 g/cm 2 (14.0 cm) Density1.395 g/cm 3 (1 bar) Boiling Point87.2 K (1 bar) 89.3 K (1.25 bar) Nucl. Int. Length117 g/cm 3 Diffusion Coef.4.8 cm 2 /s Recombination factor0.64 (decreases ions/cm) dE/dx (min)2.1 MeV/cm e – in 3mm sampleTRANSCRIPT
November 4, 2004 Carl Bromberg, FNAL LAr Exp. Workshop Nov. 4-6, 2004 1
Liquid argon as an active medium
Carl Bromberg Michigan State University
& Fermilab (2004)
Better titleWhat has been learned by
ICARUS collaboration from ~20 years of drifting electrons in LAr
November 4, 2004 Carl Bromberg, FNAL LAr Exp. Workshop Nov. 4-6, 2004 2
Sources
• Talk by F. Sergiampietri, at NuFact ‘01 (LANNDD)• Talk by A. Para at Fermilab (Wine & Cheese)• Publications
– “Design, construction and tests of the ICARUS T600 detector”, NIM A527, 329 (2004)
– “Study of electron recombination in liquid Argon with the ICARUS TPC” NIM A523, 275 (2004)
– Measurement of the muon decay spectrum with the ICARUS T600 liquid Argon TPC”, Euro Phys J C33,2 (2004) 233
See list of ICARUS talks and papers onFLARE web site
/www-off-axis/flare/documents.htm
Particularly:
November 4, 2004 Carl Bromberg, FNAL LAr Exp. Workshop Nov. 4-6, 2004 3
Liquid Argon basicsWion (1 MeV e–) 23.6 eVRadiation Length 19.55 g/cm2 (14.0 cm)Density 1.395 g/cm3 (1 bar)Boiling Point 87.2 K (1 bar)
89.3 K (1.25 bar)Nucl. Int. Length 117 g/cm3
Diffusion Coef. 4.8 cm2/s Recombination factor
0.64 (decreases ions/cm)
dE/dx (min) 2.1 MeV/cme– in 3mm sample : 16,000e−t/t , t : 5 −10m s
November 4, 2004 Carl Bromberg, FNAL LAr Exp. Workshop Nov. 4-6, 2004 4
November 4, 2004 Carl Bromberg, FNAL LAr Exp. Workshop Nov. 4-6, 2004 5
TPC operation• Time Projection
– electrons drift toward transparent wire planes (minimum 1), and collection wire plane
– planes with wires at various angles for stereo
• Ambiguities– track parallel to wire planes,
all hits have same time, i.e., x.
– track “dip” resolved by space points: vertices, delta rays or ionization bumps
– distance between space points changes in the two views
ZX (Time)Y60°
delta ray
vertex
November 4, 2004 Carl Bromberg, FNAL LAr Exp. Workshop Nov. 4-6, 2004 6
Signal characteristics
• Diffusion not a big factor in signal shape for d ~ 2 m• Fit for x-position, resolution < 1 mm (2.5 MHz clock), helps
with ambiguity resolution. • Even with significant overlap in time, distinguish 1 track from
2, by consistent ionization/pulse width over many wires. • But tracks in drift direction have very distorted pulse shapes
FWHM ~ 4.5 mm tracks = 16 mm
November 4, 2004 Carl Bromberg, FNAL LAr Exp. Workshop Nov. 4-6, 2004 7
Energy ResolutionElectron energy
E resolution
s =11% E(MeV) ⊕ 2%
Stopping m± → e±ν ν
November 4, 2004 Carl Bromberg, FNAL LAr Exp. Workshop Nov. 4-6, 2004 8
FLARE is not ICARUS• Typical ICARUS capacitance is 20 pF/m + 200
pF cable ~400 pF (max) induction wire• Induction signals are smaller than collection
signals by ~30% • FLARE will have wires 4 times as long, noise
will be 1.6 times larger, yielding S/N ~ 8• Does increasing wire spacing (to say 5 mm)
help by lowering capacitance and increasing the signal?
• Cables for horizontal or stereo wires? Long cables mean more capacitance. Restrict to collection wires.
• Pixels anyone? K. McDonald.
November 4, 2004 Carl Bromberg, FNAL LAr Exp. Workshop Nov. 4-6, 2004 9
For what is needed? • Energy resolution of 2% great for EM shower. For total
energy, make corrections based on particle ID via ionization changes, range, ->m->e decays, nuclear fragments & n-stars
• Full reconstruction is probably not needed. Automated scanning perhaps possible in 2D
• In scanning simulations, stereo views were not that useful. Helped in large angle particle ID, but not often in electron ID.
• Automatic space point finding is a challenge• Cosmic Rays (during 1.3 ms readout). Should do
simulation. Get ICARUS raw data? Interest by others trying to do surface calorimetry and tracking.
νm → νe