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full electromagnetic simulation of multi-strip detectors. Diego González-Díaz (GSI-Darmstadt) A. Berezutskiy (SPSPU-Saint Petersburg), G. Kornakov (USC-Santiago de Compostela), M. Ciobanu (GSI-Darmstadt), Y. Wang (Tsinghua U.-Beijing), J. Wang (Tsinghua U.-Beijing).
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full electromagnetic simulation of multi-strip detectors Diego González-Díaz (GSI-Darmstadt) A. Berezutskiy (SPSPU-Saint Petersburg), G. Kornakov (USC-Santiago de Compostela), M. Ciobanu (GSI-Darmstadt), Y. Wang (Tsinghua U.-Beijing), J. Wang (Tsinghua U.-Beijing) Darmstadt, November 24th
Some references used in this talk [1a] H. Alvarez Pol et al., 'A large area timing RPC prototype for ion collisions in the HADES spectrometer', NIM A, 535(2004)277. [2a] A. Akindinov et al., 'RPC with low-resistive phosphate glass electrodes as a candidate for CBM TOF', NIM A, 572(2007)676. [3a] J. Wang et al., paper in preparation. [4a] L. Lopes et al., 'Ceramic high-rate RPCs', Nuclear Physics B (Proc. Suppl.), 158(2006)66. [5a] D. Gonzalez-Diaz et al., 'The effect of temperature on the rate capability of glass timing RPCs', NIM A, 555(2005)72. [6a] A. Ammosov et al., talk at XIII CBM collaboration meeting, Darmstadt, Germany. [7a] L. Nauman et al., talk at XIV CBM collaboration meeting, Split, Croatia. [1] A. Mangiarotti et al., 'On the deterministic and stochastic solution of Space-Charge models and their impact in high resolution timing' talk at RPC Workshop Seoul, 2005. [2] G. Chiodini et al., 'Characterization with a Nitrogen laser of a small size RPC', NIM A 572(2007)173. [3] A. Colucci et al., 'Measurement of drift velocity and amplification coefficient in C2H2F4-isobutane mixtures for avalanche-operated resistive-plate counters', NIM A, 425(1999)84. [4] W. Riegler et al., 'Detector physics and simulations of resistive plate chambers', 500(2003)144 . [5] E. Basurto et al., 'Time-resolved measurement of electron swarm coefficients in tetrafluoretane (R134a)', Proc. to 28th ICPIG, Prague, 2007. [6] P. Fonte, V. Peskov, 'High resolution TOF with RPCs', NIM A, 477(2002)17. [7] P. Fonte et al., 'High-resolution RPCs for large TOF systems', NIM A, 449(2000)295. [8] A. Akindinov et al. 'Latest results on the performance of the multigap resistive plate chamber used for the ALICE TOF', NIM A 533(2004)74. [9] G. Aielli et al., 'Performance of a large-size RPC equipped with the final front-end electronics at X5-GIF irradiation facility', NIM A 456(2000)77. [10] S. An et al., 'A 20 ps timing device—A Multigap Resistive Plate Chamber with 24 gas gaps', NIM A 594(2008)39. [11] A. Blanco et al., 'In-beam measurements of the HADES-TOF RPC wall', NIM A 602(2009)691. [12] W. Riegler, D. Burgarth, 'Signal propagation, termination, crosstalk and losses in resistive plate chambers', NIM A 481(2002)130. [13] T. Heubrandtner et al., NIM A 489(2002)439.
The Compressed Baryonic Matter Experiment Transition Radiation Detectors Tracking Detector Electro- magnetic Calorimeter Muon detection System Ring Imaging Cherenkov Detector Silicon Tracking Stations Projectile Spectator Detector (Calorimeter) Vertex Detector Dipole magnet Resistive Plate Chambers (TOF)
The CBM-TOF wall. Design requirements • Overall time resolution (including start time) σT = 80 ps. • Occupancy < 5 % for Au-Au central collisions at E=25 GeV/A. • Space resolution ≤ 5 mm x 5 mm. • Efficiency > 95 %. • Pile-up < 5%. • Rate capability = 20 kHz/cm2. • Multi-hit capability (low cross-talk). • Compact and low consuming electronics (~65.000 electronic channels). • Multi-strip design in the outer region, due to the very low occupancies. Why? -> Why not?. If electrically possible it is mechanically much more easy.
The CBM-TOF wall. Simulation based on occupancies In order to accommodate the different granularities as a function of the polar angle, five different regions were defined: • Padregion (1): 2.0 x 2.0 cm2 ( 27072 channels, ~10 m2) • Strip region (2): 2.0 x 12.5 cm2 ( 3840 x 2 channels, ~10 m2) • Strip region (3): 2.0 x 25.0 cm2 ( 5568 x 2 channels, ~30 m2) • Strip region (4): 2.0 x 50.0 cm2 ( 6150 x 2 channels, ~60 m2 ) • Strip region (5): 2.0 x 100.0 cm2 ( 2900 x 2 channels, ~60 m2 ) TOTAL ( ~65000 channels, ~170m2)
A multi-gap RPC in general. Here a differential RPC ('a la' STAR), just for the sake of 'electrical elegance' *parameters not from STAR differential pre-amplifier particle HV insulator with Vbreak>10-15 kV standard PCB with read-out strips on one side Rin +V at least 4 gas gaps (~0.3 mm thick) -V float glass HV coating with R~100 MΩ/□
More electrical schemes are (un)fortunately possible HADES-SIS FOPI-SIS ALICE-LHC -V -V V V -V -V STAR-RHIC -V -V V V ! V -V V -V V S. An et al., NIM A 594(2008)39 [10] all these schemes are equivalent regarding the underlying avalanche dynamics... but the RPC is also a strip-line, and this is manifested after the avalanche current has been induced. And all these strip-lines have a completely different electrical behavior. HV filtering scheme is omitted
Generation + induction + transmission + FEE. Sketch transmission 1 2 generation + induction 4 3 multi-strip FEE response
Avalanche generation. A simple avalanche model 8.7 Raether limit log10 nelectrons space-charge regime ~7.5 ~7 exponential-growth regime threshold ~2 exponential-fluctuation regime 0 to tmeas t avalanche Furry-type fluctuations simplifying assumptions • The stochastic solution of the avalanche equation is given by a simple Furry law(non-equilibrium effects are not included). • Avalanche evolution under strong space-charge regime is characterized by no effective multiplication. The growth stops when the avalanche reaches a certain number of carriers called here ne,sat. • The amplifier is assumed to be slow enough to be sensitive to the signal charge and not to its amplitude. We work, for convenience, with a threshold in charge units Qth.
Parameters of the gas used for input: α* (effective Townsend coefficient), vd (drift velocity), no (ionization density) little dependence with mixture! no [mm-1] HEED (from Lippmann[4]) αextrapolated to mixture by using Freon's partial pressure: αmixture = αFreon(E/fFreon) fFreon *purely phenomenological! continuous line: data from Basurto et al. in pure Freon [5] vddirectly taken from Freon (inspired on microscopic codes) vd,mixture = vd,Freon
MC results. Efficiency and resolution for 'wide-pad' detectors
MC results. Prompt charge distributions for 'wide-pad' detectors 1-gap 0.3 mm RPC standard mixture 4-gap 0.3 mm RPC standard mixture Eff = 74% Eff = 60% Eff = 38% simulated simulated measured qinduced, prompt [pC] qinduced, prompt [pC] measured assuming space-charge saturation at ne,sat= 4.0 107 (for E=100 kV/cm) data from Fonte, [6,7] qinduced, total [pC]
Generation + induction + transmission + FEE transmission 1 2 generation + induction 4 3 multi-strip FEE response
Induction and weighting field Ez read-out ws-s ~0 mm g=0.3 mm t=2.5 mm HV w=22 mm wide-pad limit t << w additionally when g<<t (typical situation) Ez does not depend on the position –z- along the gap We adapted to multi-gap the formulas from: problem: under-estimation of Ez for large inter-strip separations T. Heubrandtner et al. NIM A 489(2002)439
Cross-talk in a 2-strip RPC modeled as a loss-less transmission-line (I) W. Riegler, D. Burgarth, NIMA 481(2002)130 [12] see if a 4-gap RPC seen as a transmission-line dominated by skin-effect: small for typical dimensions and rise-times very small, due to the presence of gas and glass two different modes in the transmission line!. This causes 'modal dispersion' unless: true for homogeneous transmission lines! 1) for typical materials (glass) loss-less line! 2)
Cross-talk in a 2-strip RPC modeled as a loss-less transmission-line (II). Limits. zo = position along the strip where the signal is induced for exponential signals small dispersion high-frequency /large distance / dispersive limit low-frequency /small distance / non-dispersive limit very large dispersion the 2 modes are fully decoupled see also [12]
Cross-talk influence in the timing of a coincident (double) hit. A simple derivation (I). space-charge log[i(t)] ith exponential regime t variations in base-line due to cross-talk variations in time at threshold due to cross-talk
Cross-talk influence in the timing of a coincident (double) hit. A simple derivation (II). Assumptions: • Within the same primary collision cross-talk extends up-to infinite time. • It does not depend on position. • Fluctuations in time of cross-talk signal are smaller than fluctuations coming from the avalanche charge distribution. • Pick-up strips are separated by a typical distance bigger than the area of influence of the avalanche. Charge sharing during induction can be neglected!. • Cross-talk is small, given by Fct. cross-talk is expected to affect timing when
History revisited: 1.6m-long 2-strip RPC (P. Fonte et al., 2002) strip separation = 1mm gap = 0.3mm glass = 3mm width = 5cm length= 1.6m
Zc~13 Ω Cross-talk in Fonte multi-strip RPC Cm=88 pF/m BW=1.5 GHz Rin=50 Ω experimental conditions: Π, E=3.5 GeV, low rates, trigger width = 2 cm Cg=521 pF/m Fct=50%! very dispersive! transverse scan 'fine-tunning' Fct=40% HV=5.7 kV 80%-90% measured cross-talk levels reproduced
Minimizing cross-talk (I) ->increase strip separation Cg Cm Δv/v trise x10
Minimizing cross-talk (II) ->increase strip/width separation ->reduce glass thickness Cg Cm Δv/v trise /2.5 x6 /6
Minimizing cross-talk (III) ->increase strip/width separation ->reduce glass thickness ->reduce band-width Cg Cm Δv/v low coupling low dispersion trise BW/10 /2.5 x6 /6
Minimizing cross-talk (IV) ->put guard strip Cg Cm Δv/v trise guard strip
Minimizing cross-talk (V) ->use only two electrodes Cg Cm (it flips!) Δv/v trise not mirrored
Minimizing cross-talk (VI) ->use only two electrodes ->couple locally to ground Cg Cm Δv/v low coupling NO dispersion trise not mirrored coupling to PCB
Minimizing cross-talk + detector response (IV) BW/10 /2.5 x6 /6
Minimizing cross-talk + detector response (V) not mirrored coupling to PCB
'some' of the new CBM prototypes(preliminary short compilation)
Zc~18 Ω 35-cm long wide-strip, mirrored and shielded Cm experimental conditions: ~mips from p-Pb reactions at 3.1 GeV, low rates, trigger width = 2 cm BW=260 MHz Rin=100 Ω ... ... Cg little dispersive Fct=11% transverse scan 'fine-tunning' inter-strip region dominated by trigger width Fct=19% probability of pure cross-talk: 1-3% Analysis with high resolution tracking on-going.
1-mlong counter, 6-strip RPC, 12-gap, mirrored and shielded experimental conditions: ~mips from p-Pb reactions at 3.1 GeV, low rates, trigger width = 2 cm (< strip width) long run. Very high statistics. ... ... No simulations available yet
1-m long counter, 12-gap, mirrored and shielded double-hit in any of 3rd neighbors double-hit in any of 2nd neighbors double-hit in any of 1st neighbors no double hit No simulations available yet
Multi-strip design of timing RPCs at 1-m scale with acceptable cross-talk, small cluster size and small deterioration of time resolution seems doable. Further optimized structures based on simulations are on the way (Fct~1%). For making a multi-strip fully robust against streamer-crosstalk there is still a long way to go (maybe impossible). -> Detailed optimization based on physics performance soon to follow. Then we will know if cross-talk is 'high' or not. conclusions and outlook
The FOPI counter Multi-strip-MRPC (MMRPC) Glass: ε=7.5, strip width = 1.64 mm, strip gap = 0.9 mm, strip length = 900 mm copper (20 μm) 8 gaps 1.1 mm 0.22 mm 0.5 mm 1.1 mm
Cross-talk in an un-terminated line 50 50 anode 1 cathode 1 50 50 50 50 anode 2 cathode 2 50 50 signal from BC420 scintillator (used as current generator) 50 50 anode 3 cathode 3 50 50 50 anode 4 cathode 4 50 50 50 anode 5 cathode 5 50 50
Cross-talk in a terminated line 50 50 anode 1 cathode 1 50 50 50 50 anode 2 cathode 2 50 50 50 50 anode 3 cathode 3 50 50 50 50 anode 4 cathode 4 50 50 50 50 anode 5 cathode 5 50 50
Cross-talk and signal shape low dispersion counter, typical working conditions, BW=260 MHz cross-talk constant, very independent from the signal shape Take as a typical shape the one of an avalanche produced at the cathode Even for dispersive counters it is reasonable since most of the charge is coming from that region
The FOPI counter (11th strip) cathode 50 50 anode 0 50 50 anode 1 50 50 .......... 50 50 anode 11 50 50 anode 12 50 50 anode 13 50 50 anode 14 50 50 anode 15
The FOPI counter (9th strip) cathode 50 50 anode 0 50 50 anode 1 50 50 .......... 50 50 anode 9 50 50 anode 10 50 50 anode 11 50 50 anode 12 50 50 ..........