The GOSSIP Calibrator for the ATLAS Muon Spectrometer

1. The GOSSIP Calibratorfor the ATLAS Muon Spectrometer Harry van der Graaf ATLAS/Detector R & D Nikhef, Amsterdam ATLAS Muon Week CERN, Geneva, Jan 30, 2008

2. Summary: - We have developed a new (gaseous) tracking detector - This detector potentially outperforms Si trackers due to: - low mass - low power consumption (thus mass) - radiation hardness and is therefore an interesting candidate for the ATLAS SCT Upgrade - We would like to demonstrate the new detector in ATLAS - It would be useful to have an independent Muon Calibrator in the ATLAS Muon Spectrometer [MUST (Schuller, Virchaut)!] - We propose to construct & install a GOSSIP Muon Calibrator

3. Cathode (drift) plane Si [depletion] layer Cluster1 Cluster2 1mm, 100V Vbias Cluster3 Integrated Grid (InGrid) CMOS chip 50um, 400V Slimmed Silicon Readout chip Input pixel 50um Si (vertex) track detector GOSSIP Gas: 1 mm as detection medium 99 % chance to have at least 1 e- Gas amplification ~ 1000: Single electron sensitive All signals arrive within 20 ns • Si strip detectors • Si pixel detectors • MAPs • CCDs

4. Grids Silicon wafer HV biasing Wafer post-processing:InGrid Hex / Pillars InGrid: an Integrated Grid on Si (wafers or chips) • perfect alignment of grid holes and pixel pads • small pillars Ø, hidden pillars, full pixel area coverage • Sub-micron precision: homogeneity • Monolithic readout device: integrated electron amplifier

5. Full post-processing of a TimePix Moiré effects + pillars CERN • Timepix chip + SiProt + Ingrid: MESA+ “Uniform” IMT Neuchatel Charge mode Timepix chip + Micromegas mesh:

6. Full post-processing of a TimePix • Timepix chip + SiProt + Ingrid: 14 mm MESA+ “Uniform” Charge mode IMT Neuchatel

7. A “scratch” occurred during the construction of Ingrid; Loose parts removed. Ingrid working!

8. Kα escape Kβ escape 13.6 % FWHM Kβ-filtered spectrum with Cr foil 11.7% FWHM New InGrid developments and results • Process improvement: grids much flatter • Extremely good energy resolution: 13.6 % FWHM with 55Fe in P10 • Removal of Kβ 6.5 keV line: 11.7 % @ 5.9 keV in P10 • With F=0.17 and Ne = 229 gain fluctuation ~ 0.5 • New wafer masks: hole pitches down to 20 μm with various diameters and gaps • Investigate Micromegas geometry • Test of the ion backflow theory feasible • Until now: 1 μm thin Al but can now be increased to 5 μm by electrolysis Expect less damaged from sparks

9. setup Next-1,2

10. Drifttime (bin = 10 ns) cathode @ - 1500 V 14 mm 10 mm A “long” cosmic track Timepix + 20 μm thick Siprot + Ingrid Stable operation in He iC4H10

11. Cosmic rays in Argon Time mode

12. 1.2 mm Gossip: replacement of Si tracker Essential: thin gas layer (1.2 mm)

13. GOSSIP-Brico: PSI-46 (CMS Pixel FE chip) First prototype of GOSSIP on a PSI46 is working: • 1.2 mm drift gap • Grid signal used as trigger • 30 µm layer of SiProt

14. We can see tracks! (Frame # 17 is really great) 7.8mm 8mm Animated GIF of 100 hits on the PSI46 brico, 30µm SiProt. (if this does not animate, drop the picture into a web browser)

15. Tracking sensor material: gas versus Si • it is light • primary electrons can simply be multiplied: gas amplification: low power • no bias current: low power & simple FE circuits • gas can be exchanged: no radiation damage of sensor • gas has a low εr: with small voxels the source capacity can be small (10 fF) • allowing fast, low-noise, and low-power preamps • gas is usually cheap • low sensitive for neutron and X-ray background • δ-rays can be recognized • [high ion & electron mobility: fast signals, high count rates are possible] • discharges/sparks: readout system should be spark proof • ageing: must be solved and must be understood / under control • diffusion: limits max. drift length

16. Un-coated anode Coated anode InGrid TimePix chip • SiProt protection against: • hot spark plasma • Too large charge in pixel circuitry [principle of RPCs] • local reduction of E-field: quenching • widening discharge funnel: signal dilution • increased distance of ‘influention’ 3 µm • SiProt: a low T deposited hydrogenated amorphous silicon (aSi:H) layer • Up to 50 μm thick films, ~1011Ω.cm

17. Final assessment: spark-proofness • 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 Charge mode Since 1 week, some 5.104 alpha events recorded in 1% of which …

18. Qmax ~ 1 – 2 fC Chip may die if Qmax > 10 fC

19. … discharges are observed ! For the 1st time: 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

20. Discharge signals on grid directly measured on scope

21. proportional signals from alfas discharges • CMOS chips are no longer destroyed • discharges in gas proportional chambers are hard to exclude • SiProt makes chips spark proof • This a-Si layer may be useful for the ATLAS Muon ‘Micromegas’ upgrade: • charge spread widening over anode pads

22. Demo Movie: ‘Helix event’ B = 0.2 Tesla Gas: He Isobutane 77/23 Irradiation with beta’s from 90Sr: endpoint 2.5 MeV

23. Ageing Radiation damage of CMOS pixel chip is relevant - common for all tracking detectors - believed to widthstand ATLAS Upgrade Dose in 90 nm technology Radiation damage of sensor: not relevant for Gossip sensor since this is gas being exchanged Typical for gaseous detectors: the deposit of an (insulating) polymer on the electrodes of a detector. Decrease of signal amplitude • Little ageing expected: • little primary ionisation (~ 10 e-/track) • low gas gain (500 – 1000) • large anode surface (compare pixel anode plane with surface of thin wire) • E-field at flat anode ~3 lower than E-field at anode wire

24. gas: standard Ar/Methane 90/10. Deposit containing C found on anode

25. set up ageing test

26. little ageing in Argon/Isobutane But: HV breakdown after 3 x 1015 MIPs

27. Upgraded SCT: Gossip could replace: • Pixel vertex detector: Gossip • Si Strip detectors: replace by Gossip Strixel detectors • TRT: use Gossip as tracker/TR X-ray detector • Essentials: • power dissipation: 60 mW/cm2 • intrinsic mass: 0.1 % radiation length • low cost: 10 $ / cm2

28. - Ladder strings fixed to end cones • Integration of beam pipe, end cones & pixel vertex detector • 5 double layers seems feasible

29. data lines (Cu/kapton) ladder cross section casted aluminium Gossip chip + InGrid drift gap cathode foil Stainless steel tube: - string - power - CO2 cooling ladder side view ladder top view

30. Upgraded SCT: Gossip/GridPix could replace: • Pixel vertex detector: Gossip • Si Strip detectors: replace by Gossip Strixel detectors • TRT: use GridPix as tracker/TR X-ray detector strixels/strips preamp channels ~ 20 mm • Essentials: • power dissipation: 1/16 x 60 mW/cm2 = 4 mW/cm2 • now:25 mW/cm2 • intrinsic mass: 0.1 % radiation length • low cost: 10 $ / cm2

31. Upgraded Tracker: Gossip could replace: • Pixel vertex detector: Gossip • Si Strip detectors: replace by Gossip Strixel detectors • TRT: use Gossip with 17 mm Xe layer • as tracker/TR X-ray detector • Essential: • high position-resolution tracker throughout tracker • low mass, low cost detector • Efficient TRD possible

32. Testbeam Nov 5 – 12, 2007 PS/T9: electrons and pions, 1 – 15 GeV/c L=30 mm V0 V1 f Transition Radiator 0.05 mm Anatoli Romaniouk, Serguei Morozov, Serguei Konovalov Martin Fransen, Fred Hartjes, Max Chefdeville, Victor Blanco Carballo

33. Particle Identification Samples pions (left) and electrons (right) 6 GeV/c

34. 5 (double) layer Gossip Pixel 4 layer Gossip Strixel radiator 3 layers Gossip TRT

35. Conclusions and plans • Gossip has shown to work with the PSI-46 CMS Pixel FE chip • With a 20 µm SiProt layer, CMOS chips are spark proof Next steps: • Build from PSI-46 + SiProt + InGrid • Demo ‘beam telescope’: testbeam work • ATLAS Muon Calibrator • Demo B-layer: to be installed in hot spot in ATLAS near beam pipe • Gas ageing studies: testing Si containing compounds (SiO2, SiH4, SiCnHm) • In framework of CERN R&D project RD51 (kick-off Worshop @ Nikhef April 2008) • Simulations • Development of general purpose GridPix chip TimePix-2

36. GOSSIP-Brico: PSI-46 (CMS Pixel FE chip) First prototype of GOSSIP on a PSI46 is working: • 1.2 mm drift gap • Grid signal used as trigger • 30 µm layer of SiProt

37. ATLAS MUON Projective extension plate design / BML common support The worst case is on HV side : BML HV common support Extension plate Lens bloc from Nikhef Projective platform Cutting out 2 Holes for common support screws Aluminium profile glued (+ 1 rivet)

38. RASNIK systems in the ATLAS Muon Spectrometer Muon Calibrator

41. 20 m 1 NIM crate eq. Gas Ar/CO2 Gas in HV power data Ethernet Could we implement this GOSSIP Calibrator ‘GOSCAL’ into the ATLAS Muon Spectrometer?

42. NIKHEF Harry van der Graaf, Max Chefdeville, Fred Hartjes, Jan Timmermans, Jan Visschers, Marten Bosma, Martin Fransen, Yevgen Bilevych, Wim Gotink, Joop Rovekamp, Lucie de Nooy University of Twente Cora Salm, Joost Melai, Jurriaan Schmitz, Sander Smits, Victor Blanco Carballo University of Nijmegen Michael Rogers, Thei Wijnen, Adriaan Konig, Jan Dijkema, Nicolo de Groot CEA/DAPNIA Saclay D. Attié, P. Colas, I. Giomataris CERN M. Campbell, X. Llopart University of Neuchatel/MTI Nicolas Wyrsch Czech Tech. Univ. Prague, Praha Pixelman: T. Holy et al.