Hartmut F.-W. Sadrozinski, US ATLAS Upgrade Meeting Nov 10, 20051 Tracking Detector Material Issues for the sLHC Hartmut F.-W. Sadrozinski SCIPP, UC Santa.

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Hartmut F.-W. Sadrozinski, US ATLAS Upgrade Meeting Nov 10, Tracking Detector Material Issues for the sLHC Hartmut F.-W. Sadrozinski SCIPP, UC Santa Cruz, CA 95064

Hartmut F.-W. Sadrozinski, US ATLAS Upgrade Meeting Nov 10, Outline of the talk - Motivation for R&D in new Detector Materials - Radiation Damage - Initial Results with p-type Detectors - Expected Performance - R&D Plan - Much of the data from RD In collaboration with Mara Bruzzi and Abe Seiden - Presumably this is relevant for both strips and pixels - Will not discuss 3-D detectors here Announcement: 2nd Trento Workshop on Advanced Detector Design (focus on 3-D and p-type SSD) Feb 15. –

Hartmut F.-W. Sadrozinski, US ATLAS Upgrade Meeting Nov 10, Motivation for R&D in New Detector Materials - The search for a substitute for silicon detectors (SSD) has come up empty. - Radiation damage in SSDs impacts the cost and operation of the tracker. - What is wrong with using the p-on-n SSD a la SCT in the upgrade? - Type inversion requires full depletion of the detector - Anti-annealing of depletion voltage constrains thermal management - Large depletion voltages require high voltage operation - Slower collection of holes wrt to electrons increases trapping - What is wrong with using the n-on-n SSD a la ATLAS pixels in the upgrade? - Cost: double-sided processing about 2x more expensive - Type inversion changes location of junction (but permits under-depleted operation) - Strip isolation challenging, interstrip capacitance higher? -Potential solution: SSD on p-type wafers (“poor man’s n-on-n”) - Single-sided processing, no change of junction - Strip isolation problems still persist - Need to change the wafer properties to reduce the large depletion voltages: MCz

Hartmut F.-W. Sadrozinski, US ATLAS Upgrade Meeting Nov 10, Charge collection efficiency CCE on n-side G. Casse, 1st RD50 Workshop, 2-4 Oct n-side read-out after irradiation. 1060nm laser CCE(V) for the highest dose regions of an n-in-n ( p/cm 2 ) and p-in-n ( p/cm 2 ) irradiated LHC-b full-size prototype detector.

Hartmut F.-W. Sadrozinski, US ATLAS Upgrade Meeting Nov 10, Radiation Effects in Silicon Detectors Basic effects are the same for n-type and p-type materials. - Increase of the leakage current. - Change in the effective doping concentration (increased depletion voltage), - Shortening of the carrier lifetimes (trapping), - Surface effects (interstrip capacitance and resistance). The consequence for the detector properties seems to vary widely. - An important effect in radiation damage is the annealing, which can change the detector properties after the end of radiation. - The times characterizing annealing effects depend exponentially on the temperature, constraining the temperature of operating and maintaining the detectors. - Fluence dependent effects normalized to equivqlent neutrons (“neq”), We use mostly proton damage constants and increase the fluence by 1/0.62.

Hartmut F.-W. Sadrozinski, US ATLAS Upgrade Meeting Nov 10, particle Si s Vacancy + Interstitial Point Defects (V-V, V-O.. ) clusters E K > 25 eV E K > 5 keV Frenkel pair V I Radiation Induced Microscopic Damage in Silicon Trapping (e and h)  CCE shallow defects do not contribute at room temperature due to fast detrapping charged defects  N eff, V dep e.g. donors in upper and acceptors in lower half of band gap generation  leakage current Levels close to midgap most effective Influence of defects on the material and device properties

Hartmut F.-W. Sadrozinski, US ATLAS Upgrade Meeting Nov 10, Leakage Current Hadron irradiation Annealing Damage parameter  (slope)  independent of  eq and impurities  used for fluence calibration (NIEL-Hypothesis) Oxygen enriched and standard silicon show same annealing Same curve after proton and neutron irradiation 80 min 60  C M. Moll, Thesis, 1999

Hartmut F.-W. Sadrozinski, US ATLAS Upgrade Meeting Nov 10, V dep and N eff depend on storage time and temperature T = 300K ShallowDonor Removal Beneficial Annealing Reverse Annealing G.Lindstroem et al, NIMA 426 (1999) Short term: “Beneficial annealing” Long term: “Reverse annealing” time constant : ~ 500 years (-10°C) ~ 500 days ( 20°C) ~ 21 hours ( 60°C) 30min (80°C) M. Bruzzi, Trans. Nucl. Sci. (2000) Stable Damage 80min at 60°C after inversion and annealing saturation N eff  

Hartmut F.-W. Sadrozinski, US ATLAS Upgrade Meeting Nov 10, Charge Collection Efficiency Limited by: Collected Charge : W: Detector thickness d: Active thickness  c : Collection time  t : Trapping time  Partial depletion  Trapping at deep levels  Type inversion (SCSI) 1/  e,h = β e,h ·  eq [cm -2 ] From TCT measurements within RD50:  t ~ 0.2*   /  t ~ 0.2 ns for   cm - 2 Luckily this is excludedby CCE measurements:   t ~ 0.48*   /  Fluence  [neq/cm 2 ] 3· · · ·10 15 Trapping time [ns]

Hartmut F.-W. Sadrozinski, US ATLAS Upgrade Meeting Nov 10, Influence the defect kinetics by incorporation of impurities or defects: Oxygen Initial idea: Incorporate Oxygen to getter radiation-induced vacancies  prevent formation of Di-vacancy (V 2 ) related deep acceptor levels Higher oxygen content  less negative space charge One possible mechanism: V 2 O is a deep acceptor OVO (not harmful at RT) V VOV 2 O (negative space charge) V 2 O(?) EcEc EVEV VO V 2 in clusters Defect Engineering of Silicon DOFZ (Diffusion Oxygenated Float Zone Silicon) RD48 NIM A465 (2001) 60

Hartmut F.-W. Sadrozinski, US ATLAS Upgrade Meeting Nov 10, Discrepancy between CCE and CV analysis observed in n-type (diodes / SSD, ATLAS / CMS, DOFZ / Standard FZ) ■ ● ♦ ▲ To maximise CCE it is necessary to overdeplete the detector up to : V bias ~ 2 V dep Caveat with n-type DOFZ Silicon

Hartmut F.-W. Sadrozinski, US ATLAS Upgrade Meeting Nov 10, Caveat: The beneficial effect of oxygen in proton irradiated silicon microstrip almost disappear in CCE measurements G.Casse et al. NIM A 466 (2001) ATLAS microstrip CCE analysis after irradiation with 3 x p/cm 2

Hartmut F.-W. Sadrozinski, US ATLAS Upgrade Meeting Nov 10,  Miniature n-in-p microstrip detectors (280  m thick) produced by CNM-Barcelona using a mask-set designed by the University of Liverpool.  Detectors read-out with a SCT128A LHC speed (40MHz) chip  Material: standard p-type and oxygenated (DOFZ) p-type  Irradiation: 24GeV protons up to p cm -2 (standard) and p cm -2 (oxygenated) CCE ~ 60% after p cm -2 at 900V( standard p-type) CCE ~ 30% after p cm V (oxygenated p-type) At the highest fluence Q~6500e at V bias =900V. Corresponds to: ccd~90µm, trapping times 2.4 x larger than previously measured. CCE n-in-p microstrip detectors G. Casse et al., Nucl. Inst Meth A 518 (2004)

Hartmut F.-W. Sadrozinski, US ATLAS Upgrade Meeting Nov 10, Recent n-in-p Results Detector with 1.1× p/cm 2 Important to check that there are no unpleasant surprises during annealing. Minutes at 80 o C converted to days at 20 o C using acceleration factor of 7430 (M. Moll). Detector after 7.5× p/cm 2 showing pulse height distribution at 750V after annealing. (Landau + Gaussian fit) G. Casse et al., 6 th RD50 Workshop, Helsinki June

Hartmut F.-W. Sadrozinski, US ATLAS Upgrade Meeting Nov 10, Expected Performance for p-type SSD Conservative Assumptions:  p  = 2.5· A/cm (only partial anneal) C total = 2 pF/cm V dep = 160V +  ( with 2.7* V/cm 2 ) (no anneal) (=  = neq/ cm 2 )   Noise = (A + B·C) 2 + (2·I·  s )/q A = 500, B = 60 S/N for Short Strips for different bias voltages: Details in : “Operation of Short-Strip Silicon Detectors based on p-type Wafers in the ATLAS Upgrade ID M. Bruzzi, H.F.-W. Sadrozinski, A. Seiden, SCIPP 05/09 no need for thin detectors, unless n-type: depletion vs. trapping 600V seems to be sufficient

Hartmut F.-W. Sadrozinski, US ATLAS Upgrade Meeting Nov 10, Expected Performance for p-type SSD, cont. Noise for SiGe Frontend (see talk by Alex Grillo) Leakage current important: Trade shaping time against operating temperature ( 20 ns & -20 o C vs. 10 ns & -10 o C ) Fluence: 2.2·10 15 neq/cm 2 (short strips) 2.2·10 14 neq/cm 2 (long strips) The maximum bias voltage is 600 V Temperature: -10 deg C

Hartmut F.-W. Sadrozinski, US ATLAS Upgrade Meeting Nov 10, Expected Performance for p-type SSD, cont. Heat Generation in 300  m SSD Only from active volume

Hartmut F.-W. Sadrozinski, US ATLAS Upgrade Meeting Nov 10, n-type and p-type detectors processed at IRST- Trento Microstrip detectors Inter strip Capacitance test Test2 Test1 Pad detector Edge structures Square MG-diodes Round MG-diodes An Italian network within RD50: INFN SMART Wafers Split in: 1.Materials: (Fz,MCz,Cz,EPI) 2.Process: Standard Low T steps T.D.K. 3.Isolation: Low Dose p-spray High Dose p-spray

Hartmut F.-W. Sadrozinski, US ATLAS Upgrade Meeting Nov 10, V dep variation with fluence (protons) and annealing time (C-V): SMART News: Annealing behaviour of MCz Si n- and p-type A.Macchiolo et al. Submitted to NIM A, presented at PSD 7, Liverpool, Sept G. Segneri et al. Submitted to NIM A, presented at PSD 7, Liverpool, Sept Beneficial annealing of the depletion voltage: 14 days at RT, 20 min at 60 o C. 3 min at 80 o C. Reverse (“anti-”) annealing starts in p-type MCz: at 10 min at 80 o C, 250 min (=4 hrs) at 60 o C, >> 20,000 min (14 days) at RT, in p-type FZ : at 20 min at 60 o C in n-type FZ: at 120 min at 60 o C.

Hartmut F.-W. Sadrozinski, US ATLAS Upgrade Meeting Nov 10, (is n-type MCz inverted?) SMART News: Annealing behaviour of n- type MCz Si A.Macchiolo et al. Submitted to NIM A, presented at PSD 7, Liverpool, Sept M. Scaringella et al. presented at Large Scale Applications and Radiation Hardness Florence, Oct N-type

Hartmut F.-W. Sadrozinski, US ATLAS Upgrade Meeting Nov 10,  m pitch Inter-strip Capacitance One of the most important sensor parameters contributing to the S/N ratio Depends on the width/pitch ratio of the strips and on the strip isolation technique (p-stops, p-spray). Observe large bias dependence on p-type detectors, due to accumulation layer. 100  m pitch SMART 14-5 p-type FZ low-dose spray w/p = 15/50 V dep = 85 V (I. Henderson, J. Wray, D. Larson, SCIPP) Cint = 1.5 pF/cm Irradiation with 60 Co reduces the bias dependence, as expected.

Hartmut F.-W. Sadrozinski, US ATLAS Upgrade Meeting Nov 10,  Radiation hard materials for tracker detectors at SuperLHC are under study by the CERN RD50 collaboration. Fluence range to be covered with optimised S/N is in the range cm -2. At fluences up to cm -2 (Mid and Outer layers of a SLHC detector) the change of the depletion voltage and the large area to be covered by detectors is the major problem.  High resistivity MCz n-type and p-type Si are most promising materials.  Quite encouragingly, at higher fluences results seem better than first extrapolated from lower fluence: longer trapping times ( p-FZ, p-DOFZ) delayed and reduced reverse annealing ( MCz SMART) sublinear growth of the V dep with fluence ( p - MCz&FZ) delayed/supressed type inversion ( p- MCZ&FZ, MCz n- protons)  The annealing behavior in both n- and p-type SSD needs to be verified with CCE measurements. Status

Hartmut F.-W. Sadrozinski, US ATLAS Upgrade Meeting Nov 10, R&D Plan: - Need to confirm findings of C-V measurements - Fabricate SSD on MCz wafers, both p- and n-type. - Optimize isolation on n-side. - Measure charge collection efficiency (CCE) on SSD, pre-rad, post-rad, during anneal. - Measure noise on SSD pre-rad, post-rad, during anneal. Un-irradiated SMART SSD

Hartmut F.-W. Sadrozinski, US ATLAS Upgrade Meeting Nov 10, R&D Plan Submission of 6” fabrication run within RD50 Goals: -a. P-type isolation study -b. Geometry dependence -c. Charge collection studies -d. Noise studies -e. System studies: cooling, high bias voltage operation, -f. Different materials (MCz, FZ, DOFZ) -g. Thickness