Velo Upgrade for high luminosity operation Marina Artuso Syracuse University Requirements Technology choices R&D Issues Cost and timeline 1/12/2007 Marina Artuso LHCb High Luminosity Upgrade Workshop 1 LHCb Upgrade Goals Upgrade LHCb detector such that it can operate at 10 times design luminosity of ℒ ~ 2 x1033 cm-2s-1 z Upgrade LHCb detector to maximize sensitivity to many interesting hadronic channels z Vertex trigger z Optimization of photon detection z 1/12/2007 Marina Artuso LHCb High Luminosity Upgrade Workshop 2 Impact on vertex detector upgrade requirements Radiation resistance (>1015 1 MeV neutroneq /cm2 ) z Fast and robust pattern recognition capabilities ⇒ detached vertex criteria at the lowest trigger level (L0 Vertex Trigger) z Optimization of impact parameter resolution z Reduce detector inner radius z RF foil modifications z z 1/12/2007 Material minimization for chosen solution Marina Artuso LHCb High Luminosity Upgrade Workshop 3 Additional considerations z Resources for this detector need to be identified z The chosen solution must be technically achievable in the time scale envisaged for the project (∼2013): Coordinated R&D effort should start now z R&D must demonstrate capabilities for large scale production in a ∼3 years time span z 1/12/2007 Marina Artuso LHCb High Luminosity Upgrade Workshop 4 Velo now See T. Bowcock’s talk z rφ strip detector with variable pitch: z z 1/12/2007 tradeoff between number of channels and resolution Quick rz tracking for triggering purposes Marina Artuso LHCb High Luminosity Upgrade Workshop VELO Module Length determined by angular acceptance and minimum radius requirement “spare” system very close in design to present system is planned and is not the upgrade discussed in this talk 5 towards a LHCb Pixel Telescope 4 cm 2 cm 5 cm 10 cm 1.2 cm Beam 5 cm •Need to identify optimum geometry: •Parametric study of telescope configuration (number of stations, cell size…) as a function of rmin •Detailed study of vertex reconstruction algorithm with full simulation 1/12/2007 Marina Artuso LHCb High Luminosity Upgrade Workshop 6 Why pixel? z thinned 8cm Z Beam 1/12/2007 Measurement of 3D space points, with very few additional noise hits, implies excellent pattern recognition capabilies: z Vertex reconstruction in “real time” feasible (see E. Gottshalk talk) •Optimal radiation resistance (⇒inner detector in all LHC devices): •Allows operation with smaller rmin & higher luminosity without replacement for the duration of the experiment •Low noise (∼200 e- @ 25 ns) allows more precise charge interpolation & (in principle) thinner detectors. Marina Artuso LHCb High Luminosity Upgrade Workshop 7 The pixel module z Design choices: z z z 1/12/2007 Sensor-front end electronics High density hybrid Mechanical support/cooling Marina Artuso LHCb High Luminosity Upgrade Workshop 8 Hybrid pixel devices sensor module z Fully engineered solution (ATLAS, CMS, BTeV) z Allows separate R&D on sensor and electronics z Material needs to be minimized (sensor-electronic thinning-RF-overall system design) bump bonds wire bonds readout chips high density interconnect TPG substrate BTeV plane 0.22 0.12 1.11 1/12/2007 9 Well understood technology z z z z Predictions from Monte Carlo simulation validated in extensive test beam studies Sensor design well established (Atlas, BTeV) Lots of experience in system issues during CMS/ATLAS commissioning Front end design mature (see D. Christian’s talk) 1/12/2007 Marina Artuso LHCb High Luminosity Upgrade Workshop MC simulation BTeV pixel TB 1999 10 Material minimization: wafer thinning z z 1/12/2007 BTeV/CMS R&D achieved 200 μm backthinning of bump bonded electronics (target thickness) & FPIX2 dies have been thinned down to 150 μm (1 step) & 130 μm (2 steps) We can capitalize on advances in thinning silicon wafer, hybrid silicon wafer assemblies Marina Artuso LHCb High Luminosity Upgrade Workshop 11 R&D activities - sensors z Sensor-electronics technology: z Monolithic Pixel Devices (Liverpool) z z z z Monolithic CMOS Active Pixel devices Silicon on Insulator 3D sensors (Glasgow) Substrate material to ensure maximum radiation resistance (in collaboration with RD50): z z z 1/12/2007 p-type substrates (Liverpool, Syracuse) Magnetic Czochralski (Glasgow) Others…. Marina Artuso LHCb High Luminosity Upgrade Workshop 12 Monolithic Pixel Devices z Advantages: z Easier to reduce module material z Eliminate one interconnection step: bump bonding of sensor and electronics z In general, no separate development path for sensor and electronics z No large scale production experience RALLiverpool prototype wafer 1/12/2007 Front end electronics Sensor: epitaxial layer (Variation: silicon on insulator 13 3d silicon sensors z Combine VLSI processing and MEMs (Micro Electro Mechanical System) technology z Variant of the sensor implementation in hybrid pixel systems z Advantages: z Very low depletion voltage z Very low capacitance z The edge is an electrode: dead volume near the edge < 5μm 1/12/2007 Marina Artuso LHCb High Luminosity Upgrade Workshop 14 Radiation hard technologies z charge collection efficiency as detector lifetime predictor Liverpool GlasgowCERN Czochralski 1/12/2007 n-on-p Marina Artuso LHCb High Luminosity Upgrade Workshop 15 Front-end electronics z Must provide digitized data to trigger processor in real time: Time stamping z On chip sparsification z On chip digitization z Ideal option: adapt fully engineered solution to our application z New smaller feature size technologies may allow smaller “long pixel dimension” z FPIX2 1/12/2007 Marina Artuso LHCb High Luminosity Upgrade Workshop 16 R&D activities – front end electronics z Optimization of the front-end device: noise, speed, power. z Choice of optimal data flow architecture z Technology: proved radiation hardness, must be available throughout the duration of the project, development and production cost. z Much more on D. Christian’s talk 1/12/2007 Marina Artuso LHCb High Luminosity Upgrade Workshop 17 Signal connections From R. Yarema Vertex2005 1/12/2007 Marina Artuso LHCb High Luminosity Upgrade Workshop 18 The vacuum tank z Critical issue: can we reduce the material in front of the first measuring point? z z A drastic solution: vertex detector in the machine vacuum. Issues: z z z z 1/12/2007 Is it feasible? Is it allowed? Necessary to fully understand outgassing properties of each material used in the pixel module, redundancy and safety margin in vacuum components, effect of beam image currents (beam simulator) The prize is well worth the R&D effort Marina Artuso LHCb High Luminosity Upgrade Workshop 19 Summary of R&D needed z Physics case + geometry optimization simulation work (23FTE): define geometry and prioritize choices among various R&D options described: z z z z z 1/12/2007 rad hard sensors Data driven front-end electronics interconnection technologies mechanical issues Synergistic interactions with R&D effort with similar goals z Sensor RD50 (already in progress: Glasgow, Liverpool, Syracuse) z Submicron technology, other implementations of data push architecture (Syracuse-Fermilab) z Other SLHC upgrade efforts Marina Artuso LHCb High Luminosity Upgrade Workshop 20 Construction cost & manpower projection (assuming a pixel telescope) Material cost FTE Sensor Hybridization (sensors, bump bonding…) 2.1M$ 9 Front electronics 1.0M$ 7 Services (LV/HV/Cables) 1.7M$ 5 Mechanics, cooling and vacuum 1.6M$ 25 Integration and testing 0.8M$ 57 total 7.2M$ 1/12/2007 Marina Artuso LHCb High Luminosity Upgrade Workshop <FTE>=26 over 5 years, ramping up Projected construction time 4-5 years (depending upon time contingency assumed) 21 Conclusions z z z z A vertex detector suitable for a fast L0 vertex trigger is critical to achieve the goals of an LHCb upgrade. A pixel technology with self triggering readout electronics is an important element of such a system. Additional R&D items include low mass and reliable interconnections and mechanical system aspects such as vacuum design, RF shielding … Construction expected to last 4-5 years based on experience on similar projects: R&D should start soon to achieve desired timeline 1/12/2007 Marina Artuso LHCb High Luminosity Upgrade Workshop 22