ALCPG2005, Aug. 27, 2005 SiD Summary H.Weerts For the SiD Design Concept Study.

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ALCPG2005, Aug. 27, 2005 SiD Summary H.Weerts For the SiD Design Concept Study

ALCPG2005, Aug. 27, 2005 Introduction Victoria 2004  Snowmass 2005 Original concept for SiD from M.Breidenbach and J.Brau (2003) Start of ILC detector concepts by WWS at ALCPG04, Victoria First SiD kick-off meeting with interested parties Critical SiD Questions document (still valid) Kick off meetings at ECFA & ACFA meetings Fall ‘04 Over the last year we have had many phone meetings which were all more or less driven by subgroups. Had one afternoon meeting at LCWS05 Snowmass 2005 is first occasion for people interested to participate in SiD to actually spend some time together and work on SiD. This was an important step for SiD and this may be the first in a series of SiD design study meetings

ALCPG2005, Aug. 27, 2005 SiD Organization EXECUTIVE COMMITTEE H.Aihara, J.Brau, M.Breidenbach, J.Jaros, J.Karyotakis, H.Weerts & A.White SOLENOID FLUX RET R.Smith -- VERY FORWARD -- SIMULATION N.Graf -- MDI P.Burrows T.Tauchi -- VERTEXING Su Dong -- CALORIMETERS R.Frey J.Repond -- MUON H.Band H.E.Fisk -- BENCHMARKING T.Barklow -- COST M.Breidenbach -- R& D COORDINATOR A. White ADVISORY COMMITTEE All names on this chart Put SiD organization in place in Fall & Winter ’04/’05; form subgroups and start work in those: simulation, CAL/PFA, tracker layout & design starting quickly. Followed by: solenoid feasibility, vertex, benchmarking and others later.

ALCPG2005, Aug. 27, 2005 Coming to Snowmass Critical area for all development & progress in SiD with a lot of development and work done is simulation. SiD now has a simulation of the detector “starting point” First version: SIDMAY05 and now the latest SIDAUG05 Description can be found at: howAttachments=true#attachments This starting point is called: SiD 00 Most of the simulations done at this workshop were based on SiD 00 and it will be referred to as SiDMAY05/SiDAUG05 Thanks to simulation group for making this possible

ALCPG2005, Aug. 27, 2005 SiD Concept Design Study Goals  Design a comprehensive LC detector, aggressive in performance but constrained in cost.  Optimize the integrated physics performance of its subsystems.  Evolve the present starting point of SiD towards a more complete and optimized design.  Interest the international HEP community in the experimental challenges of a LC. u a) Two-jet mass resolution comparable to the natural widths of W and Z for an unambiguous identification of the final states. u b) Excellent flavor-tagging efficiency and purity (for both b- and c-quarks, and hopefully also for s-quarks). u c) Momentum resolution capable of reconstructing the recoil-mass to di-muons in Higgs-strahlung with resolution better than beam-energy spread. u d) Hermeticity (both crack-less and coverage to very forward angles) to precisely determine the missing momentum. u e) Timing resolution capable of tagging bunch-crossings to suppress backgrounds in calorimeter and tracker. u f) Very forward calorimetry that resolves each bunch in the train for veto capability. Standard Physics requirements

ALCPG2005, Aug. 27, 2005 Detector outline considerations Architecture arguments  Calorimeter (and tracker) Silicon is expensive, so limit area by limiting radius (and length)  Maintain BR 2 by pushing B (~5T)  Excellent tracking resolution by using silicon strips  5T field allows minimum VXD radius.  Do track finding by using 5 VXD space points to determine track – tracker measures sagitta. Exploit tracking capability of EMCAL for V’s.  Accept the notion that excellent energy flow calorimetry is required, use W-Si for EMCAL and the implications for the detector architecture… This is the monster assumption of SiD (MB quote)

ALCPG2005, Aug. 27, 2005 Detector outline A high performance detector for the LC Uncompromised performance BUT Constrained & Rational cost This is simulated SiD 00

ALCPG2005, Aug. 27, 2005 Plans for Snowmass General theme: simulation and study of the baseline detector and possibly variations of that baseline, but this is rather group dependent In following summarize ( incomplete !!) some of the work done in SiD subsystems and working groups. Start with detector subsystems at smallest radius. NOTE: An integrated detector design for ILC depends critically on the Particle Flow Algorithm (PFA), which is used to measure jet energies and uses all parts of the detector. It dominates most activities, but I will cover it under calorimetry.

ALCPG2005, Aug. 27, 2005 Vertexing= VXD 5 barrel layers 4 end disks SiD 00 Work on mechanical layout of VXD Z= 6.25cm 5T Design drivers: Smallest radius possible Clear pair background Seed tracks & vertexing Improve forward region Role: Z [cm] R [cm]

ALCPG2005, Aug. 27, 2005 Vertexing Concept of VXD support (started at Snowmass) Issues considering: Thickness and mechanical design of endplate & support Sensor technology ( several being pursued; common among all concepts; more in summary) Increase # layers by 1 in barrel & endcap

ALCPG2005, Aug. 27, 2005 Tracking I SID 00 Cylinders tiled with 10x10cm sensors with readout chip Single sided (  ) in barrel R,  in disks Modules mainly silicon with minimal support (0.8% X 0 ) Overlap in phi and z Closed CF/Rohacell cylinders Nested support via annular rings Power/readout motherboard mounted on support rings

ALCPG2005, Aug. 27, 2005 Tracking II SDAUG05: 5T, R=125cm SD PETITE: 5T, R=100cm LOW FIELD: 4T, R=125cm At 90 o Obtained momentum resolution 0.5% Excellent momentum resolution

ALCPG2005, Aug. 27, 2005 Tracking III March ’05 concept of open tracker; allow access to VXD Snowmass update

ALCPG2005, Aug. 27, 2005 Tracking IV; examples of work done Tracking in from EMCAL for V’s Many other studies; see summaries on SiD concept page VXD seeded tracking efficiency for 5 and 8 layer tracker as function of angle from Thrust axis. 500GeV Use other track seeding for “missing” fraction ( outside –in)

ALCPG2005, Aug. 27, 2005 SiD Calorimetry  We would like a detector which can examine new physics processes in such detail...  Use it to obtain excellent jet energy resolution (through PFA).

ALCPG2005, Aug. 27, 2005 EMCAL Si/W pixel size: prototypes are 16 mm 2 readout chip: designed for 12 mm 2 How small can we go?? 2-4 mm 2 ? Need a physics argument for smaller pixels.  ->  +  o

ALCPG2005, Aug. 27, 2005 Distance in cm Fraction 1.5 x the pad size Fraction of the photon(s) energy per event, closer to a charged track than some distance J.-C. Brient

ALCPG2005, Aug. 27, 2005 Hadron Calorimetry Considering several options for HCal: SS or Tungsten with any one of 3 readout technologies ScintillatorGEMsRPCs TechnologyProven (SiPM?)Relatively newRelatively old Electronic readoutAnalog (multi-bit) or Semi-digital (few-bit) Digital (single-bit) Thickness (total)~ 8mm Segmentation3 x 3 cm 2 1 x 1 cm 2 Pad multiplicity for MIPsSmall cross talkMeasured at 1.27Measured at 1.6 Sensitivity to neutrons (low energy) YesNegligible Recharging timeFastFast?Slow (20 ms/cm 2 ) ReliabilityProvenSensitiveProven (glass) CalibrationChallengeDepends on efficiencyNot a concern (high efficiency) AssemblyLabor intensiveRelatively straight forward Simple CostNot cheap (SiPM?)Expensive foilsCheap

ALCPG2005, Aug. 27, 2005 Calorimetry II: PFA’s applied to SiD 00 A. Respereza S. Magill Note: Z→u,d,s Area of intense work in SiD

ALCPG2005, Aug. 27, 2005 PFA activities MST clustering and fragments associationM. Charles, Iowa density-weighted clusteringLei Xia, ANL density-weighted clusteringV. Zutshi, G. Lima, NIU Neural-net based id – 15 discriminators – based on Bower, Cassel, Pathek NN S. Kuhlmann, S. Magill, ANL hadrons: Full PFA’s under development for SiD: ANL, SLAC – Magill, Graf, Cassell, Kuhlmann H-matrix, track extrapolation, and nearest n’bor had. clust. ANL – Lei Xia – cluster based NIU – Chakraborty, Lima, Zutshi – cluster based MST clustering (follow up with H-matrix id?)N. Meyer, Iowa H-matrix id developmentN. Graf, SLAC H-matrix id (preceded by n-n’bor clustering) Photon sep  pi0 kinematic fit  improved res. ! G. Wilson, E. Benavidez, Kansas H-matrix based idS. Kuhlmann, S. Magill, ANL Photons:

ALCPG2005, Aug. 27, 2005 Solenoid Did feasibility study and convinced ourselves & others that this 5T solenoid can be built, based on CMS design & conductor. Inner radius: ~ 2.5m to ~3.32m, L=5.4m; Stored energy ~ 1.2 GJ Stresses and forces comparable to CMS. SiD coil  Same conductor as CMS  CMS (4 layer)  SiD (6 layer)  CMS 5 modules 2.5 m long  SiD 2 modules 2.6 m long

ALCPG2005, Aug. 27, 2005 Solenoid next steps Provides field maps for SiD and for MDI questions Design of Detector-Integrated-Dipole (DID) for beam X-angle 9 20mrad) 0.15 m 0.02 m Inner radius of dipole coils is 1 cm greater than support cylinder radius NI per dipole coil = A-t Wrap saddle coils on support cylinder Provides required field Forces are manageable Developing parametric cost model based on CMS cost; solenoid is cost driver

ALCPG2005, Aug. 27, 2005 Muon system Muon group just started at this workshop.  Glass & Bakelite RPCs –  Scintillator and Photo-detectors  GEMs  Wire Chambers Strips vs. pixels SiD Muon System Strawman  24 10cm plates w/23 gaps. Muon ID studies done to date with 12 instrumented gaps. ~1cm spatial resolution? Start with 12 planes, more when needed (e.g. 1TeV).  6-8 planes of x,y, u or v upstream of Fe flux return for xyz and direction of charged particles that enter muon system.  Detector Technologies  Is the muon system needed as a tail catcher?  How many layers are needed (0-23)? Use HCAL ?  Position resolution needed? Questions

ALCPG2005, Aug. 27, 2005 MDI  18 ‘urgent’ questions issued by WWS/MDI to 3 detector concepts  Written responses provided pre-Snowmass  Responses digested and summarised by WG4/MDI  L* range under discussion by WG4: 3.5m < L* < 4.5m Range is acceptable to SiD  Beampipe radius: effectively discussing 15 < r < 25 mm if backgrounds allows: SiD prefers smallest r  Bunch spacing: ns acceptable to SiD Excellent liaisons to MDIpanel/WG4: P.Burrows & T.Tauchi Most of the work done in WG4, but need interaction WG4 – SiD: Need to specify tolerable background rates Refine answers to questions MDI questions

ALCPG2005, Aug. 27, 2005 Benchmarking Recoil Mass (GeV)

ALCPG2005, Aug. 27, 2005 Cost Much more on cost in separate talk by Marty Breidenbach Cost by subsystem Cost minimum vs. tracker radius

ALCPG2005, Aug. 27, 2005 SiD: salient features Smallest L*, compatible with crossing-angle reach VXD: smallest radius ( 5T helps) Tracker: excellent  p/p; silicon robust; minimize material uniformly over cos(  ); demonstrated pattern recog ( in  out; out  in, stand alone ECAL: excellent segmentation 4x4 mm, R Moliere =13mm HCAL: excellent segmentation Calorimetry: imaging, hermetic Solenoid: feasible, 5T Instrumented flux return & imaging HCAL: excellent muon ID Time stamp/digitize bunch by bunch Cost: constrain cost, have a parametric model

ALCPG2005, Aug. 27, 2005 R&D needs & priorities Concepts have been asked to identify and prioritize their R&D needs. Draft of R&D report submitted: SiD Detector Concept for the International Linear Collider Research and Development Report for WWS R&D Panel Introduction The SiD design concept is continuously evolving. R&D on most detector subsystems has started, but generally with rather limited funding. For the purposes of providing information on the status and needs of R&D, this report therefore takes two approaches: (1) We give a “top-down” estimate (separate file) based on the overall best estimate of the final SiD detector cost, by subsystem, and experienced-based estimates of the R&D as a percentage of final cost. This also involves risk assessment for each subsystem in terms of a contingency for the R&D. (2)(below) We give a detailed list of the present SiD R&D projects as far as is known and their present/anticipated funding. Clearly there is a large gap in the figures for each subsystem deriving from the two approaches. However, we take this information to be input to the WWS R&D Panel and future deliberations, starting at Snowmass Vertex Detector (Su Dong) Top Down approach: R&D needs of subsystems: SiD SubsystemCost Estimated R&D %R&D CostR&DR&D Cost Contingency % With Contingency VXD Tracker EMCal HCal Muon system Electronics Magnet MDI TOTALS/AVG Next Step: Prioritize R&D needs of SiD; started at Snowmass

ALCPG2005, Aug. 27, 2005 Looking towards near future Evolve SiD 00 towards a baseline: explore variations of current starting point: B, R tracker, barrel length plus others and optimize using some benchmarks. Need PFA with sufficient accuracy and sensitivity to do this. These steps needed to be able to produce a draft a detector outline document by LCWS06 (DD= detector document) Plan a SiD meeting (few days) middle of december

ALCPG2005, Aug. 27, 2005 SiD socially & outside dark rooms SiD at Crater Lake

ALCPG2005, Aug. 27, 2005 Conclusion of Snowmass 2005 First time for SiD concept study participants to get together in person and for more then a few hours. Establish working relationships which are very positive and necessary to complete the work ahead of us in the next few months and longer future. Excellent progress made on understanding and simulating SiD 00 starting point. We have put SiD on a more solid foundation. Thanks to all who contributed to the progress on SiD Only a small fraction of the work done by my colleagues was described in this summary. SID summaries yesterday took 4 hours ! THANK YOU to organizers (and others) for making this workshop happen and allowing SiD to take a giant step forward

ALCPG2005, Aug. 27, 2005 THE END

ALCPG2005, Aug. 27, 2005 VXD backup SiD ILC 500 Nominal VXD Background rates N Q Y P H 500 GeV 1 TeV R= Takashi Maruyama Large rate difference between Layer 1 and outer layers Needs at least x2 margin from nominal configuration These are for pair background only. What about synchrotron radiation ?

ALCPG2005, Aug. 27, 2005 Benchmarking SiD Detector Resolution p=20 GeV, SIMDET LDC p=20 GeV p=3 GeV p=100 GeV A comparison of momentum resolution vs. angle in simulations: Fast MC Using SID 00

ALCPG2005, Aug. 27, 2005 Tracking II/backup