HFT Project Overview
CD0 Review
H.G. RitterLBNL
HFT CD0 Review, February 25 and 26, 2008 2
Project
• In the first part we have shown– Compelling science– Proposed detector can do necessary
measurements• In the second part we will show
– Properties of detector– How we build it– We have the team and the organization
to build it
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OverviewSTAR Tracking Upgrade to identify mid-rapidity Charm and Bottom hadrons through direct reconstruction and measurement of the displaced vertex
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HFT Project
• Time line:– February 2008 (CD-0) – June 2013
(CD-4)• Budget
– Previous (proposal):$15.1M-16M– Present estimated cost range:
$11.1M-14.7M•Updates to Design•Contingency
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PIXEL
• 2 layers of 30x30 m pixels at 2.5 and 8 cm radius
• Very low material budget to limit multiple scattering
• Rapid insertion and removal• Precision positioning• Air cooling • Data reduction and formatting on
chip
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PIXEL
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Engineering Prototype
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IST
• One layer of single sided silicon pads at a radius of 14 cm
• ~23 ladders• 11 units
(modules) per ladder
• Conventional and proven technology
• MIT expertise
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Optimal technology
• Pixel: New technology– Resolution– Low material budget
• IST: Proven strip-pad technology– Experience– Cost effective
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SSD• Existing detector• Needs upgrade to cope with DAQ1000
– (order of 350k$)
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Collaboration
• BNL: C. Chasman, D. Beavis, R. Debbe, J.H. Lee, M.J. Levine, F. Videbaek, Z. Xu
• UCLA: R. Cendejas, H. Huang, S. Sakai, G. Wang, C. Whitten• Kent State: J. Joseph, D. Keane, S. Margetis, V. Rykov, W.M.
Zhang• Prague: M. Bystersky, J. Kapitan, V. Kushpil, M. Sumbera • Strasbourg: J. Baudot, C. Hu-Guo, A. Shabetai, M. Szelezniak,
M. Winter• MIT: J. Balewski, D. Hasell, J. Kelsey, R. Milner, M. Plesko, R.
Redwine, B. Surrow, G. Van Nieuwenhuizen• LBNL: E. Anderssen, X. Dong, L. Greiner, H.S. Matis, S.
Morgan, H.G. Ritter, A. Rose, E. Sichtermann, R.P. Singh, T. Stezelberger, X. Sun, J.H. Thomas, V. Tram, C. Vu, H.H. Wieman, N. Xu
• Purdue: A.S. Hirsch, X. Li, B. Srivastava, F. Wang, Q. Wang, W. Xie
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STAR - HFT Collaboration
• LBNL, MIT and BNL are main institutes for construction– Excellent track record– Experience
• Strasbourg/LBNL - active pixel sensor development
• Kent State, Purdue, Prague, UCLA, LBNL play lead role in simulation, analysis software and calibration
• Entire STAR collaboration will analyze data– Excellent track record– Experience
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Management Structure
HFT Project ManagementContract Project Manager: HG Ritter (acting) LBNLDeputy, Contract Project Manager: RP Singh LBNL
Deputy, Contract Project Manager: F. Videbaek BNL
PIXEL
Wieman LBNL
Anderssen LBNL
IST
B. Surrow MIT
J. Kelsey MIT
Integration
F. Videbaek BNL
J. Kelsey MIT
Software
S. Margetis KSU
SSD LiaisonJ. Thomas LBNL
Safety CoordinatorTBD
DOEJ. Simon-Gillo
Budget ControlS. Morgan LBNL
STARSpokesperson: T. HallmanUpgrade coord: R. Majka
BNLLBNL
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HFT Technical Committee
Ritter - Project ManagerSingh - Deputy Project ManagerMorgan - BudgetVidebaek - IntegrationWieman - PixelAnderssen - Pixel, IntegrationSurrow - ISTKelsey - IST, IntegrationThomas - SSD LiaisonMargetis - SoftwareHallman - STARMajka - STAR
Weekly meetings, management control
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Risk Management
• APS Sensors depending on Strasbourg pace of development– Early prototypes, involved in testing
and design• Kinematic mount, low mass ladder,
alignment challenging– Solve problem in the R+D phase
• SSD is essential– Involved in upgrade and running of
SSD, design redundancy into IST
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Performance Requirements
• Thickness of beam pipe + first Pixel layer < 0.5% radiation length
• Pixel integration time < 200 s• Read-out compatible with DAQ
1000• Internal alignment and stability
better than 20 m for Pixel and better than 300 m for IST
• Detector hit efficiency of Pixel > 95%
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Projected Run Plan
1) First run with HFT: 200 GeV Au+Au v2 and RCP with 500M M.B. collisions
2) Second run with HFT: 200 GeV p+p RAA
3) Third run with HFT: 200 GeV Au+Au Centrality dependence of v2 and RAA
Charm background and first attempt for electron pair measurements
C baryon with sufficient statistics
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Milestones
◊ CD-0 February 2008◊ CD-1 October 2008◊ CD-2/3 August 2009◊ CD-4 June 2013◊ Modified East Cone with West Cone in for Summer
’09 – June 2009◊ Installation of Engineering Prototype – September
2010◊ Engineering Prototype in Beam – January 2011◊ Ultimate Installed – September 2011◊ Ultimate In Beam – January 2012◊ IST Installed – July 2012
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Estimated Cost Range
WBS Task Name
Cost in $K
Cont. in %
Cont. in $K
Lower Range in $K (Est. TPC)
Upper Range in $K
1.1Research and Development
1,461 0 0 1,461 1,461
1.2 Pixel 1,985 46 1,125 3,110 4,354
1.3 Strip Detector 2,345 36 878 3,223 4,351
1.4 Integration 1,665 41 946 2,611 3,656
1.5 Software 0 0 0 0 0
1.6 Project Management 732 0 0 732 878
Total 8,188 29 2,949 11,138 14,701
Appropriate labor ratesEscalated Risk based contingency
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Summary• Compelling science for the RHIC II era• A detector
– That can deliver the science– Built on the strength of STAR
•Coverage and particle identification– Uses innovative technology to get
superior resolution • A team and an organization
– That can build the detector– That will extract the science in a timely
fashion• Meets the charges
Back-up
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Technology Driven Schedule