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ATLAS ID Upgrade

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1. D. Lissauer, BNL. ATLAS ID Upgrade. Scope R&D Plans for ... Cryogenics detectors. Middle and Outer Radius: 2D Single sided detectors 'Macro pixel Detectors' ... – PowerPoint PPT presentation

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Title: ATLAS ID Upgrade


1
ATLAS ID Upgrade
  • Scope RD Plans for ATLAS Tracker
  • First thoughts on Schedule and Cost

2
Detectors General Considerations
3
Inner Tracking
  • Assumption is that the inner tracker will need to
    be re-built using higher granularity detectors in
    a harder radiation environment in order to
    preserve the current pattern recognition,
    momentum resolution, b-tagging capability.
  • a Radiation increase by 10.
  • a To keep Occupancy constant granularity has to
    increase by a factor 10.
  • Small Radius Region Vertex detector (r lt 20cm)
  • aim for a pixels size factor 5-8 smaller than
    today
  • (50x400 mm2 g 50 x 50 mm2) g benefit
    b-tagging, t-tagging
  • RD
  • Pixels Sensor Technologies
  • Super rad-hard electronics to achieve small
    pixel size

4
Inner Tracking
  • Intermediate Radius 20ltrlt60 cm
  • Aim for cell sizes 10 times smaller than
    conventional Si strip
  • detectors.
  • benefit momentum-resolution and pattern
    recognition
  • RD
  • Lower cost/channel compared to present Si strip
    detectors
  • Si macro-pixels of an area 1mm2 pads or
    shorter strips ?
  • Single sided two dimensional readout (new
    concepts)
  • Large Radius 60ltr
  • Large area Si detectors.
  • Could use present day radiation resistant
    strip technology,
  • or new single sided technology
  • RD
  • Similar to intermediate radius less demanding
    except for cost.

5
Inner Tracking
Engineering/Integration Aim at a factor of 10
more channels but with less material. This means
that the System aspects have to be integrated and
understood from the start. RD new light
weight materials for stable structures. Power
Power distribution. Multiplexing of
readout. cooling. alignment. installation and
maintenance aspects. (replacement of existing
infrastructure) Activation 250 mSv/h
implications for access and maintenance Timescale
Need 8-10 years from launch of RD
4-6 years of RD and prototyping , 4 years to
build,
6
RD Scope
  • Simulation Detector geometry, readout
    granularity.
  • Support Structure Integrated Support of the ID,
    Mass less.
  • Cooling Thermal management of the system.
  • Si Detector Technology, Contact with industry.
  • Readout Technology,Power, Connections.
  • Module Layout Technology, Integration at the
    module level.
  • System InfrastructureCabling, Multiplexing,
  • Optical Links Power consideration,multiplexing,
    Rad hard.
  • 9. Power Supplies Location, distribution,
    Cabling.
  • Radiation Hardness Radiation hardness of ALL
    components.
  • 11. Assembly/InstallationAssembly and
    installation above ground and in pitt.
  • 12. System Tests Validation of the performance
    at the system level.

7
Simulation
  • Tracker configuration Overall optimization of
    the tracker. Number of layers in the inner ,
    middle and outer radius.
  • Sensor geometry For each layer determine the
    detector granularity, readout
    geometry.
  • Optimal readout Analog.vs. digital, speed of the
    readout.
  • Data Compression Study possible data compression
    schemes.

8
Space Boundary Conditions
  •    Simulation
  • detector geometry, readout granularity

TRT
SCT
Pixel
9
2. Support Structure
  • Conceptual design
  • beam pipe support
  • Vertex detector support
  • Intermediate Si tracker support
  • Outer Layer Support
  • Assembly
  • Technology
  • Materials
  • Optimal Configuration
  • Assembly
  • FEA Calculations
  • Services/Cooling interface
  • Integration of the Support structure and the
    services/cooling.
  • Interface to the Thermal Shield.
  •              

10
3. Thermal Management
  • Conceptual Design
  • Cooling capacity
  • Cooling method
  • Evaporative Cooling
  • Binary ICE
  • Operating temperature
  • Pixels and SCT run at 70C
  • Thermal enclosures
  • Heat Shields and thermal divisions
  • Cooling Control
  • Prototype Cooling System

11
4. Si Detector - I
  • Issues
  • Cost Detector /Readout
  • Connectivity
  • Radiation hardness
  • Optimal temperature operation
  • Detector Technology
  • Inner Radius Candidate Technologies
  • 3D readout
  • Integrated readout and Pixel in one wafer
  • Cryogenics detectors
  • Middle and Outer Radius
  • 2D Single sided detectors
  • Macro pixel Detectors
  • Si Strips
  • Wafer Size
  • Wafer Size aim to go to higher Wafers to reduce
    cost as well as number of detectors. Presently 6
    are used should be able to go to 8 and possibly
    12.          

12
5. Readout
  • Issues
  • Multiplexing
  • Technology
  • ATLAS SCT readout used the DMILL process will
    not be available to upgrade
  • PIXEL has used IBM deep sub-micron need to
    investigate the limit of the radiation hardness
    of this process.
  • New readout chip development
  • Tools
  •          

13
6. Module Layout - I
  • Issues
  • Module layout and interface to readout
    electronics.
  • Interface to services.
  • Production Cost.
  • Industrial Solution vs. Assembly at inst.
  • Technology
  •      
  •     

14
7. Cabling/ Multiplexing/ Grounding.
  • Issues
  • Cable routing.
  • Multiplexing.
  • Production Cost.
  • Industrial Solution.
  •            

15
8. Optical Links
  • Issues
  • Development of new fast optical Links Power.
  • New technology Industrial solution.
  • Production Cost.
  •          

16
9. Power Supplies
  • Issues
  • Location of power supplies.
  • Optimal Multiplexing of power and implication on
    Noise, Cable, cost etc.
  • New readout technology moves toward low voltage,
    implication is that we will need very large
    currents unless we can Ladder the power.
  •             

17
10. Radiation Hardness
  • Issues
  • Testing of all components to new levels.
  •        

18
11. Assembly /Installation
  • Issues
  • Replacing present ID with new one while the
    rest of the experiment stay in tact more or less.
  • E.g Cable routing when the Muon chambers are in
    place? Do we need to remove BIL, BIS Chambers?
  • Max amount of cables services we can route?
  •           

19
12. System Tests
  • Issues
  • Ideas on multiplexing, power dist. Etc. all need
    to be confirm in a realistic condition.
  • Cooling systems need to be tested and developed.
  • Combine test of the whole system needs to be done
    to validate both the concept and the system
    aspects.
  • ATLAS was (is) very weak on this point.
  •           

20
Tracker Upgrade Schedule
  • ATLAS will start running in 07 and for the first
    5 years will operate with the present ID.
  • After 5 years the LHC Luminosity will be
    upgraded and a new and improved ID will be
    needed.
  • Even if there is no Luminosity upgrade we expect
    that the ID will need to be upgraded.
  • The time scale is
  • Formal proposal 04
  • Identify Collaborators in the US and outside.
  • RD directed Generic 04-09
  • Proposal for ATLAS Upgrade 09-10
  • Production of New ID Tracker 10-13
  • Installation of new ID Tracker 14

21
Tracking Cost estimate
  • The estimate is very preliminary and is based on
    the following assumptions The active components
    of the tracker are all Si. The inner radius has
    upgraded Si Pixel detectors, followed by Si Strip
    detectors, in the outer radius we use single
    sided 2-D Si detectors.
  • The estimate was done by scaling the cost of the
    ATLAS Si detector as well as information from
    CMS, and the CDF/D0 upgrade cost.
  • In scaling the costs we had to make assumptions
    on how the main cost drivers will scale with the
    number of channels, the area and the expected
    time evolution.
  • The RD and final design will have to be driven
    by optimizing the cost to performance of the
    overall system.

22
Tracking Cost estimate
  • Mechanics The mechanics does not scale with the
    number of channels.
  • One has to keep the services and the total
    weight to a minimum.
  • The cost estimate assumes there is added
    complexity due to light weight
  • Si Detectors Scale with the detector area.
  • The optimization of the number of layers and
    exact location has not been finalized. The total
    amount of Si will be factor of 5-10 greater
    than the present ATLAS detector.
  • Possible cost reduction
  • Si detectors Cost is driven largely by wafer
    size. Industry is moving toward larger wafers.
  • Minimize the the amount of Si by using
    advances in detector technology. For example
    single sided 2D readout can be used in the
    medium and larger radii where the segmentation
    needs are dominated by tracking accuracy rather
    than occupancy.

23
Tracking Cost estimate
  • On detector read out electronics
  • The readout electronics cost is driven by the
    number of channels.
  • Take advantage of the reduction in the feature
    size of the electronics. (ATLAS design used
    ATMEL/DMILL rad hard technology that has a
    conservative feature size of 1.2 Micron in the
    Strips. CMS and ATLAS pixels are using sub micron
    technology of 0.25 micron)
  • Present industry standard is 0.18 moving
    toward 0.13 microns.
  • Expect that by the time we go into production
    the standard feature size will be as low as 0.08
    microns. Allowing for a substantial reduction in
    the power and space needed for the electronics
    and allowing for finer granularity without an
    increase in power and space needed.
  • The reduction in power has important
    implication also on the cooling and services that
    will be needed.

24
Tracking Cost estimate
  • Module integration
  • Module integration costs include costs of
    Hybrids and the components assembly.
  • In the case of the Pixel detectors the cost of
    bump bonding Si is a significant part of the
    module integration.
  • Significant cost reductions are possible
    assuming one of the integrated developments
    matures in time. They integrate the readout and
    the active detector on the same wafer
    eliminating the need for individual bonds.
  • Cables Data Links
  • Assumed a higher level of multiplexing compared
    to the present solutions. In particular the
    amount of power cables that need to be reduced
    for physics (reduced mass), space and cost
    reasons.
  • Power Supplies
  • Power supplies will need to be optimized and
    serve a larger number of modules. This has
    implication on coherent noise and very detailed
    system integration will be needed to achieve
    this.

25
Tracking Cost estimate
  • Cooling (Additional) The needed cooling capacity
    will scale with the number of channels, but we
    have taken advantage of the lower power
    requirements of the lower feature size
    electronics. A large part of the external cooling
    can be reused.
  • Off detector electronics (Read out Drivers) We
    have to take advantage of advances and reduction
    in the cost of electronics. We assume that a
    factor of 10 more data 10 years from now will
    cost factor of 1.5 more than present cost.
  • The Tracker cost for one detector thus estimated
    to be between
  • 150-180 M. (assuming the full detector is built
    in the US)
  • These numbers are only given as a rough
    estimate. We are not ready for an engineering
    estimate, which will have to be done after RD
    has progressed and better optimization done.
  • What should be the US part?

26
Conclusions
  • Tracker Upgrade is a complex technical problem.
  • The RD plan needs significant effort in many
    areas.
  • An ATLAS wide collaboration will need to be
    established for the execution of the project.
  • U.S. should plan a significant role in the ATLAS
    Tracker upgrade.
  • With ATLAS detector still not completed and
    installed. Preparations for Physics on going we
    need to find the right balance for this effort.

27
ATLAS
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