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Highresolution, fast and radiationhard silicon tracking station

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Both high resolution and a respectively low material budget are needed. D0K-p D0K-p ... High rate: 40 MHz / cm2. 100 ps time resolution. Fluence 4.5 1014 cm2 ... – PowerPoint PPT presentation

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Title: Highresolution, fast and radiationhard silicon tracking station


1
High-resolution, fast and radiation-hard silicon
tracking station
STS working group
  • CBM collaboration meeting March 2005

2
Status STS
  • Conceptual design (CDR)
  • First round of simulations (TSR)
  • ITS with 3 pixel planes
  • SIT with 4 equidistant planes, strip technology
    through out
  • Design iteration (partly in TSR)
  • Optimize configuration
  • Include HitProducers in simulation
  • Physics performance studies for different physics
    cases
  • Final design (TDP 2006?!)
  • Senors/FE chip, module, supportcooling, readout
  • Technological feasibility (RD)
  • Full performance simulation

3
Facts after 2nd round of simulations
Depends strongly on the physics case. Alternative
configurations for different observables possible.
Beam pipe of 1 cm Ø
First 3 stations (ITS) inside the vacuum!
Possibly shielded against good beam vacuum by a
foil.
Fluence above 1016
Is this the last word
?
Pixel
Strip
Only strip sensors for stations 4 to 7 (SIT) if
micro2 strips are used close to the beam!
4
Challenging tasks of the tracking station (I)
  • Micro vertex reconstruction (main task of the
    ITS)
  • Secondary vertex reconstruction better 50mm
    (z-coordinate)
  • Extremely high track density

D0?K-p
Both high resolution and a respectively low
material budget are needed.
5
D0?K-p
Material budget / plane
I. Vassiliev
6
Challenging tasks of the tracking station (II)
  • Background rejection in low mass dielectron
    spectroscopy
  • Reconstruction of "incomplete" tracks
  • Needs probably much more redundancy

7
d-electrons are a huge concern
  • Yield in 1st station 5/gold ion passing the (1)
    target
  • 5000 at frame rates of 10 ms and 109 ions/s !?

8
Possible configuration (B-TeV inspired)
  • Outer section of plane 3 outside the vacuum!
  • Highest granularity not needed there
  • Allows using thin vacuum window
  • Detectors can be moved in two halfs.
  • Remove sensors from beam area during focusing
  • Only two different module geometries
  • Optional for MAPS or Hybrids

9
Generic designs for simulation
  • MAPS-like
  • Radiation hardness
  • Read-out speed
  • Hybrid-like
  • Material budget
  • Resolution

10
MAPS material budget a first assessment by
Michael Deveaux
  • Stacking of sensors due to inactive read-out area
  • Design VELO (LHCb) inspired

0.29
11
MAPS RD
  • Dense program of chip submission in 2005
  • MIMOSA 9 ? factor 2 lower signal than expected
  • MIMOSA 10 ? MIMOSTAR1 first prototype for STAR
    IT
  • MIMOSA 11 ? Various sensor geometries for
    studying aspects of radiation tolerance
  • MIMOSA 12 ? Multiple charge storage
    on-pixel, aspects of capacitor performance
  • MIMOSA 13 ? Current readout faster, better
    noise immunity
  • Transfer of one test station to Frankfurt
  • Support RD efforts starting with MIMOSA11
  • Aspects of cryogenic operation

12
Assessment for GIGATRACKER
http//na48.web.cern.ch/NA48/NA48-3/groups/gigatra
cker/
  • NA48 CERN-SPSC-2004-029 (K?pnn)
  • Concept (only small area needs to be covered)
  • High rate 40 MHz / cm2
  • 100 ps time resolution
  • Fluence 4.5 1014 cm2 (12 Mrad)
  • 0.13 mm envisaged

x/X0 lt 0.6
13
STS working packages
14
Design optimization
Mainframe
STS group
Tracking groups
Algorithms
Digitizers
MAPS HitProducer (Michael)
Design Optimization
Strip HitProducer(Valeri)
Final configuration
15
Towards a Design Proposal
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