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The TileHCAL, studies and time plans, V' Korbel, DESY, 30m

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The last meetings since ECFA-DESY workshop in Prague (Nov. 2002) actual status of R&D: ... design/build cassettes, for 9 tiles, 9 mm tick, 27 pieces for July tests ... – PowerPoint PPT presentation

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Title: The TileHCAL, studies and time plans, V' Korbel, DESY, 30m


1
The Tile-HCAL, studies and time plans,V. Korbel,
DESY, 30m
  • The last meetings since ECFA-DESY workshop in
    Prague (Nov. 2002)
  • actual status of RD
  • scintillators
  • WLS-fibres, clear fibres, fibre coupling
  • optimisation of tile-fibre system (TFS)
  • photodetectors
  • preamps
  • measurements with the minical
  • readout and DAQ
  • cosmics,
  • noise and pedestals
  • LED-calibration
  • plans for e-beam test at DESY (summer 2003)
  • status of preparations for the 1m3 prototype for
    E-flow beam tests
  • photodetectors
  • preamps
  • VFE RO boards

2
The last Tile-HCAL meetings
  • Since the Prague ECFA-DESY workshop
  • main meetings 4.12.2002, 20.1.2003,
    4.3.2003
  • LAL-Orsay, preamps for APDs, dela Taille,
    Cvach,... Dec. 2002
  • CERN, VFE for APDs with DUBNA, I. Golutvin, I.
    Tiapkin, F. Sefkow, Dec. 2002
  • DUBNA, VFE, I. Golutvin, I. Tiapkin, Y. Gilitski,
    Minsk people,.... Febr. 2003
  • ITEP and MEPHI, Moscow, B. Dolgoshein, V.
    Rusinov,..... Febr. 2003
  • LAL-Orsay, VFE for APDs, dela Taille, I. Tiapkin,
    F. Sefkow,... Febr. 2003
  • ????
  • future main meetings 6.5.2003, 17.6.2003 ??? To
    be fixed these days

Documentation 1. tasks, institutes, people,
time plans, meetings, talks and minutes in
Web gtgtgthttp//www.desy.de/korbel/see/tilehacal/.
... 2. detailed Tile-HCAL RD report, Oct. 2002,
available The Tile-HCAL Calorimeter
for the TESLA Detector, a Status Report
on the RD-Studies 3. new web-page with
better guidance is prepared, open next week!
3
Presentations for the Tile-HCAL on this workshop
  • CALICE collaboration meeting (Monday,31.3.03,NIKHE
    F)
  • V. Korbel, Introduction to CALICE Tile-HCAL
    meeting
  • Status of the RD, 15
  • M. Danilov for ITEP, RD in Russia, 20
  • B. Dolgoshein for MEPHI,
  • News from the Si-PMs as
    Photodetetctors for the Tile-HCAL, 20
  • S. Nemecek for Prague,
  • APDs for the HCAL, gain
    stability
  • V. Korbel for DESY, LPI
  • Tests with the minical, plans
    for prototype, time scale
  • DAQ and Trigger meeting
  • V. Korbel, DAQ concepts for the minical and
    Tile-HCAL prototype, 10
  • P. Daucey, CALICE beam test DAQ
  • Calorimeter Session, Hadronic Calorimeter
  • V. Korbel, The Tile-HCAL, studies and time plans
  • V. Morgunov for DESY, ITEP, Prototype Tile-HCAL
    Simulation with
  • Si-PMs as Photodetectors
  • P. Dauncey, DAQ for the CALICE beam test

4
The plastic scintillators for the tiles
  • The different scintillators studied
  • PVT -BC-408, BC-404,.....
  • PS
  • SCSN-81, Kuraray
  • new RD scintillators from Kuraray
  • ITEP/Vladimir BASF-143, others
  • Protvino/LPI SC-306M, SC-307.....
  • Charkov
  • The PS scintillators based on PS
  • show 0.5..0.65 LY of PVT
  • but 5 x cheaper
  • possibility to cast them in tiles
  • (with grooves)
  • gtgtgt made studies on
  • LY and uniformity, ok?
  • gtgtgt decision to select producer

M.Danilov,CALICE main recent measurements in ITEP
5
Details of TFS Optimisation Studies
Centre/straight WLS-fibre
Diagonal/bent WLS-fibre
No stress on fibre, fibre refl. tile
reflector

more stress on fibre, fibre refl. tile
reflector
L7.85cm
L7,85cm
L5cm
clear RO fibre to couple 1-3.5m in
detector, light attenuation lt18
  • Double looped fibre
  • strong fibre bend,
  • most stress on fibre,
  • probably ageing damages,
  • fibre end fibre reflector
  • inside tile gtgtgt
  • special reflective coating
  • needed ?
  • 1.1 mm hole in center
  • drilled and polished?
  • could it be made during tile moulding?

L31,4cm
6
The WLS-fibres
1 mm diameter, double clad, BC-91A BC-92 BC-Daygl
o, red range extended Kuraray, Y-11(100-500ppm)
WLS shifting component polishing of fibre
end fibre end reflector attenuation
length conversion efficiency stability against
bends, loops (2.4 mm radius) ageing agains bend
stress, in radiation field gtgtgtgt Y-11(300) for
short fibres Y-11(500) for long
fibres material available for all minical channels
University Friedberg/Giessen
7
The coupling of WLS-fibres to scintillator
, similar to BC-408, 404
Have selected Kuraray Y11(300)
8
TFS LY measurements at ITEP
M.Danilov,CALICE main
9
The actual achieved LY for the TFS
Scintillator BC-408,
, Kuraray, WLS-fibre
3M-Super Radiant Reflector
Light yield/tile/MA-PM
  • 22/-1.5 pe (BC-408, Aug. 2002)
  • gtgt 26 (new results from ITEP)
  • both Russian scintillators
  • have 2/3 of BC-408 LY
  • 20 more LY can be expected
  • by improving polishing
  • of WLF-fibre end,
  • no gluing needed anymore

All together
100 reflectivity at fibre end
10
Light attenuation measurement in RO-fibres
WLS-fibre, Kuraray
10,20,50 and100 cm
clear-fibres, Bicron and Kuraray
  • attenuation in clear RO-fibres minimal
  • BC-98 0,65 db/m 40 for 5m fibre
  • no damage observed for bent fibres
  • (d5 cm)
  • no ageing during 1 day observed
  • gtgtgt Y11(300), on tile BC-98 RO-fibre

(ITEP)
Photocathode sensitivity of APD
11
WLS fibre-clear fibre connection
  • WLS-fibre gtgtclear fibre
  • standard is gluing with optical glue
  • better procedure
  • thermo-fusing, 80-120oC,
  • heating by 1-2 windings of resistive wire
  • fibres cut, adjusted and pushed together
  • in glass tube of 1.10 mm inner hole diameter
  • few A current for a few sec.
  • gtgt connection difficult to find by eye
  • no light loss seen at connection
  • first results 84 transmission
  • improvement potential
  • still available in the fusing procedure
  • Well established procedure at FNAL
  • for CDF calorimeter, 90 transmission
  • gtgtproduction parameters
  • can be optimised

Pressure, temperature, time guide tube diameter ?
12
Photodetectors
The remaining candidate photodetectors APDs
S8664-55spl, 3x3mm2, S8550, 32 pixels of
1.6x1.6mm2 at test in
Prague Si-PMs (MEPhI) gain 2106
photocathode eff. 15-20 sizes 1x1mm2,
576 and 1000 pixels/mm2 -800-1200
Photodetectors needed (APDs) with 3-7 tiles
combined to calo cells or -3200-4800 Si-PMs of
1x1mm2 needed alternatively -decision to use both
detectors in prototype
13
APDs
Hamamatsu, 3x3mm APD, S8664-55spl package is same
as S8664-55 (5x5 mm APD)'s with
resin coating. Delivery time takes 1.5 months for
30 pcs typical performance gain 50 100
gt1000 possible Id 600pA 1.2nA C 28pF
28pF have 6 APDs for tests 170 Euro per piece,
for 30 122 Euro per piece, for 300 60 Euro per
piece, for 1500 25 Euro ? for gt 100 000 APDs?
Future plan (Hamamatsu) APD Array try to
make low capacity type, proceed with "3 x 3
mm, 4 x 4 ch APD-array". target characteristic is
as follows. C 15 pF Variation of
gain /- 20 to 30
GAIN M
C
100
Id
10
500 V
14
SiPMs, Silicon Photomultiplier
RD at MEPHI (Moscow), B. Dolgoshein, together
with PULSAR (Russ. Industry)
  • Some features
  • Sensitive size 1x1mm2 on 1.5x1.5 mm2
  • Gain 2?106 at Ubias 50V
  • Recovery time 100 ns/pixel
  • Nuclear counter effect negligible
  • (due to Geiger mode operation)
  • Number of pixels 576, now 1000/mm2
  • Dynamic range gt 200

For further details see Advanced study of
SiPM http//www.slac.stanford.edu/pubs/icfa/fall0
1.html
15
Performance of SiPMs with 1 scint.Tile
minical
4-8 pe 576 px 53-55V
15 pe 1000 px Si-PM on tile
10 pe, 576 px 54V
DESY e-test beamwith various Si-PMs (MEPHI)
16
Si-PMs, dark rate and MIP detection
Sum of 3 tiles,e-beam test DESY
576pix/mm2 From Elena Popova, MEPhI
17
Minical array
Stack and Tile structure
  • Assembled with up to
  • 27 scintillator layers,
  • of 9 tiles each,
  • 5x5X0.5 cm3
  • 243 scintillator tiles
  • or
  • 81 cells of 3 tiles
  • read out by
  • 50 cm WLS fibres to
  • photo-detectors
  • APDs 3 tiles/APD
  • MA-PMs 16fold, 3 tiles/pixel
  • Si-PMs 1 tile/Si-PM
  • also1x32 M-APD array (Pra
  • Aim of this device is
  • cosmics, study of
  • LY
  • uniformity of response
  • calibration with MIPs
  • stability of MIP signals
  • different photodetectors
  • long term ageing
  • LED monitoring
  • stability
  • dynamic range
  • e-beam, study of
  • energy resolution
  • constant term

18
Minical, pictures
19
Minical, pictures
20
Where are we?
  • Status now, for minical tests
  • WLS-fibres ordered and delivered, 500m(Y11-300)
    and 100m(Y11-500)
  • 3M super-reflector foil available
  • minical now modified by Prague group
  • 9 mm gaps, larger housing,
    windows for feed-through, light tight,
  • easier access to interior
  • 6 new Hamamatsu APDs (3x3 mm2, 190 Euro/piece)
    now at DESY
  • to be inserted in minical for MIP tests, yield
    next 3 weeks ?
  • Si-PM production/delivery schedule (see Boris
    talk)
  • next 30 available, than 100 up to June,
    1000 pixels/mm2
  • TFS geometry, reduce variety soon, up to end
    April
  • design/build cassettes, for 9 tiles, 9 mm tick,
    27 pieces for July tests
  • preamps to design/order gtgt LAL Orsay 7.4.03,
    delivery 30.6.03
  • RD for Minsk/Gilitski, Prague, DESY/Smirnov
    types goes on
  • APDs and Si-PMs to order gtgt 30 APDs and 100
    Si-PMs (with 1000pixels)
  • HV distribution to design/order/build
  • 380-420V, APD, 30 channels
  • and 55-68 V, Si-PM, 100 channels

21
minical-tasks, TFS production details
  • The TFS for the minical
  • --81 tiles with Si-PMs, short WLS-fibres, SI-PM
    inserted, from Vladimir/ITEP
  • --81 tiles from Protvino, with cylindrical
    holes??,
  • cast in moulds, together with the tiles or
    drilled, to insert the WLS-fibres
  • --81 tiles from BC-408, cut and polished at DESY,
    with
  • a) WLS-fibres in cylindrical, drilled
    central holes, 50 cm more fibre to APDs
  • b) WLS fibres in curved diagonal grooves,
    also 50cm to APDs
  • Hope to have a technology to replace the
    WLS-fibre
  • outside the tiles by fused clear fibres,
    who does it?
  • Can ITEP prepare also the 81 Protvino tiles?
  • gtgtI.e. make grooves or holes, insert fibres,
    wrap tiles, test in black box?
  • A special gt5 cm long drill of 1.1 mm diameter is
    in preparation at DESY.
  • We need to group tiles with equal (/-5) LY,
  • 3 tiles of same response to one APD. Thus LY
    of all 81 TFS to be measured
  • with a source. To do at DESY with help of
    Protvino/LPI people.
  • Our Time scheme
  • Production of tiles in April/mid May
  • Machining/Wrapping in May/ mid June
  • Tests and selection in June/mid July

22
Support frames for TFS
For APDs
For SI-PMs
MEPhI, ITEP
23
Direct TFS readout with SiPM
in minical at DESY
M.Danilov,CALICE main
24
Shower containment in minical, DESY e-beam
1 section, 9 layers, 81 cells
MIP peak used for calibration
Shower leakage to correct with the middle
section of minical
Studies by V. Andreev gtgtgt
25
Energy resolution in minical, DESY e-beam
  • s/Ea/sqrt(E) () c
  • Aim is to study
  • the effects contributing
  • to the constant term
  • LY fluctuations within tiles
  • lat. non-uniformity of response
  • MIP calibration precision
  • stabilty of calibration
  • noise
  • dead gaps between tiles
  • leakage

26
Energy resolution in minical, Si-PM, 576 pixels
Saturation curve number of fired pixels
vs number of photons x photo-conversion
efficiency s/Ea/sqrt(E) () c
27
Calibrating the minical cells
BC-408 scintillator single tile, diagonal bend
groove, cosmic m-peak, 60 cm WLS fibre
RO MA-PM 23,1-26,2 pe
  • Noise, randoms
  • cosmics
  • LED-pulses

28
Calibrating minical cells, studying LY
BC-408 scintillator single tile, diagonal bend
groove, cosmic m-peak, 60 cm WLS fibre RO to
MA-PM 23,1-26,2 pe
Random and pedestal subtracted cosmic m-peak
spectra of some PS-scintillators from
Protvino/LPI 9-13.3 pe
29
Remote web access to the measurements
Study the results of up to 64 channels with MIPs
  • Install in minical
  • different
  • scintillators
  • fibres
  • photodetectors
  • pre-amps
  • supply voltages
  • trigger conditions

At DESY
LED monitoring
Start run with new components or new settings all
24 hours.
  • Look for
  • gain
  • stability
  • signal width
  • signal noise separation
  • calibration with MIPs
  • run parameter file
  • via web
  • sw-tools
  • F. Krivan
  • V. Dodolov
  • A.Terkulov
  • S. Karakash

ITEP LPI MEPHI Prague Protvino DESY ....
very similar situation later during prototype
running in beam test at other laboratories
30
HCAL prototype for E-flow studies
  • Required volume 1 m3
  • 800-1200 calorimeter cells
  • Fe-structure can accept
  • analogue
  • or digital HCAL??

10 GeV pions
100 cm
Leakage detector needed!
100 GeV pions
31
The Prototype stack
  • Design/Construction Studies
  • TDR
  • LC-notes
  • K. Gadow, VK
  • DESY, Jan. 2003
  • Need now to come to decisions
  • how to build?
  • Steel, ss?
  • 2 half modules (magn.field?)
  • Where?

32
more on tile sizes and total numbers
38 layers require 5000 tiles with 38 different
tile sizes casting with minimum number of
moulds! Need to fix tile sizes soon!
33
Prototype channels
34
The fraction of prototype cells fired
Simulation studies for single pions beam
energies 10, 40, 100 GeV RO threshold cuts 0,
0.25, 0.5 MIP standard granularity 5x5cm2,
3 cells deep(3/9) 6x6cm2, 3 cells deep(4/12)
8x8cm2, 2 cells deep(2/10) 12x12cm2, 1 cell
deep (1/7) 969 cells in total
By V. Andreev
35
Energy sharing between ECAL and HCAL-PT
The following studies from V. Andreev ECAL and
TC have effect on energy resolution 45-55 of
events depose more than 2 GeV in ECAL
36
Prototype TC for energy resolution
37
The contribution of the TC to the energy
measurement
E(ECAL) E(HCAL) lt--gt E(TC)/(E(ECAL) E(HCAL))
Epion5,10,20,30,50 GeV
38
The VFE-ROB-scheme, APDs
Online/Offline Gain/HV monitoring?
DAC-signals
PIN diode for LED monitoring
LED signals
beam
cosmic
HV, 380-420V dV/V10-4
Trigger/ RO clock
DAC
Charge injection
pedestals
Array of single APDs or matrices
pulse shapers
Sample hold
Multi plexer (analog)
charge sensitive preamps
39
Time Planing, 4.3.2003, I
  • 1. Pre-selection of appropriate photodetectors
  • available APDs(6) and Si-PMs(10)
  • ordering larger quantities for more tests in
    minical (March).
  • Need 30 APDs and 162 Si-PMs in total, Si-PMs
    (1000 pixels!)
  • 2. studies and development of integrated
    preamplifier/shaper circuits,
  • and MEPhI Si-PM with FE preamps.up to end
    April.
  • Operation in Minical.
  • 3. For minical decide on the optimal APD-preamp
    type, end March
  • ---study Minsk and Prague preamps with APDs
    in minical,
  • --- important get noise contribution to
    MIP-peak (noise vs MIP efficiency)
  • ---order/loan 2 prototype CALICE-ECAL PCI
    preamp boards
  • (which should later integrate the
    photodetector connections)
  • 4. Concept/design final preamp prototype boards
    for
  • the 1000 channel test prototype, ....all and
    DUBNA?, (April)
  • 5. design prototype boards for all APD and Si-PM
    channels, DUBNA?,(May)
  • 6. Up to May to decide, which photodetectors in
    which quantity to use
  • 1000 APDs or 5000 Si-PMs,
  • or both types in relevant quantities e.g.
    200/2500
  • 7. order of all photodetectors for the Tile-HCAL
    prototype, June

40
Time Planing,II
9. Need Russian scintillators for tests in
minical, (20 each, March) 10. ordering Bicron
BC-408 for the larger tile sizes, 8 m2, up to
Summer 11. define optimal cell and tile sizes,
from software and hardware studies, decision
up to end of April 12. Prepare 300 tile minical
test at DESY, (100/100/100) May 13. design of the
prototype stack, April/May 14. a detailed
tile-plate assembly concept has to be defined,
July 15. Minical test at DESY, with final
photodetector types, July-September 16. building
of stack steel absorber structure, in ITEP or
Prague? gtAugust 17. casting/machining of 3700
tiles up to September, (in factory ? or
machining at DESY, or elsewhere?) 18. assembly of
the TFS in tile plates (detector cassettes),
November 19. TFS connection with photodet. and
preamps, start November-December 20. RO via CAMAC
as long as British DAQ not available, end
2003 21. winter 2003/2004 operation studies with
LED gain monitoring, and calibration
studies with cosmic muons, with increasing
number of calorimeter cells as assembled.
41
Outlook
  • 1. Enough LY from TFS (200 photons at
    photodetector)
  • 2. APDs and SI-PMs are the photodetectors which
    do the task
  • 3. Preamplifiers with low noise are essential
    (MIP-noise separation,calibration)
  • 4. Minical test to establish calibration
    precision in summer
  • 5. Now design of prototype boards for APD and
    Si-PMs, DUBNA
  • 6. Photodetectors, large quantity to order in
    summer
  • 1000 APDs or
  • 5000 Si-PMs or
  • both types in relevant quantities e.g.
    250/3500
  • 7. Prototype stack (1m3) will be build in summer
  • 8. Assembly of PT-stack with TFS starts in Jan.
    2004
  • 9. Spring 2004 is used to set up and calibrate
    all channels with cosmics.

42
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