1 / 31

RICH workgroup program

RICH workgroup program. Wednesday, October 15, 2008:. Electron identification. Status RICH R&D. layout and design E. Vznuzdaev , O. Tarasenkova, E. Belolaptikova, S. Lebedev mirror M. Dürr Photodetector S. Bianco, P. Koczon, CH WLS film studies FEE test setup at GSI

nizana
Download Presentation

RICH workgroup program

An Image/Link below is provided (as is) to download presentation Download Policy: Content on the Website is provided to you AS IS for your information and personal use and may not be sold / licensed / shared on other websites without getting consent from its author. Content is provided to you AS IS for your information and personal use only. Download presentation by click this link. While downloading, if for some reason you are not able to download a presentation, the publisher may have deleted the file from their server. During download, if you can't get a presentation, the file might be deleted by the publisher.

E N D

Presentation Transcript

  1. RICH workgroup program Wednesday, October 15, 2008:

  2. Electron identification

  3. Status RICH R&D • layout and design E. Vznuzdaev, O. Tarasenkova, • E. Belolaptikova, S. Lebedev • mirror M. Dürr • Photodetector S. Bianco, P. Koczon, CH • WLS film studies • FEE • test setup at GSI • activities at IHEP Protvino V. Rykalin • prototype I.-K. Yoo, J. Yi, et al.

  4. RICH design • Visit of Evgeny Vznuzdaev and Olga Tarasenkova (PNPI, St. Petersburg) at GSI, April 2008 • discussion on RICH design • so far dimensions are still subject of layout optimization • only range can be given (compact to standard RICH dimensions) • discussions on integration of RICH an MuCh in CBM Cave • mirror layout and support discussed in some more detail • current schedule: • Preproduction design and prototyping: 2009 - 2010 • Production : 2011 - 2015 • Assembling and testing : 2014 - 2015

  5. RICH mirror design • "mirror and support are one thing" (!) • important consideration: mirror tiles of hexagon or rectangular shape? • mirror material: glass, carbon, beryllium ? • mirror support structure – depends on shape of mirror tiles or or ... hexagon tiles: one mount in center of mirror adjustment around 2 axis rectangular tiles: typically 3 adjustable mounts also shift along z-axis possible

  6. Hexagonal mirror tiles Hexagon effects: • Lack of exact geometrical description; impossible to divide a spherical surface into hexagons exactly ; one can only to approximate (manually?) the surface by hexagons with irregular gaps between them (0.5-12mm); • Cutting of hexagons to fit a line between 2 mirrors and to fit (if necessary) other sides of the surface  different size of hexagons. E. Vznuzdaev, PNPI St. Petersburg

  7. Rectangular mirror tiles Latitude/longitude division: • The globe-wise division has a precise geometrical description; • Minimal gaps between units, only technological gaps; • Only 2 variants of unit dimensions; • No fitting cuts for units E. Vznuzdaev, PNPI St. Petersburg

  8. RICH mirror design considerations Detector Rc Division S/mirror S/unit Mirror Rad. [m] layout [m2] [m2] substrate thickness ---------------------------------------------------------------------------------------------------- Hermes 2.2 2x4 (T*) 1.6 0.8x0.25 CFC 0.01 LHCb(1) 2.7 1x4 (T*) 1.9 0.8x0.6 Be 0.007 CBM 3.0 ? 5.9 ? ? ? PHENIX 4.0 2x12(T*) 10.0 0.8x0.5 CFC 0.004 ---------------------------------------------------------------------------------------------------- Compass 6.6 58(H*) 10.5 0.18(0.5**) Glass 0.06 LHCb(2) 8.6 21(H*) 4.1 0.17(0.5**) Glass 0.05 * T – trapezoid, H – hexagon ** diameter of circumscribed circle E. Vznuzdaev, PNPI St. Petersburg

  9. RICH mirror design considerations Common consideration (hexagonal shape): The geometrical relation between linear dimension of mirror unit d and radius of curvature Rc for Compass/LHCb2 case: K=d/RC=0.5/7.5 = 0.067 (soccer ball has K~0.75). Let us take the same K for CBM case. Then: d=(Rc)xK=3.0x0.067=0.2m, and number of hexagon units is 84 for square of 5.9m2, what significantly increases amount of substance for mirror support (radiation thickness). Also we should increase correspondingly the number of tuning elements for mirror unit and time for their assembling and adjustment . All above brings to increasing of the cost for the mirror support also. E. Vznuzdaev, PNPI St. Petersburg

  10. RICH mirror design considerations Detector Rc Division S/mirror S/unit Mirror Rad. [m] layout [m2] [m2] substrate thickness ---------------------------------------------------------------------------------------------------- Hermes 2.2 2x4 (T*) 1.6 0.8x0.25 CFC 0.01 LHCb(1) 2.7 1x4 (T*) 1.9 0.8x0.6 Be 0.007 CBM 3.0 84(H*) 5.9 0.07(0.2**) Glass 0.05 PHENIX 4.0 2x12(T*) 10.0 0.8x0.5 CFC 0.004 ---------------------------------------------------------------------------------------------------- Compass 6.6 58(H*) 10.5 0.18(0.5**) Glass 0.06 LHCb(2) 8.6 21(H*) 4.1 0.17(0.5**) Glass 0.05 * T – trapezoid, H – hexagon ** diameter of circumscribed circle E. Vznuzdaev, PNPI St. Petersburg

  11. RICH mirror design considerations E. Vznuzdaev, PNPI St. Petersburg

  12. RICH mirror design considerations Detector Rc Division S/mirror S/unit Mirror Rad. [m] layout [m2] [m2] substrate thickness ---------------------------------------------------------------------------------------------------- Hermes 2.2 2x4 (T*) 1.6 0.8x0.25 CFC 0.01 LHCb(1) 2.7 1x4 (T*) 1.9 0.8x0.6 Be 0.007 CBM 3.0 3x10(T*) 5.9 0.43x0.46 Glass 0.05 PHENIX 4.0 2x12(T*) 10.0 0.8x0.5 CFC 0.004 ---------------------------------------------------------------------------------------------------- Compass 6.6 58(H*) 10.5 0.18(0.5**) Glass 0.06 LHCb(2) 8.6 21(H*) 4.1 0.17(0.5**) Glass 0.05 * T – trapezoid, H – hexagon ** diameter of circumscribed circle E. Vznuzdaev, PNPI St. Petersburg

  13. RICH mirror R&D • February 2008: first mirror prototypes tested (FLABEG, 6mm thickness, 3.2m radius Al+MgF2 reflective coating) • good reflectivity (75% at 180nm) • however: surface irregularities on cm scale • nevertheless: one sample shipped to Pusan (Korea) for new RICH prototype • discussions with FLABEG, • but 2nd mirror sample of • FLABEG had basically same • deficciency • contact to Compass company • (Czech), waiting for new • prototype • (supplier of RICH2 mirrors • of LHCb) M. Dürr, HS Esslingen

  14. Mirror mount • mirror mount for rectangular mirrors: • to be tested as soon as possible together with new mirror prototypes • test bench available at PNPI E. Vznuzdaev, PNPI St. Petersburg

  15. Open Questions (Selection of open questions:) • mirror material – glass, carbon beryllium??? • material of mirror mount – aluminum, carbon structures, ... ??? • which material budget can we allow for while still having highly efficient global tracking capabilities? • mirror radius? • RICH layout, size? • can we stay with direct reflection to photodetector plane and resulting high ring densities with smaller radius? • sufficient surface regularity with small mirror radii? (what is sufficient?) simulations and work of E. Belolaptikova, S. Lebedev simulations to be done, test in RICH prototype

  16. RICH layout studies • RICH layout studies by Elena Belolaptikova (GSI summer student): • systematic studies on RICH material budget (standard RICH), in particular concerning the RICH mirror and its effect on global tracking • glass mirror of 3mm, 6mm, 10mm thickness • aluminum support structure from aluminum rods included: • radius 3 cm, 5mm wall thicknes • radius 1.5 cm, 2 mm wall thickness (proposal of E. Vznuzdaev, industry standard) • layout optimization of compact RICH detector • Systematic investigation and improvement of ring finder in high ring density environment, Simeon Lebedev (GSI/JINR) • ring finding and electron identification for standard & compact RICH scenario

  17. Photodetector R&D (GSI) • GSI activities on photodetector FEE, single photon test setup • (Simone Bianco (summer student), Piotr Koczon, C.H.) • wavelengthshifter (WLS) film studies in cooperation with CERN * • development of FEE based on n-XYTER for MAPMT (Hamamatsu, H8500) • development of test setup for single photon measurements at GSI • pulse height distributions of single photons • crosstalk effects with and w/o WLS films * cooperation and help by A. Braem, M. van Stenis, C. Joram

  18. Photodetector test during CBM testbeam Sep'08 ? • plan was: participate with photodetector test, use Cherenkov light generated by protons (p = 3.5 GeV/c (2.3 GeV/c)) in plexiglas: Hamamatsu H8500 H8500 ~6 cm DR Quarz R g a b = q-g ~6 cm q testbeam: protons, p=3.5 GeV/c L tilting needed because otherwise light would be internally reflected in quartz to check: when does intenal reflection set in again sina = n sin(q-g) → for g = 20° is a = 37.7° for Quartz thickness of 1cm and R=5cm: L = 3.16 cm, DR = 1.15 cm

  19. Simulations - testsetup setup in CbmRoot • simulations: • best tilting angle of plexiglas 45° • appr. 50 photons/ event (plexiglass of 8 mm thickness) appr. MAPMT image S. Bianco, CH, GSI

  20. n-XYTER readout for H8500 • use n-XYTER chip for readout of H8500 • problem: typical gain of H8500 1-2∙106 but dynamical range of n-XYTER 120000 e- • need attenuator of appr. factor 20-50 • → prepare PCB board n-XYTER FEB designed as general pupose board attenuator PCB board S. Bianco, CH, GSI

  21. CBMRICHAB01 PMT N-XYTER • PCB board produced, several R-C combinations tested with test pulse • ongoing discussions with detector lab S. Bianco, CH, GSI

  22. Test of CBMRICHAB01 15 ns 0.04 V • input (pulse generator): 2 V, 10 ns • R2 = 100 W, C1 = 1 nF, C2 = 10 pF • R1 = 91 W , R2 = 10 W, C1 = 0 nF, C2 = 10 pF test with n-XYTER S. Bianco, P. Koczon, GSI

  23. .... n-XYTER FEB missing • test setup was ready for the beam, however an n-XYTER FEB was missing (only 3 became available – 2 for the silicon strips, 1 for the GEM) S. Bianco, CH, GSI

  24. Next steps • more n-XYTER FEBs will become available in the near future, one existing (Rev B) can be shared already now with the silicon strip R&D group (J. Heuser) • develop and understand n-XYTER readout of H8500 • consider separate future version of CBM-XYTER specifically for H8500 • investigate characteristics of H8500 • single photon response, homogenuity across the surface and single pixels • crosstalk effects w and w/o WLS coverage • use MAPMT test setup for next CBM testbeam in February/ March 2009 • provide readout to group of i.K. Yoo, Pusan University, Korea

  25. RICH prototype • development of RICH prototype at Pusan University, Korea (I.K. Yoo JunGyu Ji, et al.) • first small scale prototype already investigated • 2nd full scale prototype to be build autumn/ winter 2008 • test various radiator gases/ mixtures • combine parts developed elsewhere: • implement first mirror prototype (FLABEG, 20 cm x 20 cm) • once available: use n-XYTER for readout • test: electron beam at TEST LINAC, PAL (Pohang Accelerator Lab.), Korea. ; (pe ≈ 60MeV/c) • problem: very wide beam spot, poor beam quality • → implement beam diagnostics, collimators!

  26. RICH prototype vessel mirror: R = 2700 or 3200 mm extension mount for 4 H8500 MAPMTs side door vessel_front window J. Yi, I.K. Yoo, Pusan University, Korea

  27. Photodetector "plane" in prototype J. Yi, I.K. Yoo, Pusan University, Korea ring on 4 MAPMTs

  28. Mount for 4 MAPMTs Mount_0 Mount_1 Bolt 4PMTs J. Yi, I.K. Yoo, Pusan University, Korea

  29. Gas system Molecular Sieve P : 3 atm P : ~1 atm P : 3 atm • T : 25C • P :±20mbar • H : ~ 23%RH 3196 ppm J. Yi, I.K. Yoo, Pusan University, Korea

  30. Summary: RICH prototype • gas vessel under production in Pusan • develop beam setup which allows to work with the existing poor beam quality • n-XYTER readout to be investigated/ developed at GSI • 1st mirror prototype delivered by HSE • future prototypes will be combined and tested with mirror mount

  31. Discussion • layout and design studies • mechanical concepts developed at PNPI, details on RICH size and mirror layout missing for further progress • detailed (promising!) simulations on RICH material budget (mirror and mount), RICH layout, e-ID in high ring density environment • mirror R&D • 1st prototype shipped to Pusan for RICH prototype • new prototypes expected soon, if promising combine with mount • photodetector R&D • promising WLS film studies (crosstalk with MAPMT?) • FEE under way (plan use of n-XYTER FEB) • test setup at GSI under development • prototype under construction at Pusan university • important: get beam quality under control!

More Related