1 / 24

High Resolution Hypernuclear Spectroscopy at Jefferson Lab, Hall A: the Experimental Challenge

High Resolution Hypernuclear Spectroscopy at Jefferson Lab, Hall A: the Experimental Challenge. Francesco Cusanno , INFN Gruppo Sanità, Sezione di Roma. Hall A Experimental setup modification The Septum Magnets Optics of new High Resolution Spectrometer setup The Jlab Hall A RICH Layout

Télécharger la présentation

High Resolution Hypernuclear Spectroscopy at Jefferson Lab, Hall A: the Experimental Challenge

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. High Resolution Hypernuclear Spectroscopy at Jefferson Lab, Hall A: the Experimental Challenge Francesco Cusanno, INFN Gruppo Sanità, Sezione di Roma • Hall A Experimental setup modification • The Septum Magnets • Optics of new High Resolution Spectrometer setup • The Jlab Hall A RICH • Layout • Electronics Read Out and DAQ • Performance and results during • experiment e94-107 – • electroproduction of Hypernuclei • Rich upgrade for higher momenta and faster acquisition • Conclusions IXth International Conference on Hypernuclear and Strange Particle Physics (HYP06) - Mainz, Germany, 10 -14 October, 2006

  2. Jefferson LABSite Location and the CEBAF facility Hall A Francesco Cusanno – HYP06 – Mainz, Germany, 10 – 14 October 2006

  3. Optimization of Optics: the Database Francesco Cusanno – HYP06 – Mainz, Germany, 10 – 14 October 2006

  4. Performances of New Setup and Database Typical HRS System Four Optical Elements (QQDQ) Design Resolution 10-4 FWHM momentum resolution Previously best obtained 2.5 10-4FWHM momentum resolution Multiple Coulomb Scattering is the reason for the difference Old D.B. New D.B. Both Spectrometers Have Demonstrated ~ 10-4 FWHM δResolution Francesco Cusanno – HYP06 – Mainz, Germany, 10 – 14 October 2006

  5. Hadron Identification through Aerogel p p k ph = 1.7 : 2.5 GeV/c All events p k p AERO1 n=1.015 AERO2 n=1.055 Protons = AERO1 • AERO2 Pions = AERO1 • AERO2 KAONS = AERO1 • AERO2 Francesco Cusanno – HYP06 – Mainz, Germany, 10 – 14 October 2006

  6. Hypernuclear spectroscopy KAON Id Requirements – Physics case Signal Vs. Background Monte Carlo • Very forward angle  high background of p and p • TOF and 2 threshold Cherenkov aerogel are NOT sufficient for unambiguous K identification • RICH DETECTOR Francesco Cusanno – HYP06 – Mainz, Germany, 10 – 14 October 2006

  7. JLAB Hall A RICH layout – similar to ALICE HMPID RICH Freon Radiator: 1800x400x15 mm3 single box with quartz windows glued on neoceram housing Grid plane: 100 mm positive wires (collects electrons ionized in the gap) Wire chamber : composed by 20 mm anode wires plane sandwitched between a cathode plane formed by 100 mm wires and the cathode plane formed by the photocathodes Three Photocathodes : 403x640 mm2each, divided in 8.4 x 8 mm2 size pads evaporated with a 300 nmCsI layer Francesco Cusanno – HYP06 – Mainz, Germany, 10 – 14 October 2006

  8. N. of detected photoelectrons Õ = J e D » 2 N 370 L sin E 20 . . p e c i i JLAB Hall A RICH MonteCarlo Simulations Separation power p, K Separated by qp – qK = 30 mrad p, K Separated by  6.8 s Francesco Cusanno – HYP06 – Mainz, Germany, 10 – 14 October 2006

  9. JLAB Hall A RICH: some components Francesco Cusanno – HYP06 – Mainz, Germany, 10 – 14 October 2006

  10. Photocathode positioning in the glove box Francesco Cusanno – HYP06 – Mainz, Germany, 10 – 14 October 2006

  11. JLAB Hall A RICH: the evaporation system Quantum Efficiency 110 cm Measurement System details in : F.Cusanno et al. NIM A502(2003)251 Photocathode 120 cm crucibles 10-6 mbar vacuum 2 nm/s CsI deposition at T = 60ºC (CERN experts indications). Vacuum - heating conditions starts15 – 24 h before evaporation. A post-evaporation heat treatment is done for 12 hours. Francesco Cusanno – HYP06 – Mainz, Germany, 10 – 14 October 2006

  12. RICH front end electronics and DAQ system • 3 PhotoCathode each divided in 80*48=3840 pads  11520 tot. channels • FEE arranged in 8*6 = 48 rows each each rows handling 240 channels with 15 GASSIPLEX chips (for amplification, holding and multiplexing analogue signals – 16 pads per gassiplex chip) • Readout using CAEN System with CAEN V550 CRAMS and V551 Sequencer • 240 pads (15 Gassiplex chips multiplexed signal with zero suppression) per CRAM channel (10 bit FADC) • total number of 24 VME modules + 2 VME V551 Sequencer in two VME CRATES. • 2 MHz clock speed • no data buffering foreseen in CRAMS - CRAM memory read out for each trigger • Achieved performance : • sampling 120 ms (clock) + 10 ms = 130 ms • VME (60 hits) 54 ms • overhead 16 ms  200 ms deadtime per trigger • Experience : 20 – 25 % deadtime with 1kHz random trigger Francesco Cusanno – HYP06 – Mainz, Germany, 10 – 14 October 2006

  13. JLAB Hall A RICH Event Display during data taking Francesco Cusanno – HYP06 – Mainz, Germany, 10 – 14 October 2006

  14. JLAB Hall A RICH OPERATING conditions • Gas: Pure Methane (Minimize Photon Feedback, High Q.E.) • High Voltage: ~ 2100 Volts for a gain of 8x104 • Grid Voltage: 250 - 450 Volts • Optimal trigger to read-out delay: ~400 ns (peaking time of gassiplex response) cluster charge and hit size MIP charge and hit size Francesco Cusanno – HYP06 – Mainz, Germany, 10 – 14 October 2006

  15. Rich Performances – key parameters : p Cherenkov angle reconstruction Npe for p and P Nclusters Cherenkov average angle (rad) Npep/p ratio : Angular resolution : Francesco Cusanno – HYP06 – Mainz, Germany, 10 – 14 October 2006

  16. Rich Performances – PID : p/K population ratio Aero Selected p Angular resolution Aero Selected K (!) Aero Selected P Separation power Aero Selected K on a large sample of filtered data This would accept ~ 10-4 pions x p/K ratio 1/100 pion contamination …. But NON GAUSSIAN TAILS GIVE AN IMPORTANT CONTRIBUTION ! Kaon selection: Francesco Cusanno – HYP06 – Mainz, Germany, 10 – 14 October 2006

  17. Rich – PID – Kaon selection results : Time of coincidence for Aerogel Selected Kaons w/o and w/ rich : AERO K AERO K && RICH K p P K Francesco Cusanno – HYP06 – Mainz, Germany, 10 – 14 October 2006

  18. Rich – PID – Pion rejection factor : Time of coincidence for Aerogel Selected Pions: effect of Rich Kaon selection AERO p && RICH K AERO p p p N.Evts in the peak Backgnd subtr. = 64656 N.Evts in the peak Backgnd subtr. = 63 Pion rejection ~ 1000 Francesco Cusanno – HYP06 – Mainz, Germany, 10 – 14 October 2006

  19. Rich Possible improvements : • MWPC stability for high rates • For single rates ≤ 60 KHz HV=2100 V is OK • In the range 60 KHz – 100 KHz HV=2075 V is OK • Above 100 KHz HV must be reduced further •  MWPC stability (and mechanics) needs to be studied • for high rates running • However running at reduced gain with moderately good • performance seems to be feasable • p/K separation for p>2.5 GeV/c • Doable “just” replacing the radiator  C5F12 in liquid phase (<24°C) • DAQ rate bottleneck (~1kHz) can be overcome replacing front-end Francesco Cusanno – HYP06 – Mainz, Germany, 10 – 14 October 2006

  20. Rich p/K separation for p > 2.5 GeV/c Radiator C5F12 n=1.24 sCh~ 5mr Radiator C6F14 n=1.29 sCh~ 5mr 4 s separation at ~ 2.5 GeV/c 4 s separation at ~ 3.0 GeV/c Francesco Cusanno – HYP06 – Mainz, Germany, 10 – 14 October 2006

  21. Rich p/K separation Vs. proximity Gap length with C5F12 (n=1.24) radiator - MonteCarlo Simulations Francesco Cusanno – HYP06 – Mainz, Germany, 10 – 14 October 2006

  22. Rich p/K separation with C5F12 (n=1.24) radiator (14 cm proximity gap) MonteCarlo Simulations >20 s separation at ~ 2 GeV/c ~ 4 s separation at 3.0 GeV/c Francesco Cusanno – HYP06 – Mainz, Germany, 10 – 14 October 2006

  23. Rich electronics upgrade : The HMPID ALICE RICH DAQ scheme fbD[27..0] fbD[31..0] VME to Local Bus Interface LOC_ADD[11..0] LOC_ADD[3..0] DILO 5 Boards (ADC and DILOGIC) Column Controller (1 to 8) Segment Controller LOC_CS GASSIPLEX LOC_CS LOC_R/Wn LOC_R/Wn RCB BOARD SEGMENT Front end digitization/ multiplexing On board 48 multiplexed channels (instead of 240) Clock rate up to 10 MHz Francesco Cusanno – HYP06 – Mainz, Germany, 10 – 14 October 2006

  24. Conclusions: • Septum Magnets has been successfully operated, • High Resolution Spectrometers with Septum Magnets provide momentum resolution of 10-4 FWHM • The RICH detector has been successfully operated during the • hypernuclear experiment at JLab • It is a powerful tool for Particle Identification • Average Cherenkov angle resolution sq~ 5 mr in good agreement with • Monte Carlo simulations • Clean kaon identification is possible with a pion rejection ratio ~1000 • Upgrade foreseen both to increase the max DAQ rate limit and to increase momentum range for p/K separation Francesco Cusanno – HYP06 – Mainz, Germany, 10 – 14 October 2006

More Related