EIC Detector – JLab – 04/June/2010
EIC Detector Workshop
JLab : 4-5/June/2010
HERMES: Forward RICH Detector
Evaristo Cisbani / INFN-Rome Sanità Group
Cisbani / HERMES RICH
Most of the slides from R. De Leo and D. Ryckbosch
• Overview
• Performances
• Inheritance
• HERMES RICH in SBS HallA
• Aerogel RICH in CLAS12
1
HERMES Experimental Setup
EIC Detector – JLab – 04/June/2010
e+N e’ + h +X in DIS
Cisbani / HERMES RICH
2 identical RICH modules
2
Hadron PID: HERMES RICH
EIC Detector – JLab – 04/June/2010
Identify p, K and p
from 2 to >12 GeV/c 5.5 GeV K+
C4F10 gas
REAL DATA from NIMA 479 (2002) 511
Cisbani / HERMES RICH
14.6 GeV e-
1.5 GeV p-
aerogel
Two radiators: aerogel and gas
PMTs as photon detector gas
Focusing Optics
Reference: NIMA 479 (2002) 511-530 3
HERMES RICH module layout
EIC Detector – JLab – 04/June/2010
147
63
101
Cisbani / HERMES RICH
180
48
281 126
unit is cm
4
Radiators
EIC Detector – JLab – 04/June/2010
Aerogel
Dirk Rickbosch – DESY07
(Absorb otherwise randomly
reflected photons)
Cisbani / HERMES RICH
(cut photons with l5GeV) plot vs day
4
1
Cisbani / HERMES RICH EIC Detector – JLab – 04/June/2010
average n (e+>5GeV)
EIC Detector – JLab – 04/June/2010
Dn ~
0.0003
Cisbani / HERMES RICH
Dn ~
0.0003
Dn ≈ 3 *10-4 in 10 years!
Dn ≈ 1*10-4 in the last 5 years! 1
5
one RICH module preserved @ UVa (thanks to G. Cates)
EIC Detector – JLab – 04/June/2010
HERMES
RICH
Cisbani / HERMES RICH
Aerogel Spare
Now stored at UVa under safe/controlled conditions + additional wall of spare 1
Aerogel from the other module. 6
EIC Detector – JLab – 04/June/2010
SIDIS (Cond. appr. Exp.): Setup and parameters
e+3He→e’+p(K)+X
BB: e-arm at 30o
= 45 msr
GEM Tracker
Gas Cherenkov
Shower
Cisbani / HERMES RICH
GMn/PR-09-019
SBS: h-arm at 14o
= 50 msr
GEM tracker
excellent PID / RICH
Hadron CALO
Event rate: ~104×HERMES
Beam: 50 mA, E=8.8 and 11 GeV (80% long. Pol.) 60 days of production
Target: 65% polarized 3He GEn(2)/PR-09-016 expected stat. accuracy:
Luminosity: 1.4×1037 cm-2s-1 10*better than HERMES on 1
7
proton
HERMES RICH in SBS (SIDIS Exp.)
(old GEM setup)
8
1
Cisbani / HERMES RICH EIC Detector – JLab – 04/June/2010
RICH detector in CLAS12
EIC Detector – JLab – 04/June/2010
Main Requirements:
1. separation up to 8 GeV/c
2. from 5 to 40 degree polar angle
3. p/K rejection>100 (<1% p contamination)
4. minimize material budget
Substitute 2 LTCC sectors with a RICH detector
Possible option: aerogel + SiPM (with time
correlation) RICH
Cisbani / HERMES RICH
GeV
1 2 3 4 5 6 7 8 9 10
/c
TOF
p/K LTCC
HTCC
TOF
p/p LTCC
HTCC
TOF
K/p LTCC ratio K/p ~ 0.1-0.15 1
9
From. M. Contalbrigo
Aerogel characteristics improvements
EIC Detector – JLab – 04/June/2010
Cisbani / HERMES RICH
2005 IEEE Nuclear Science Symposium Conference Record
M. Tabata et al.
2
0
EIC Detector – JLab – 04/June/2010
Aerogel RICH with 2 x mirrors
35o
Proximity between 5 and 10
degree 25o
Focusing
Mirrors acts at polar angle mirror 20o
above 10 degree Photon
detectors
10o
Target 5o
Beam
Doubled detector area
Cisbani / HERMES RICH
Focusing mirrors to reduce
detector area to ~ 2 m2/sec
Relax performance requests
for the external half (lower p)
Increase pad size
Reduce channel number
Standard PMTs
Similar to i.e. LHC-b !!! 2
1
From. M. Contalbrigo
EIC Detector – JLab – 04/June/2010
Aerogel RICH with mirror & semi-reflective layer
35o
25o
Proximity up to 15 degree
20o
Mirror above 15 degree
10o
Target 5o
High density of hits Semi-reflective Beam
check with track multiplicity mirror
Cisbani / HERMES RICH
Photon
detector
Too high absorption in aerogel
semi-reflective mirror
Reduced collection efficiency
(bi-alcali q.e. 25 %)
ultra bi-alcali q.e. 45 %
cost increases by 50 %
New concept !!!
2
2
From. M. Contalbrigo
Summary
EIC Detector – JLab – 04/June/2010
• HERMES RICH designed and built in ~2 years
– Configuration: Mirror Focusing, dual radiator, with PMT readout
– First RICH using aerogel radiator in a real experiment
– Very stable performance in 10 years
• HERMES RICH “inheritance”:
– H-RICH for SIDIS physics in SBS/Hall A
– CLAS12 p-K-p PID detector (work in progress!)
Cisbani / HERMES RICH
• Presently available improvements (at reasonable price):
– Better aerogel (higher transmission and reduced scattering)
– Smaller photon detectors: multianode PMTs, SiPM (with time
information)
– Improved mirrors
2
Recent RICH 2010 conference: http://rich2010.in2p3.fr/ 3