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Challenges and Opportunities of High Luminosity Tracking Charles Hyde Université Blaise Pascal, and Old Dominion University « Structure of the Nucleon » GDR Instrumentation Workshop 8-9 April 2008, CEA-Saclay
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Deeply Virtual Exclusive Reactions Small cross sections at high Q 2. –High luminosity Competition between exclusive and inclusive channels –Tracking and/or particle ID Complicated spin structure –Target and/or recoil spin observables Plus charge- exchange reations
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Luminosity Limits Beam Current –All JLab Deeply Virtual experiments operate below available beam limits. –Single exception is Hall C H(e,e’ + )n « Pion Form Factor » Polarized Targets Detector / Tracking – Occupancy, – Ageing. DAQ
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Polarized Targets Hall A, 3 He, –neutron luminosity = 10 36 –Proton + window Luminosity ≈ (2+6)10 36 –Secondary Luminosity ≈ 210 37 –Recent discussion to boost luminosity by 10x to 100x –Free rotation of long. and transverse polarization Hall B, NH 3, ND 3 Longitudinally polarized –Dilution factor ≈ 0.05 –CLAS Luminosity 10 34 –CLAS12 Luminosity = 10 35 –Hall C target operated at 100nA with transverse pol. HD Targets –Low Holding Field: Preferred for Transverse Pol. –Maximum Luminosity Acceptance TBD.
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Detector Limits CLAS DC –2% maximum “safe” occupancy level for high efficiency track reconstruction Probably a good general limit. Drift Chamber rate limits: –HV trips, Ageing, Recovery time after each event –GEM / MicroMegas: extend operating limits by orders of magnitude Does not resolve occupancy problem unless granularity is increased Si tracking: –High Granularity Hall A PbF 2 blocks expected to diminish light output by 20% after 7 days at 410 37 /cm 2 /s –Cure with blue light ≈ 1 day / week.
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DAQ Limits Open Trigger in open geometry –scattered electron; or –Electron + 1 charged particle –High raw data rates from DIS and photo-production limit rate for rare processes CLAS12 DAQ tuned to 10 35 with open (Q 2 >1 GeV 2 ?) trigger. Hall A DVCS: –DIS electrons (kHz) –>1GeV photon Coincidence rate 100 Hz at 410 37
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Specialized Triggers for Deeply Virtual Processes The deeply virtual ep ep and ep ep reactions have a special signature ≥90% of beam energy is visible in two EM showers For one shower is really 2 closely spaced showers. Each of the two showers has ≥ 30% of beam energy. Possibility of operating at higher luminosity Tracking detectors must still operate at high efficiency A pre-scaled Open Trigger can still provide access to other channels at close to normal count rates.
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Photon Background in e+H 2 Two dominant process (X/X 0 <1%) Quasi-real bremsstrahlung followed by e Compton Scattering Møller (e,e’) scattering followed by internal bremsstrahlung (e, ) cross sections O ( r e 2 ) Compton/Møller edge at E =m e /(1-cos ) Pavel Degtiarenko: DINREG
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Bremsstrahlung Compton Model Excellent agreement for naïve estimate
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Energy Integrated; Angle Averaged Bremsstrahlung endpoint is too hard
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Can Drift Chambers be Shielded against random X-ray and -ray hits? e+H photon background spectra are ≈ 1/ E for 0.1 MeV< E <m/(1-cos ) –P. Degtiarenko, DINRAD MC –Everything above 13 eV is “high energy” from H Photo-absorption E >>1 MeV is universal Z(Z+1)/A and dominated by e + e creation Photo-absorption at E ≈1MeV is universal Z/A and dominated by Compton Scattering on atomic electrons Photo-absorption << 1 MeV is atom specific
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Photo-Conversion in Drift Chamber gas If photon spectrum is ≈1/E , then equal numbers of photons per decade –(10-100KeV, 100KeV-1MeV, 1MeV-10MeV, etc). But, low energy -rays are preferentially converted in chamber gas 5 KeV photon: 1000x greater conversion probability than 10MeV photon ≈MIP signal
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Photon Attenuation Thin multi-Z sandwich –Preferentially absorb low energy -rays –Multi-layer, multi-Z to absorb secondary K-shell X-rays etc. physics.nist.gov/PhysRefData/Xcom/Text/XCOM.html
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Gamma-Shield Concept Thin multi-Z sandwich can preferentially absorb low energy -rays with only 1% radiation length (1mr multiple scattering at 1.5 GeV/c) target DC
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Photon Conversion in Unshielded Chamber Background -flux is ≈1/E –Arbitrary units Photon conversion probability in 1cm Chamber gas Relative hit rate is semi-dominated by low-energy -rays
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Absorption in 1% multi-Z sandwich Background -flux is ≈1/E –Arbitrary units Attenuation coef (cm 2 /g) in 1% radiation length multi-Z absorber Transmission coef. of absorber Transmitted -ray flux. – Photons below 50KeV strongly absorbed
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Random hits in DC after 1% radiator multi-Z sandwich -flux with and without multi-Z absorber –Left hand axis conversion rate with and without absorber –Right hand axis -ray background spectrum is strongly cut-off at high energy –E <m/(1-cos ) –20deg E <8 MeV
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Recoil Tracking for DVCS H(e,e’ p) –Over-complete exclusivity A(e,e’ A) –Nuclear recoil detection required for exclusivity –D(e,e’ D) CLAS (M. Amarian et al, deferred) – 4 He(e,e’ ) CLAS+BONUS H(e,e’ p) Recoil Polarization –Alternative to target polarization.
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Acceptance vs. Luminosity CLAS12: (e,e’ )Acceptance Luminosity ( L ) ≈ 0.5 10 35 –Large t-range –All [Q 2,x B ] bins; unequal statistics –Physics luminosity ≈10x lower for polarized targets For an equivalent single [Q 2,x B ] bin –Hall A azimuthal acceptance V HRS /sin( ) ≈ (120mr)/sin(20 ) ≈ 0.6rad –(e,e’ )Acc. L ≈ (0.6/2 ) 410 37 (0.6/2 ) ≈ 410 36 Hz/cm 2 t/Q2<<1 Each [Q 2,x B ] requires separate beam time balance statistics –Is it possible to build a large acceptance recoil tracker for ≥ 10 37 luminosity in Hall A?
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Recoil Tracking at L ≥ 10 37 ? Separate GPDs via recoil polarization –FOM (500MeV/c < p < 700MeV/c) ≥0.5% –Hall A: L Acc. FOM ≥ 210 34 Hz/cm 2 –CLAS12 polarized target: p L FOM= Dilution P 2 ≈ 5% L Acc. dilution P 2 ≈ 10 35 (0.5) (0.05) ≈ 2.510 33 Hz/cm 2 Nuclear DVCS –D(e,e’ D) –Recoil deuterons are >5x minimum ionizing Raise detection threshold to suppress single hits Granularity can be increased to keep random hit rate below 2%. –Si strips of 250 m 5cm at 20 cm from target.
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Recoil Polarimeter Concept
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LANL LDRD R&D proposal for high luminosity tracking Four layer Si Tracker –5cm 225mm strips –2000 total channels –LHCb “Beetle” readout chip Measure D(e,e d) coherent cross section at t min at [Q 2,x B ]=[1.9GeV 2,0.36] during E08-025 (2010). –Test occupancy, tracking efficiency. A. Klein, G. Kunde, A. Dangoulian
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Conclusions DVCS offers compelling physics for tracking beyond current luminosity limits –[BABAR≈10 34, CLAS12 proposed 10 35 ] Low level triggers on total EM energy can keep DAQ rate within limits. In situ tests of prototype trackers needed to determine actual limits.
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LANL LDRD Proposal R&D for high luminosity tracking Si -Strips 2.54 cm C (analyzer) HRSe’
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