HYP03 Future Hypernuclear Program at Jlab Hall C Satoshi N. Nakamura Tohoku University 18 th Oct 2003, JLab.

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Presentation transcript:

HYP03 Future Hypernuclear Program at Jlab Hall C Satoshi N. Nakamura Tohoku University 18 th Oct 2003, JLab

HYP03 18th October 2003 S N Nakamura for E collaboration The (e,e’K + ) reaction for hypernuclear spectroscopy Large angular momentum transfer Spin-flip amplitude New Hypernuclei (Mirror, Neutron Rich) Various multiplet states Detailed information on the hypernuclear structure Proton to  Higher energy resolution

HYP03 18th October 2003 S N Nakamura for E collaboration The first (e,e’K + ) hypernuclear experiment (E89-009) Demonstrated that the (e,e’K) hypernuclear spectroscopy is possible! 12 C(e,e’K + ) 12  B PRL 90 (2003) , E Result Good energy resolution 900 keV (FWHM) The best hypernuclear energy resolution achieved by the reaction spectroscopy ss pp

HYP03 18th October 2003 S N Nakamura for E collaboration General experimental condition Virual Photon energy E   1.5 GeV Beam energy E e ~ 1.8 GeV e’ momentum E e’ ~E e -E    GeV Kaon momentum p K E  determines p K = 1.05 ~1.35 GeV/c Lower p K : Better resolution, particle ID σ total (  b) E γ (GeV) p( ,K + )  Total cross section Phys. Lett. B 445, 20 (1998) M. Q. Tran et al. As low as possible momenta (p e,p e’,p k )  Better energy resolution  Avoid unnecessary reaction channels

HYP03 18th October 2003 S N Nakamura for E collaboration Improvement of the E experiment Energy resolution as well as acceptance are limited by the kaon spectrometer Zero degree tagging method to maximize virtual photon flux Severe background from electrons associated with Bremsstrahlung (200 MHz for e ’ arm) Tilt Method New Spectrometer High resolution Kaon Spectrometer (HKS) New Experiment was approved by Jlab PAC19 E (Spokesmen: Hashimoto, Tang, Reinhold, Nakamura)

HYP03 18th October 2003 S N Nakamura for E collaboration New kaon spectrometer and Jlab E setup

HYP03 18th October 2003 S N Nakamura for E collaboration Jlab E setup plan

HYP03 18th October 2003 S N Nakamura for E collaboration Tilt method  The scattered electrons to be measured are associated with the virtual photons  The most serious background source is the electron associated with the bremsstrahlung Optimize the detection angle for the scattered electrons: Improve S/N drastically, Reduce e ’ s rate Virtual photon loss : higher beam intensity and thicker target Spectroscopy of the medium-heavy hypernuclei Very forward Hyper forward!

HYP03 18th October 2003 S N Nakamura for E collaboration Optimization of the tilt angle of the scattered electron spectrometer  Virtual Photon  Electron Background due to Bremsstrhalung  M  ller Scattering

HYP03 18th October 2003 S N Nakamura for E collaboration  Virtual Photon  Electron Background due to Bremsstrhalung  M  ller Scattering Tilt the electron detector by 8 degrees (  ~4 deg). ~5 times thicker target, ~50 times stronger e beam

HYP03 18th October 2003 S N Nakamura for E collaboration High resolution Kaon Spectrometer ConfigurationQ + Q + D Central Momentum1.2 GeV/c Dispersion4.7 cm/% Momentum Resolution2 x (FWHM) Solid Angle30 msr (w/o Splitter) 16 msr (w/ Splitter) K + detection angle1 ~ 13 degrees Angular Acceptance 170mrad (V),180 mrad(H) Momentum Acceptance 12.5% Max. Magnetic Field1.6 T (Normal)

HYP03 18th October 2003 S N Nakamura for E collaboration HKS magnets HKS magnets are on the way to JLab.

HYP03 18th October 2003 S N Nakamura for E collaboration Characteristics of E  From light to medium-heavy hypernuclei –Single particle nature of  in heavier hypernuclei –Core excited states –Spin-Orbit splitting Heavier targetSevierer (Z 2 ) Brems. BG Tilt Method

HYP03 18th October 2003 S N Nakamura for E collaboration Characteristics of E  Large angular acceptance (1~13deg) of HKS –Angular dependence of the hypernuclear states DWIA calculation by the code of M.Sotona Angular distribution of 12  B states (p3/2) -1 (p3/2)  3 + (s1/2) -1 (p1/2)  2 - (p3/2) -1 (s1/2)  2 - (s1/2) -1 (s1/2)  1 +

HYP03 18th October 2003 S N Nakamura for E collaboration Singles rates for E Target HKSENGE e + (Hz)  + (kHz) K + (kHz) p (kHz) e - (kHz)  - (kHz) 12 C Si V I e = 30  A, 100 mg/cm 2 Scattered electron rate is 200 times lower than E Pion and proton rates of the kaon arm are high High rejection efficiencies of Cherenkov counters for pions and protons Aerogel and Water Cerenkov counters

HYP03 18th October 2003 S N Nakamura for E collaboration Detector R&D TOF counters (resolution: 60 ps FWHM) Aerogel Cherenkov (n=1.05, for  w/3 layers) Water Cherenkov (n=1.33, 4x10 -4 for p w/ 2 layers) Drift Chamber for Kaon arm (SOS type) Drift Chamber (honeycomb cell) for e’ Scintillator Hodoscopes (50 segments x 2 layers)

HYP03 18th October 2003 S N Nakamura for E collaboration Counters’ performance test Aerogel C Water C HKS TOF Enge TOF KEK PS T1:1.05~1.35 GeV/c p,K, 

HYP03 18th October 2003 S N Nakamura for E collaboration EDC Test Beam at LNS-Tohoku  Tagged photon from 1.2GeV Stretcher Booster Ring ( Nov. ‘02)  Converted e + e - pair was used for EDC test

HYP03 18th October 2003 S N Nakamura for E collaboration Detectors were assembled and checked at JLab EEL building

HYP03 18th October 2003 S N Nakamura for E collaboration Yield comparison between E and E ItemE01-011E Gain factor Virtual photon flux per electron(x ) Target thickness(mg/cm 2 ) e’momentum acceptance and e’- K + momenta matching Kaon survival rate Solid angle of K arm (msr) Beam current(  A) Estimated yield ( 12  B gr :counts/h) (measured) 50 For d  d  (gr) = 140 nb/sr

HYP03 18th October 2003 S N Nakamura for E collaboration Expected Energy Resolution ItemContribution to the resolution (keV, FWHM) Target 12 C 28 Si 51 V 89 Y HKS momentum230 Beam momentum< 180 Enge momentum120 K + angle Target thickness< 180< 171< 148< 138 Overall< 390< 360< 350< 345

HYP03 18th October 2003 S N Nakamura for E collaboration Expected Spectra KEK-PS E336 : w/ SKS ( ,K) reaction Jlab E (e,e ’ K) Jlab E (e,e’K) [Expected]

HYP03 18th October 2003 S N Nakamura for E collaboration Summary  The (e,e’K) reaction = new and interesting  E = Best energy resolution (900keV) for reaction hypernuclear spectroscopy  With the tilt method and HKS, the E aims : Energy resolution by a factor of 2~3, S/N by a factor of ~10, hypernuclei yield by a factor of 50. From light to mid-heavy hypernuclei( 7 Li, 12 C, 28 Si, 10 B, 11 B, 51 V, 89 Y,…)  HKS magnets and detectors are completed. First beamtime is expected in 2004.

HYP03 18th October 2003 S N Nakamura for E collaboration