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E01-011 Analysis update Adjust of the Splitter-HKS Side. Yuncheng Han May 09, 2012 Hampton University JLab hypernuclear collaboration meeting. Outline. Overview of the E01-011 experiment Principle of the forward optics tune Methods of the optical matrix modification
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E01-011 Analysis updateAdjust of the Splitter-HKS Side Yuncheng Han May 09, 2012 Hampton University JLabhypernuclear collaboration meeting
Outline • Overview of the E01-011 experiment • Principle of the forward optics tune • Methods of the optical matrix modification • Further optimize the optical matrices from focal plane to sieve slit plane • Status using the new optical matrices
Overview of the E01-011 Experiment Carried out at JLab in 2005, to obtain high resolution, high yield rates hypernuclear spectroscopy, for study of hyperon-nucleon interaction. e’ Target N e /0 γ* p K+ e + p → / 0+ e’+ K+ e + N → N+ e’+ K+ Three generations : E89-009 (2000), E01-011 (2005), E05-115(2009)
-6.730.020.2 MeV The Results of E01-011 Experiment HKS JLAB 28Al d p 7He s Counts (150 keV/bin) 7He: 1st time w/ high statistics; BΛ and feature confirmed; Paper drafted: n-halo state, CSB. FWHM ~500 keV 28Al :1st medium-heavy hyper-nuclear spectrum w/ clear s-, p-, d-shell state peaks; space of s- and p- shell states 1~2 MeV wider but p- and d- shell states ~1 MeV narrower than expected 12B B (MeV) 12B : consistent of JLab E89-009; much better resolution.
The Status of E01-011 Experiment • Data analysis was already done, 7He, 12B, 28Al; • However, the splitter magnet actual current in this exp was 8.5 % bigger than the designed value, which made the real optics different a lot from the designed one. The previous analysis used the designed optics as an initial, and relying on mathematical method (nonlinear χ2fit ) for optimization; • Freedom of the mathematical tune is large (1260 elements in the optics matrices), so the reliability of the final results was not solid; • Since the fringe field near the splitter magnet region introduce asymmetry to the magnetic field map, a better optics can be gotten if consider the asymmetry.
Previous analysis method Field map Backward tune Nonlinear least χ2 fitting kinematical scan Geant3 Exp.data Final matrices Initial optics matrices Λ-hypernuclear spectroscopy CH2 data Tuned matrices Λ &Σ0mass spectroscopy Kinematics: masses and emit angles of Λ & Σ0 Mathematical tune of optics matrices
New Analysis method Qualifications of A, B and C Magnetic field study Field map Geant3 simulation Sim focal plane distribution A B Reconstructed sieve slit distri Exp data Exp focal plane distribution Optical matrices C Sieve slit geometry Mass/angle independence Calculated Λ/Σ spectroscopy
Relationship between sieve slit and focal plane Sieve Slit Focal Plane Target Q1-Q2-Dipole Splitter K+
Strategy of introduce new optics • New optical matrices was introduced to satisfy • Focal plane distribution sim match exp data • Reconstructed sieve slit distribution match • real sieve slit geometry • Calculated masses independent on • kinematical parameters of kaons (p, X’, Y’) • New optical matrices was gotten by • Introduce asymmetry function to • the magnetic field map • offset of the field map geometry • Adjust position of focal plane Sieve Slit Focal Plane Target Q1-Q2-Dipole Splitter K+ Focal plane position 235 cm to 265 cm Chambers’ distance 100 cm to 36 cm
Comparison of focal plane/sieve slit distribution • FP Y-X • Sieve Slit FP X’-X W/ initial optical matrices W/ new optical matrices
Comparison of mass dependence on kinematics • W/ initial optical matrices W/ new optical matrices
Further optimize the optical matrices Region of one hole Center of the hole (X-X0)2 + (Y-Y0)2 < R2 (X0,Y0)
Comparison of Λ/0mass spectrum Mathematical method (nonlinear least χ2fit ) • W/ initial optical matrices W/ new optical matrices
Comparison of 12B mass spectrum 12B Δ ~ 10.97 MeV Δ ~ 10.79 MeV Δ ~ 11.05 MeV Δ ~ 11.64 MeV
Summary • E01-011 experiment was carried out in 2005 at JLab, analysis was already done, 7He, 12B, 28Al; • Initial optical matrices was poor, by introduce scaling asymmetry function, offset field map geometry, and adjust position of focal plane, new optical matrices for Splitter-HKS side was obtained; • Quality of Λ/0 spectrum w/ new optical matrices is already comparable of previous finalized results; • 12B mass spectrum was checkedw/ new optical matrices ; • New optical matrices for electron arm will be tune soon • More reliable and higher quality results are expected with the new optical matrices (for both electron arm and kaon arm) and the powerful nonlinear least χ2fit mathematical tune.