X. Zheng, June 2010, JLab Hall A/C Polarized Target Workshop 1/20 Measurement of the Neutron Spin Asymmetry A 1 n using HMS+SHMS at 12 GeV – Physics Motivation.

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Presentation transcript:

X. Zheng, June 2010, JLab Hall A/C Polarized Target Workshop 1/20 Measurement of the Neutron Spin Asymmetry A 1 n using HMS+SHMS at 12 GeV – Physics Motivation – A 1 n measurements at JLab 6 GeV in Hall A in 2001 – Proposal for the A 1 n measurement with HMS+SHMS (2010 vs versions) – Summary Xiaochao Zheng Univ. of Virginia June 17, 2010

X. Zheng, June 2010, JLab Hall A/C Polarized Target Workshop 2/20 Success of the Standard Model QCD tested in the high energy (perturbative) region Standard Model of Particle Physics (Strong Interaction Sector) within Major Challenges within the Standard Model Understand and test QCD in extreme conditions (RHIC, LHC) energy (GeV) (~1/distance) aSaS Understand and test QCD in “strong” interaction region (non- perturbative) Understand the nucleon structure, how quarks and gluons form the nucleon's mass, momentum, and spin

X. Zheng, June 2010, JLab Hall A/C Polarized Target Workshop 3/20 Data vs. Theory – How do we test QCD? For most cases, QCD cannot predict (be used to calculate) the value of structure functions because of their non-perturbative nature. However, there are a couple of exceptions: F 2 p /F 2 n and d/u at large x A 1 p, A 1 n, or Du/u and Dd/d at large x At large Q 2, A 1 has only weak-dependence on Q 2 (g 1 and F 1 follow the same LO and NLO evolutions, but not in higher orders or higher twists). Virtual photon asymmetry:.at large Q 2

X. Zheng, June 2010, JLab Hall A/C Polarized Target Workshop 4/20 Why Large x? At large x, valence quarks dominate, easier to model; Less contribution from q-qbar sea and gluons — a relatively clean region to study the nucleon structure; To understand the nucleon spin, high x is a good place to start with.

X. Zheng, June 2010, JLab Hall A/C Polarized Target Workshop 5/20 Predictions for A 1 and  q/q at large x The only place QCD can make absolute predictions for structure functions.

X. Zheng, June 2010, JLab Hall A/C Polarized Target Workshop 6/20 The 6 GeV Hall A Measurement (21 PAC days, 2001) X. Zheng et al., Phys. Rev. Lett. 92, (2004); Phys. Rev. C 70, (2004) HHC not valid quark OAM?

X. Zheng, June 2010, JLab Hall A/C Polarized Target Workshop 7/20 Polarized DIS and Nucleon Spin Structure H. Avakian, S. Brodsky, A. Deur, F. Yuan, Phys. Rev. Lett.99:082001(2007) Figure credit: A. Deur (DIS only)

X. Zheng, June 2010, JLab Hall A/C Polarized Target Workshop 8/20 Polarized DIS and Nucleon Spin Structure The JLab Hall A data were quoted by the 2007 NSAC long range plan as one of the “most important accomplishments since the 2002 LRP”; flag-ship Extensions of these measurements are flag-ship experiments for JLab 11 GeV. H. Avakian, S. Brodsky, A. Deur, F. Yuan, Phys. Rev. Lett.99:082001(2007) Figure credit: A. Deur (DIS only)

X. Zheng, June 2010, JLab Hall A/C Polarized Target Workshop 9/20 Original Proposal for PAC-30 (Conditionally approved) Measured A 1 n in DIS from using 12 GeV polarized e - beam, P beam =80% (dP/P=1% Compton, Moller) Polarized 3 He target, hybrid pumping, 40cm, o C, P Targ =50% (dP/P = 3%) — (GEn E has achieved 55% in beam) HMS+SHMS to detect e', measure both A ll and A  : ppn Total: 1908h (79 days) + Target Installation Will reach DA 1 n =±0.071(stat) ±0.032(syst) at x=0.77

X. Zheng, June 2010, JLab Hall A/C Polarized Target Workshop 10/20 Improvements on the Polarized 3He Target (2010) Will use the same design as GEN-II (11 GeV): use of alkali-hybrid mixtures to increase the spin-exchange efficiency; use of narrow-lined high-power diode lasers; study of polarimetries for both 3He and alkali-metal vapor and their densities to improve understanding of the target performance; use of convection to overcome beam and other depolarization effects; metal-based target chamber to resist radiations and avoid cell rupture; Goal: a 60-cm long target chamber, 12 amg density, up to 60uA beam with 60% polarization Overall, provide a factor of 8 improvement in luminosity! allow the use of less beam time to achieve higher precision (now set statistical uncertainty = systematic at x=0.77) added resonance measurements (with little extra beam time)

X. Zheng, June 2010, JLab Hall A/C Polarized Target Workshop 11/20 Kinematics Production (DIS and resonance) Elastic e- 3 He(ll) and D(1232) (  ) at low Q 2 to check P b P t and beam helicity: 10 4 :1 p rejection is needed

X. Zheng, June 2010, JLab Hall A/C Polarized Target Workshop 12/20 Other Inputs: F 2 p, F 2 D – NMC fits and MRST/CTEQ Uncertainty on Pp expected to reduce by factor of 4 from Hall A Ax and Az measurements; R(x,Q 2 ) – R1998, PLB 452, 194 (1999) EMC for F 2 3He, F 2 D Acta Phys.Polon. B27, 1407 (1996) ( nucl-th/ ) A 1 p – from fit to world data (at large x also consistent with CLAS12 expected results) Phys. Rev. C 70, (2004) From 3 He to Neutron S, S', D, D isobar in 3 He wavefunction: Phys. Rev. C65, (2002) dominant for high x

X. Zheng, June 2010, JLab Hall A/C Polarized Target Workshop 13/20 Projected A 1 n Uncertainties DIS Resonance

X. Zheng, June 2010, JLab Hall A/C Polarized Target Workshop 14/20 Expected Results

X. Zheng, June 2010, JLab Hall A/C Polarized Target Workshop 15/20 Expected Results

X. Zheng, June 2010, JLab Hall A/C Polarized Target Workshop 16/20 Beam Time Request Production: 684 hours Commissioning: 3 days if not including the target, longer if include target. Elastic; D(1232); Reference Cell (N 2 run) Configuration changes; Beam pass change; Moller; Target polarimetry; Total: 843h (35 days) + Target Installation, ~45% of our 2006 request

X. Zheng, June 2010, JLab Hall A/C Polarized Target Workshop 17/20 Expected Results Combined results from Hall A (neutron) and B (proton) 11 GeV experiments

X. Zheng, June 2010, JLab Hall A/C Polarized Target Workshop 18/20 Complementarity with the Hall A BigBite Proposal The current version of Hall A proposal uses the BigBite spectrometer, will provide DIS data up to x=0.71 with a 8.8 GeV beam, with smaller uncertainties than this proposal. It is unknown yet whether it will work for 11 GeV; Even if BigBite works for 11 GeV, it will be limited by systematics at x=0.77. And The physics of A 1 n at large x is important enough that it's worth more than one measurement; A combination of the Hall A and C measurement will allow the study of the Q2-dependence of A 1 n up to x=0.71. The use of HMS+SHMS (close spectrometers) will allow clean measurements of A 1 n with less systematics than open spectrometers. As a result, reliable and fast online and/or offline data analysis will be possible, allowing fast turn-out of physics results. condition of PAC30

X. Zheng, June 2010, JLab Hall A/C Polarized Target Workshop 19/20 Summary Will measure A 1 n up to x=0.77 in DIS, test of CQM, pQCD and the role of quark OAM; Wide Q 2 coverage allows the study of Q 2 -dependence up to x=0.55; Requires: pol3He target in Hall C + SHMS + HMS w/ 10 4 :1 p rejection; Compare to the 2006 version: Added resonance data to test quark-hadron duality; Recent development in the target allows significant reduction of the beam time and increased physics outcome. Beam time request: 35 days total (not including target commissioning) Complementary to the Hall A BigBite proposal, Use of HMS/SHMS spectrometers allows clean studies of A 1 n and fast offline (even online) analysis; Will combine with CLAS12 proton data to extract Dq/q; provide further tests of predictions.

X. Zheng, June 2010, JLab Hall A/C Polarized Target Workshop 20/20 Frontiers of Nuclear Science (1) QCD and its implications and predictions for the state of matter in the early universe, quark confinement, the role of gluons, and the structure of the proton and neutron; “Building on the foundation of the recent past, nuclear science is focused on three broad but highly related research frontiers: (1) QCD and its implications and predictions for the state of matter in the early universe, quark confinement, the role of gluons, and the structure of the proton and neutron; (2) the structure of atomic nuclei and nuclear astrophysics, which addresses the origin of the elements, the structure and limits of nuclei, and the evolution of the cosmos; and (3) developing a New Standard Model of nature's fundamental interactions, and understanding its implications for the origin of matter and the properties of neutrinos and nuclei.”

X. Zheng, June 2010, JLab Hall A/C Polarized Target Workshop 21/20 Extra slides

X. Zheng, June 2010, JLab Hall A/C Polarized Target Workshop 22/20 to Major Challenges to the Standard Model Higgs mechanism yet to be tested (observed); Cannot explain the observed non-zero mass of n's; Does not include gravity, neither does it explain dark matter/energy; Requires too many parameters; Conceptually, there is always “room” for New Physics. Parity violation in lepton/electron scattering can help to test the Standard Model by looking for “signs” of new physics.

X. Zheng, June 2010, JLab Hall A/C Polarized Target Workshop 23/20 Nucleon Spin Structure in the Valence Quark Region

X. Zheng, June 2010, JLab Hall A/C Polarized Target Workshop 24/20 Polarized DIS and Nucleon Spin Structure Will pQCD predictions (with quark OAM) work? H. Avakian, S. Brodsky, A. Deur, F. Yuan, Phys. Rev. Lett.99:082001(2007) Figure credit: A. Deur (DIS only) extracted from A 1 data

X. Zheng, June 2010, JLab Hall A/C Polarized Target Workshop 25/20 A 1 n in the Valence Quark Region at JLab 11 GeV To be rated August 2010 Hall A PR : approved Hall C: PR : conditionally approved Hall A+SOLID: to be proposed

X. Zheng, June 2010, JLab Hall A/C Polarized Target Workshop 26/20 A 1 p at 11 GeV