Parity Violating Deep-Inelastic Scattering Jian-ping Chen, Jefferson Lab for the JLab SoLID collaboration Lanzhou Workshop, July 31 - August 1, 2009 Introduction Physics potential of PVDIS Test of Standard Model Precision study of hadronic properties: •Charge symmetry violation (CSR) •Higher twist •Parton distributions d/u at high x • Experimental Setup and Plan • Acknowledgements: E. Chudakov, P. Souder, X. Zheng … Interactions and Structure • Standard Model: EM and Weak (Electro-weak) Interactions well understood Strong Interaction, difficult at low energy (nucleon scale) • Nucleon and nuclear structure mainly due to strong interaction • EM or weak interaction clean probe to study nucleon/nuclear structure • Search for new physics beyond the Standard Model Look for deviations from Standard Model Often try to avoid complications from structure Weak Neutral Current (WNC) Interactions Low energy Weak NC interactions (Q2<<MZ2) Z0 Historical Context: • 1960s: An Electroweak Model of Leptons (and quarks) • SU(2)L X U(1)Y gauge theory predicted the Z boson • 1973: antineutrino-electron scattering • First weak neutral current observation • Mid-70s: Does the Weak Neutral Current interfere with the Electromagnetic Current? • Central to establishing SU(2)L X U(1)Y Parity is conserved Consider fixed target electron scattering Parity is violated First Electron Parity Experiment APV in Deep Inelastic Scattering off liquid Deuterium: Q2 ~ 1 (GeV)2 APV ~ 104 Q2 (GeV2) This experiment convinced the world that the Z-boson violated parity •Cleanly observed weak-electromagnetic interference •sin2W = 0.224 ± 0.020: same as in neutrino scattering •Established experimental technique: (APV) < 10 ppm Electroweak Interaction – The Standard Model Mixing of the SU(2)L and UEM(1)g is giving by the Weak Mixing angle sin W A B cosW W3 sin W ( m 0) Z B sin W W3 cosW ( m 0) Electron and quark neutral currents are given by vector and axial couplings In the Standard Model NC J NC J 1 e (e) ueg ( gV g Ae g 5 )ue 2 1 q (q ) uqg ( gV g Aq g 5 )uq 2 Fermions nA, n e- , u, c d, s gAf 1 2 1 2 1 2 1 2 g Vf 1 2 1 sin 2 W 2 1 4 2 sin W 2 3 1 2 sin 2 W 2 3 PV Electron Scattering on Hadron (gAegVT + gVegAT) •The couplings depend on electroweak physics as well as on the weak vector and axial-vector hadronic current •Both new physics at high energy scales as well as interesting features of hadronic structure come into play •A program with many targets and a broad kinematic range can untangle the physics Electron-Quark Phenomenology A V V A Moller PV is insensitive to the Cij C1u and C1d will be determined to high precision by Qweak, APV Cs C2u and C2d are small and poorly known: one combination can be accessed in PV DIS New physics such as compositeness, leptoquarks: Deviations to C2u and C2d might be fractionally large Deep Inelastic Scattering e- eZ* g* X N APV GF Q 2 a(x) Y (y) b(x) 2 y 1 E / E C Q f (x) a(x) = Q f (x) + 1i i i 2 + i i fi fi f i i i a(x) and b(x) contain quark distribution functions fi(x) C Q f (x) b(x) Q f (x) 2i i i i 2 i i i at high x For an isoscalar target like 2H, structure functions largely cancel in the ratio at high x 3 0.62s a(x) (2C1u C1d ) 1 10 u d At high x, APV becomes independent of x, W, with well-defined SM prediction for Q2 and y 0 3 uv dv b(x) (2C2u C2d ) 10 u d C2q inaccessible in elastic scattering 1 PVDIS at High x 2C2u C2d ~ 0.14 2C1u C1d 0.5% fractional precision on the asymmetry is needed! APV APV ~ 0.5% 2C2u C2d 2C2u C2d ~ 5% Feasible (in narrow kinematics) with existing JLab spectrometers. JLab 6 GeV experiment: scheduled to run in Hall A Oct.-Dec., 2009 Spokespersons: Michaels, Reimer, Zheng PhD Students: X. Deng, K. Pan, D. Wang JLab 11 GeV proposal: Conditional approval Spokespersons: Paschke, Reimer, Zheng • Experimental systematic errors challenging • Averaged over large Q2, W, and x range Hall C HMS / SHMS spectrometers PVDIS with SoLID • Solenoid (from BaBar, CDF or CLEOII) contains low energy backgrounds trajectories measured after baffles • Fast tracking, particle ID, calorimetry, and pipeline electronics • Precision polarimetry (0.4%) • • • • • • High Luminosity on LH2 & LD2 Better than 1% errors for small bins x-range 0.25-0.75 W2 > 4 GeV2 Q2 range a factor of 2 for each Moderate running times Statistical Errors (%) vs Kinematics For SOLID Spectrometer Error bar σA/A (%) shown at center of bins in Q2, x 4 months at 11 GeV 2 months at 6.6 GeV PAC34 Why do we need so many data points? • Possible new physics • New interactions • Charge symmetry violation (CSV) • Higher twist effects Like neutron beta decay experiments: many diverse physics topics Sensitivity: C1 and C2 Plots : 6 GeV E08-011 PDG best fit R. Young SAMPLE (combined) SLAC/ Prescott R. Young Cs APV (PVES) Qweak (expected) R. Young (combined) MIT/ Bates SLAC/Prescott Expected: JLab 6 GeV PV-DIS E08-011 12 GeV PVDIS Sensitivity: C1 and C2 Plots World’s data 6 GeV PVDIS Precision Data Qweak Cs PVDIS Search for CSV in PV DIS u (x) d (x)? p n d (x) u (x)? p n • u-d mass difference • electromagnetic effects u(x) u p (x) d n (x) d(x) d p (x) u n (x) •Direct observation of parton-level CSV would be very exciting! •Important implications for high energy collider pdfs •Could explain significant portion of the NuTeV anomaly For APV in electron-2H DIS: APV APV 0.28 u d ud Sensitivity will be further enhanced if u+d falls off more rapidly than u-d as x 1 CSV Theory and Data Londergan & Thomas, (also B. Ma) MRST PDF global with fit of CSV Martin, Roberts, Stirling, Thorne [Eur Phys J C35, 325 (04)]: Analytic calculation similar to global fit Sensitivity with PVDIS RCSV APV x APV x 0.28 u x d x u x d x Higher Twist • Deep-inelastic Scattering (DIS) structure functions, unpolarized and polarized. • Operator-product expansion (OPE) – twist expansion expansion in terms of power of 1/Q • Leading twist (twist-2): parton distributions another series in terms of s: LO, NLO, NNLO,… • Twist-3: quark-gluon correlations • Twist-4: quark-quark correlations Leading twist Higher twist Higher Twist in F2 Analysis of Blumlein and Botcher Higher twist is clearly seen at the PVDIS kinematics. What can we add? MRST Fits F2 (x,Q2)=F 2 (x)(1+D(x)/Q2) D/Q2min(%) D/Q2min(%) LO NNNLO 0.5 -14 2 0.003 1.0 -11 0.0 -.06 -0.001 1.7 -3.5 -0.5 0.4-0.5 .22 0.11 2.6 8 4 0.5-0.6 .85 0.39 3.8 22 10 0.6-0.7 2.6 1.4 5.8 45 24 0.7-0.8 7.3 4.4 9.4 78 47 x MRST, PLB582, 222 (04) Q2min=Q2(W=2) Q2=(W2-M2)/(1/x-1) D(x) D(x) LO NNNLO 0.1-0.2 -.007 0.001 0.2-0.3 -.11 0.3-0.4 Q2min APV=APV(1+C(x)/Q2) MRST fit of F2: order of DGLAP affects HT F2(x,Q2)=F2(x)(1+D(x)/Q2) Order of DGLAP influences size of HT Higher twist falls slowly compared to PDF’s at large x. Why HT in PVDIS is Special • Twist-2 (mostly) cancel in asymmetry • Twist-4 is (basically) leading twist • Clean access twist-4 effect: free from twist-2 order dependence • Study quark-quark correlations Coherent Program of PVDIS Study Strategy: requires precise kinematics and broad range Fit data to: 1 2 A A1 HT CSV x 3 2 (1 x) Q C(x)=βHT/(1-x)3 • Measure AD in NARROW bins of x, Q2 with 0.5% precision • Cover broad Q2 range for x in [0.3,0.6] to constrain HT • Search for CSV with x dependence of AD at high x • Use x>0.4, high Q2, and to measure a combination of the Ciq’s x y Q2 New Physics no yes no CSV yes no no Higher Twist yes no yes Other Targets • Hydrogen: d/u • EMC effect PVDIS on the Proton: d/u at High x u ( x) 0.91d ( x) a ( x) u ( x) 0.25d ( x) P Deuteron analysis has large nuclear corrections (Yellow) APV for the proton has no such corrections (complementary to BONUS) 3-month run The challenge is to get statistical and systematic errors ~ 2% CSV in Heavy Nuclei: EMC Effect Additional possible application of SoLID 5% Isovector-vector mean field. (Cloet, Bentz, and Thomas) SoLID Spectrometer Gas Cerenkov Shashlyk Baffles GEM’s Baffles Rates in detectors reduced by more than 10 Kinematics at large x Physics Resolution (%) vs Detector Resolution and Angle p 2 Q x SoLID Collaboration P. Bosted, J. P. Chen, E. Chudakov, A. Deur, O. Hansen, C. W. de Jager, D. Gaskell, J. Gomez, D. Higinbotham, J. LeRose, R. Michaels, S. Nanda, A. Saha, V. Sulkosky, B. Wojtsekhowski Jefferson Lab P. A. Souder, R. Holmes Syracuse University K. Kumar, D. McNulty, L. Mercado, R. Miskimen U. Massachusetts H. Baghdasaryan, G. D. Cates, D. Crabb, M. Dalton, D. Day, N. Kalantarians, N. Liyanage, V. V. Nelyubin, B. Norum, K. Paschke, S. Riordan, O. A. Rondon, M. Shabestari, J. Singh, A. Tobias, K. Wang, X. Zheng University of Virginia J. Arrington, K. Hafidi, P. E. Reimer, P. Solvignon Argonne L. El Fassi, R. Gilman, R. Ransome, E. Schulte P. Markowitz Rutgers Florida International W. Chen, H. Gao, X. Qian, Y. Qiang, Q. Ye X. Jiang O. Glamazdin, R. Pomatsalyuk Los Alamos Duke University W. Korsch K. A. Aniol University of Kentucky NSC Kharkov Institute for Physics and Technology California State J. Erler G. M. Urciuoli Universidad Autonoma de Mexico INFN, Sezione di Roma A. Lukhanin, Z. E. Meziani, B. Sawatzky Temple University P. M. King, J. Roche Carnegie Mellon G. Ron D. Armstrong, T. Averett, J. M. Finn Tel Aviv University William and Mary T. Holmstrom P. Decowski Smith College Longwood University B.-Q. Ma, Y. J. Mao Beijing University China Institute of Atomic Energy C. Keppel Hampton University University of Science and Technology of China Benmokhtar, G. Franklin, B. Quinn Tsinghua University University of Wisconsin E. Beise MIT Z. G. Xiao X. M. Li, J. Luan, S. Zhou H. Lu, X. Yan, Y. Ye, P. Zhu W. Bertozzi, S. Gilad, W. Deconinck, S. Kowalski, B. Moffit Louisiana Tech M. J. Ramsey-Musolf Ohio University University of Maryland K. Grimm, K. Johnston, N. Simicevic, S. Wells N. Morgan, M. Pitt B. T. Hu, Y. W. Zhang, Y. Zhang Lanzhou University C. M. Camacho, E. Fuchey, C. Hyde, F. Itard J.-C. Peng LPC Clermont, Université Blaise Pascal University of Illinois A. Deshpande Virginia Tech H. P. Cheng, R. C. Liu, H. J. Lu, Y. Shi Huangshan University SUNY Stony Brook A. T. Katramatou, G. G. Petratos S. Choi, Ho. Kang, Hy. Kang B. Lee, Y. Oh Kent State University Seoul National University J. W. Martin J. Dunne, D. Dutta Mississippi State University of Winnipeg STATUS and PLANS • • • • Jan. 2009: Conditional approval Jan. 2010: Seek full approval Fall 2010: Director’s review Spring 2011: Seek CD0 Conclusions • PVDIS addresses many physics topics • • • • • Electroweak couplings CSV at the quark level Higher Twist d/u for the proton Nuclear-induced CSV • SOLID spectrometer can deliver the physics