Presentation is loading. Please wait.

Presentation is loading. Please wait.

New Results from the HAPPEx Experiments at Q2= 0.1 GeV/c2

Similar presentations


Presentation on theme: "New Results from the HAPPEx Experiments at Q2= 0.1 GeV/c2"— Presentation transcript:

1 New Results from the HAPPEx Experiments at Q2= 0.1 GeV/c2
nucl-ex / submitted to PRL Robert Michaels For the HAPPEX Collaboration Thomas Jefferson National Accelerator Facility – Argonne National Laboratory – CSU, Los Angeles -William and Mary – Duke – DSM/DAPNIA/SPhN CEA Saclay - FIU – Harvard - INFN, Rome - INFN, Bari – IAE, Beijing – IPT Kharkov - Jozef Stefan Institute – Kent State - MIT – NPIRAS, St. Petersburg – ODU – Rutgers - Smith College – Syracuse – Temple – U. Blaise Pascal – U. of Illinois Urbana-Champagne – UMass, Amherst – U. of Kentucky – U. of Virginia – UST, Heifei

2 Outline Parity-violation in electron scattering
Elastic Vector Strange Form Factors: GsE and GsM Q2 = 0.1 (GeV/c)2 as/of early 2005 Results from 2005 data taking of HAPPEx-II: HAPPEx-hydrogen and HAPPEx-Helium The present situation at Q2 = 0.1 (GeV/c)2 Implications and Conclusions

3 Strangeness in the nucleon
Nucleon in QCD « sea » s quark: cleanest candidate to study the sea ) How much do virtual pairs contribute to the structure of the nucleon ? Momentum : 4 % (DIS) Spin : 0 to -10% (polarized DIS) Mass : 0 to 30 % (N -sigma term) (large uncertainties on these contributions) Goal: Determine the contributions of the strange quark sea ( ) to the charge and current/spin distributions in the nucleon : “strange form factors” GsE and GsM

4 Parity Violating Electron Scattering  Weak NC Amplitudes
Interference:  ~ |MEM |2 + |MNC |2 + 2Re(MEM*)MNC Interference with EM amplitude makes Neutral Current (NC) amplitude accessible Tiny (~10-6) cross section asymmetry isolates weak interaction

5 Form Factors Adopt the Sachs FF:
(Roughly: Fourier transforms of charge and magnetization) NC probes same hadronic flavor structure, with different couplings: GZE/M provide an important new benchmark for testing non-perturbative QCD structure of the nucleon

6 Charge Symmetry Gg,pE,M GsE,M GuE,M GdE,M Gg,nE,M GZ,pE,M GnE,M GpE,M
One expects the neutron to be an isospin rotation of the proton : Gg,pE,M GsE,M GuE,M GdE,M Gg,nE,M Charge symmetry GZ,pE,M <N| sgm s |N> GnE,M GpE,M Shuffle Well Measured New : CSV could be as large as our stat. error: Kubis & Lewis PRC 74 (015204) 2006.

7 Isolating the form factors: vary the kinematics or target
For a proton: ~ few parts per million Forward angle Backward angle For 4He: GEs alone For deuterium: enhanced GAe sensitivity

8 Theoretical Approaches to Strange Form Factors
Models - a non-exhaustive list: kaon loops, vector dominance, Skyrme model, chiral quark model, dispersion relations, NJL model, quark-meson coupling model, chiral bag model, HBChPT, chiral hyperbag, QCD equalities, … - no consensus on magnitudes or even signs of GsE and GsM ! a challenging problem in non-perturbative QCD QCD on the lattice - Dong, Liu, Williams PRD 58(1998)074504 - Lewis, Wilcox, Woloshyn PRD 67(2003)013003 - Leinweber, et al PRL 94(2005) and PRL 97(2006)

9 Strangeness Models (as/of 2000)
Leading moments of form factors: s = GMs (Q2=0) s = GEs/ (Q2=0)

10 World Data (early 2005) at Q2 ~ 0.1 GeV2
Note : SAMPLE result adopts Zhu et al. calculation of GAe PRD 62(2000)033008 GEs = ± 0.29 GMs = 0.62 ± 0.32 . Would imply that 5-10% of nucleon magnetic moment is Strange Caution: the combined fit is approximate. Correlated errors and assumptions not taken into account

11 Measurement of P-V Asymmetries
5% Statistical Precision on 1 ppm -> requires 4x1014 counts Rapid Helicity Flip: Measure the asymmetry at 10-4 level, 10 million times High luminosity: thick targets, high beam current Control noise (target, electronics) High beam polarization and rapid flip A (ppm) Statistics: high rate, low noise Systematics: beam asymmetries, backgrounds, Helicity correlated DAQ Normalization: Polarization, Linearity, Dilution

12 HAPPEX (second generation)
E=3 GeV q=6° Q2= 0.1 (GeV/c)2 New 2005 results: nucl-ex/ Submitted to PRL Hydrogen : GsE + a GsM 4He: Pure GsE :

13 Hall A at Jefferson Lab Polarized e- Source Hall A

14 High Resolution Spectrometer
Hall A at Jefferson Lab Compton 1% syst Continuous Møller 2-3% syst Polarimeters Target 400 W transverse flow 20 cm, LH2 20 cm, 200 psi 4He High Resolution Spectrometer + septum 5 mstr over 4o-8o

15 Summary of Data Runs: HAPPEX-II
June 2004 HAPPEX-He about 3M pairs at 1300 ppm => dAstat ~ 0.74 ppm June – July 2004 HAPPEX-H about 9M pairs at 620 ppm => dAstat ~ 0.2 ppm July-Sept 2005 about 35M pairs at 1130 ppm => dAstat ~ 0.19 ppm Oct – Nov 2005 about 25M pairs at 540 ppm => dAstat ~ ppm This talk

16 elastic events by HRS optics
High Resolution Spectrometers Clean separation of elastic events by HRS optics Locate detector over elastic line and integrate the flux Detector Elastic Rate: 1H: 120 MHz 4He: 12 MHz Detector Cherenkov cones PMT 12 m dispersion sweeps away inelastic events Brass-Quartz Integrating Cerenkov Shower Calorimeter Large dispersion & heavy shielding reduce backgrounds at focal plane

17 Backgrounds Aluminum endcaps Inelastics Aluminum target windows
Shown is the single-particle momentum spectra. Detector Footprint Inelastics Aluminum target windows Inelastics and re-scattering Poletip (negligible) Aluminum endcaps Detector Footprint

18 Correcting Beam Asymmetries
Araw = Adet - AQ + i=1,5ixi natural beam jitter (regression) beam modulation (dithering) Slopes from Independent methods provide a cross-check. Each is subject to different systematic errors. Regression: Natural beam motion, measure dA/dDxi Simultaneous fit establishes independent sensitivities By definition, removes correlation of asymmetry to beam monitors Sensitive to highly correlated beam motion and electronics noise “Dithering”: Induce non-HC beam motion with coils, measure dS/dCi, dxi/dCi Relate slopes to dS/dxi Not compromised by correlated beam motion Robust, clear signals for failures Sensitive to non-linearities

19 Beam Position Differences, Helium
Position difference goal: 3 nanometers! All’s well that ends well Problem clearly identified as beam steering from electronic cross-talk No helicity-correlated electronics noise in Hall DAQ at < ppb level Large position differences cancel in average over both detectors X Angle BPM micron Helicity signal to driver removed Raw ALL Asymetry ppm Helicity signal to driver reversed Problem: Helicity signal deflecting the beam through electronics “pickup” Large beam deflections even when Pockels cell is off

20 Beam Position Corrections, Helium
Raw Left Asymmetry Corrected Left Asymmetry Beam Asymmetries Energy: -3ppb X Target: -5 nm X Angle: -28 nm Y Target :-21 nm Y Angle: 1 nm ppm ppm Raw Right Asymmetry Corrected Right Asymmetry Total Corrections: Left: -370 ppb Right: 80 ppb All: 120 ppb ppm ppm

21 Beam Position Corrections, Hydrogen
X Angle BPM Surpassed Beam Asymmetry Goals for Hydrogen Run Energy: ppb X Target: 1 nm X Angle: 2 nm Y Target : 1 nm Y Angle: <1 nm micron Corrected and Raw, Left arm alone, Superimposed! ppm Total correction for beam position asymmetry on Left, Right, or ALL detector: 10 ppb

22 Araw = 6.40 ppm  0.23 (stat)  0.12 (syst)
4He Results Slug Asymmetry (ppm) Raw Parity Violating Asymmetry Araw correction ~ 0.3 ppm Helicity Window Pair Asymmetry Q2 = ± GeV2 Araw = 6.40 ppm  (stat)  0.12 (syst)

23 Araw = -1.58 ppm  0.12 (stat)  0.04 (syst)
Asymmetry (ppm) Slug 1H Results Raw Parity Violating Asymmetry Araw correction ~3 ppb Helicity Window Pair Asymmetry Q2 = ± GeV2 Araw = ppm  (stat)  0.04 (syst)

24 Compton Polarimetry Hydrogen: 87.1 ± 0.9 % Continuous, non-invasive
Here : Electron Detector analysis Cross-checked with Møller, Mott polarimeters also: independent electron analysis Helium: ± 0.8 % Helium ran with lower beam energy, making the analysis significantly more challenging. Breakthroughs in both photon and electron analyses obtained 1% systematic uncertainty

25 Miscellany Backgrounds: Dilutions: 2 % (4He) 0.8% (1H)
Systematic ppb (4He) ppb (1H) Q2 & effective kinematics: Q2 < 1.0% Two-photon exchange corrections: small (no explicit correction made) Transverse asymmetry: measured directly in dedicated runs, cancels in left-right sum; Systematic: 4 ppb (1H) 8 ppb (4He) Electromagnetic Form Factors: use Friedrich & Walcher parameterization, Eur. Phys. J. A, 17, 607 (2003), and BLAST data for GEn Axial Form Factor: highly suppressed for 1H (not present for 4He) Vector Electroweak Radiative Corrections: Particle Data Group Blinded Analysis

26 4He: Nuclear Effects O+  O+ T=0 transition
Any one-body electroweak operator O: (eg Fetter and Walecka) <J,T|O|J,T> =  J,T (,’) <’|O|> |> = complete set one-body density matrix element single-particle matrix element (nuclear structure) (nucleon structure) Asymmetry involves ratio of weak/EM matrix elements (GEs and GET=0); Single term in J,T in transition; O same in weak and EM except for couplings  same one-body density matrix elements in numerator/denominator  nuclear structure cancels, only nucleon form factors remain This result is EXACT, if : 4He g.s. pure isospin state: Ramavataram, Hadjimichael, Donnelly PRC 50(1994)1174 No D-state admixture: Musolf & Donnelly PL B318(1993)263 Meson exchange corrections small: Musolf, Schiavilla, Donnelly PRC 50(1994)2173 Nuclear effects all << 1%, no explicit correction made.

27 Error Budget-Hydrogen
HAPPEx Error Budget-Helium 2005 (this report) 2004 run False Asymmetries 59 ppb Polarization 51 ppb Linearity 58 ppb Radiative Corrections 6 ppb Q2 Uncertainty Al background 32 ppb Helium quasi-elastic background 20 ppb Total 120 ppb False Asymmetries 103 ppb Polarization 115 ppb Linearity 78 ppb Radiative Corrections 7 ppb Q2 Uncertainty 66 ppb Al background 14 ppb Helium quasi-elastic background 86 ppb Total 205 ppb Error Budget-Hydrogen 2005 (this report) 2004 run False Asymmetries 17 ppb Polarization 14 ppb Linearity 15 ppb Radiative Corrections 3 ppb Q2 Uncertainty 16 ppb Al background 19 ppb Rescattering Background 4 ppb Total 37 ppb False Asymmetries 43 ppb Polarization 23 ppb Linearity 15 ppb Radiative Corrections 7 ppb Q2 Uncertainty 12 ppb Al background 16 ppb Rescattering Background 32 ppb Total 63 ppb

28 HAPPEX-II 2005 Results HAPPEX-4He:
Q2 = ± (GeV/c)2 APV =  0.23 (stat)  0.12 (syst) ppm A(Gs=0) = ppm GsE =  0.014(stat)  0.007(syst) HAPPEX-H: Q2 = ± (GeV/c)2 APV =  0.12 (stat)  0.04 (syst) ppm A(Gs=0) = ppm  ppm GsE GsM =  0.011(stat)  0.004(syst)  0.005(FF)

29 HAPPEX-II 2005 Results Three bands:
Inner: Project to axis for 1-D error bar Middle: 68% probability contour Outer: 95% probability contour Caution: the combined fit is approximate. Correlated errors and assumptions not taken into account

30 World Data near Q2 ~0.1 GeV2 GMs = 0.28 +/- 0.20
GEs = / ~3% +/- 2.3% of proton magnetic moment ~0.2 +/- 0.5% of electric distribution HAPPEX-only fit suggests something even smaller: GMs = /- 0.24 GEs = / Caution: the combined fit is approximate. Correlated errors and assumptions not taken into account

31 World data consistent with state of the art theoretical predictions
16. Skyrme Model - N.W. Park and H. Weigel, Nucl. Phys. A 451, 453 (1992). 17. Dispersion Relation - H.W. Hammer, U.G. Meissner, D. Drechsel, Phys. Lett. B 367, 323 (1996). 18. Dispersion Relation - H.-W. Hammer and Ramsey-Musolf, Phys. Rev. C 60, (1999). 19. Chiral Quark Soliton Model - A. Sliva et al., Phys. Rev. D 65, (2001). 20. Perturbative Chiral Quark Model - V. Lyubovitskij et al., Phys. Rev. C 66, (2002). 21. Lattice - R. Lewis et al., Phys. Rev. D 67, (2003). 22. Lattice + charge symmetry -Leinweber et al, Phys. Rev. Lett. 94, (2005) & Phys. Rev. Lett. 97, (2006) [22]

32 Figures courtesy of R. Carlini, R. Young
A Global Fit: R.D. Young, et al. nucl-ex/ all data Q2 < 0.3, leading moments of GEs , GMS Kelly’s EMF Float GAe separately for neutron and proton With HAPPEx-2005 data Before HAPPEx-2005 data Figures courtesy of R. Carlini, R. Young

33 Future: HAPPEX-3 (2007 or 8)

34 Conclusions Marvelous consistency of data. Q2 = 0.1 GeV2 : GsM and GsE consistent with zero; constraining axial FF to Zhu et al. theory favors positive GsM 4He: best fractional error in PV experiment to date (< 4%) no axial contamination  uniquely determines GsE 1H: < 100 ppb error on A, unprecedented “parity quality” Still room (& hints?) for non-zero values at higher Q2 Future of Strangeness form factors: G0 Backward: will allow GsM and GsE separation at two Q2 Mainz: PV-A4 backward-angle program well underway HAPPEx-III: high precision Q2 = 0.6 GeV2

35 Backup Slides

36 Two Photon Exchange  and Z box and crossing diagrams.
Beyond single boson exchange in electroweak interference:  and Z box and crossing diagrams. effects appear small at large  and small Q2 not a concern at present experimental precision. Electromagnetic Form Factors used to extract strange form factors: which form factors to use? Transverse Asymmetry/Beam normal asymmetry/Vector analyzing power:  “background” to PV measurements, if electron beam not 100% longitudinal and detectors not perfectly symmetric.  interesting in its own right – imaginary parts of TPE.

37 Validity of charge symmetry assumption
Size of charge symmetry breaking effects in some n,p observables: n - p mass difference  (mn - mp)/mn ~ 0.14% polarized elastic scattering n + p, p+n A = An - Ap = (33 ± 6) x 10-4 Vigdor et al, PRC 46, 410 (1992) Forward backward asymmetry n + p  d + 0 Afb ~ (17 ± 10)x 10-4 Opper et al., nucl-ex (2003)  For vector FF: theoretical CSB estimates indicate < 1% violations Miller PRC 57, 1492 (1998) Lewis & Mobed, PRD 59, (1999) Very recent : effects could be large as statistical error on our data! Kubis & Lewis PRC 74, (2006)

38 EM Form Factors Electromagnetic form factors parameterized as by:
Friedrich and Walcher, Eur. Phys. J. A, 17, 607 (2003) GEn from BLAST: Claimed uncertainty at 7-8% FF Error GEp 2.5% GMp 1.5% GEn 10% GMn GA(3) - GA(8)

39 HAPPEX (first generation)
Hydrogen Target: E=3.3 GeV, q=12.5°, Q2=0.48 (GeV/c)2 APV = ppm ± 0.98 (stat) ppm ± 0.56 (syst) ppm GsE GsM = ± (exp) ± (FF) Phys. Rev. Lett. 82,1096 (1999); Phys. Lett. B509, 211 (2001); Phys. Rev. C 69, (2004) “Parity Quality” JLab AA suppressed by ‘ (1 – 4 sin2w) where ‘ = [(1 + )(1 - 2)]½  (0.08)(0.08) here.

40 Background Dedicated runs at very low current using track reconstruction of the HRS Acceptance Rolloff Dipole field scan to measure the probability of rescattering inside the spectrometer Helium Helium QE in detector: /- 0.15% Helium QE rescatter: /- 0.15% Al fraction: /- 0.2% Hydrogen: Al fraction /- 25 % Hydrogen Tail + Delta rescatter: <0.1% Total systematic uncertainty contribution ~40 ppb (Helium), ~15ppb (Hydrogen)

41 Determining Q2 Asymmetry explicitly depends on Q2: Goal:
Q2 measured using standard HRS tracking package, with reduced beam current Central scattering angle must be measured to dq < 0.5% Asymmetry distribution must be averaged over finite acceptance

42 SAMPLE (MIT/Bates) GMs = 0.23  0.36  0.40
GeA(T=1) =  0.57  0.50 E.J. Beise et al., Prog Nuc Part Phys 54 (2005) Results of Zhu et al commonly used to constrain GSM result: GsM = 0.37  0.20Stat  0.36Syst  0.07FF

43 PV-A4 (MAMI/Mainz) GEs + aGMs
Q2 (GeV2) A  stat  syst (ppm) GEs + aGMs 0.230 -5.44  0.54  0.26 GEs GMs =  0.034 0.101 -1.36  0.29  0.13 GEs GMs =  0.036 “Evidence for Strange Quark Contributions to the Nucleon’s Form Factors at Q2 = 0.1 GeV2” PRL 94, (2006) Back Angle runs underway to separate GsM, GA at additional points…

44 s and s have different spatial distributions in proton
What would non-zero GsE and GsM imply? GsE  0 GsM  s and s have different magnetization distributions in proton -> contribute to magnetic moment, etc. s and s have different spatial distributions in proton Kaon = us proton proton Hyperon = uds (naive model for illustration)

45 A Simple Fit (for a simple point)
GEs = r_s*t GMs = mu_s Includes only data Q2 < 0.3 GeV2 Includes SAMPLE constrainted with GA theory and HAPPEX-He 2004, 2005 G0 Global error allowed to float with unit constraint Nothing intelligent done with form factors, correlated errors, etc. Preliminary Quantitative values should NOT be taken very seriously, but some clear, basic points: The world data are consistent. Rapid Q2 dependence of strange form-factors is not required. Sizeable contributions at higher Q2 are not definitively ruled out. (To be tested by HAPPEX-III, G0 and A4 backangle.)


Download ppt "New Results from the HAPPEx Experiments at Q2= 0.1 GeV/c2"

Similar presentations


Ads by Google