The Q p weak Experiment: A Search for New TeV Scale Physics via a Measurement of the Proton’s Weak Charge Measure: Parity-violating asymmetry in e + p.

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Presentation transcript:

The Q p weak Experiment: A Search for New TeV Scale Physics via a Measurement of the Proton’s Weak Charge Measure: Parity-violating asymmetry in e + p elastic scattering at Q 2 ~ 0.03 GeV 2 to ~4% relative accuracy at JLab Extract: Proton’s weak charge Q p weak ~ 1 – 4 sin 2  W to get ~0.3% on sin 2  W at Q 2 ~ 0.03 GeV 2 tests “running of sin 2  W ” from M 2 Z to low Q 2 sensitive to new TeV scale physics W.T.H. van Oers

What about the running of sin 2  W ? Running coupling constants in QED and QCD QED (running of  ) ss QCD(running of  s ) 137  Q 2, GeV 2

“Running of sin 2  W ” in the Electroweak Standard Model Electroweak radiative corrections  sin 2  W varies with Q + +  All “extracted” values of sin 2  W must agree with the Standard Model prediction or new physics is indicated.

LE Experiments: Good News/Bad News A 1% measurement of a weak-scale quantity, suppressed by an order of magnitude, is sensitive to physics at the scale 3 TeV. This is well above present colliders and complementary to LHC. Fine print: Low energy experiments can’t measure Λ or g separately, only Λ /g. With no bump to display, enormous burden of proof on experiment and theory. If limited by systematic errors, a factor of 2 increase in mass scale requires 2 2 = 4 reduction in the systematic error. (eg, atomic experiments) If limited by statistical errors, a factor of 2 increase in mass scale requires ( 2 2 ) 2 = 16 improvement in statistical figure of merit. (eg, scattering experiments) A factor of 2 increase in Λ /g in the scattering sector may happen only once per generation! Nevertheless, JLab can do that and a bit more. Courtesy of D.J. Mack

Weak Charge Phenomenology This accidental suppression of the proton weak charge in the SM makes it more sensitive to new physics (all other things being equal). Note how the roles of the proton and neutron are become almost reversed (ie, neutron weak charge is dominant, proton weak charge is almost zero!) Courtesy of D.J. Mack

(at tree level) Q p weak : Extract from Parity-Violating Electron Scattering measures Q p – proton’s electric charge measures Q p weak – proton’s weak charge M EM M NC As Q 2  0 Q p weak is a well-defined experimental observable Q p weak has a definite prediction in the electroweak Standard Model

Parameterize New Physics contributions in electron-quark Lagrangian A 4% Q p Weak measurement probes with 95% confidence level for new physics at energy scales to: g: coupling constant,  : mass scale The TeV discovery potential of weak charge measurements will be unmatched until LHC turns on. If LHC uncovers new physics, then precision low Q 2 measurements will be needed to determine charges, coupling constants, etc. Energy Scale of an “Indirect” Search for New Physics

JLab Qweak Run I + II + III (preliminary) ±0.006 (proposed) - Qweak measurement will provide a stringent stand alone constraint on Lepto-quark based extensions to the SM. Q p weak (semi-leptonic) and E158 (pure leptonic) together make a powerful program to search for and identify new physics. SLAC E158 Q p weak & Q e weak – Complementary Diagnostics for New Physics Erler, Kurylov, Ramsey-Musolf, PRD 68, (2003)

Model-Independent Constraints Figures courtesy of Paul Reimer (ANL) Forget about the predictions of any specific new physics model! Do the up- and down-quarks have their expected SM weak charges? -Qw(up)/2 -Qw(down)/2 today future Constraints by 12C and APV are nearly parallel (N ~ Z). Proton measurement is needed so weak charges can be separated with interesting errors. Qw(He) where N = Z could provide an important cross-check on Cs APV. Dot is SM value -Qw(down)/2 now

Overview of the Q p Weak Experiment Incident beam energy: GeV Beam Current: 180 μA Beam Polarization: 85% LH 2 target power: 2.5 KW Central scattering angle: 8.4° ± 3° Phi Acceptance: 53% of 2 Average Q²: GeV 2 Acceptance averaged asymmetry:–0.29 ppm Integrated Rate (all sectors): 6.4 GHz Integrated Rate (per detector): 800 MHz Experiment Parameters (integration mode) Polarized Electron Beam 35cm Liquid Hydrogen Target Collimator with 8 openings θ= 8° ± 2° Region I GEM Detectors Region II Drift Chambers Toroidal Magnet Region III Drift Chambers Elastically Scattered Electron Eight Fused Silica (quartz) Čerenkov Detectors Luminosity Monitors

How it Works : Qweak Apparatus in GEANT4 Courtesy of Klaus Grimm (W&M) Courtesy of D.J. Mack

  A phys /A phys  Q p weak /Q p weak Statistical (2200 hours production) 1.8% 2.9% Systematic: Hadronic structure uncertainties % Beam polarimetry 1.0% 1.6% Absolute Q 2 determination 0.5% 1.1% Backgrounds 0.5% 0.8% Helicity-correlated Beam Properties 0.5%0.8% _________________________________________________________ Total 2.2% 4.1%   A phys /A phys  Q p weak /Q p weak Statistical (2200 hours production) 1.8% 2.9% Systematic: Hadronic structure uncertainties % Beam polarimetry 1.0% 1.6% Absolute Q 2 determination 0.5% 1.1% Backgrounds 0.5% 0.8% Helicity-correlated Beam Properties 0.5%0.8% _________________________________________________________ Total 2.2% 4.1% (Erler, Kurylov, Ramsey-Musolf, PRD 68, (2003)) Q p W =  theoretically 0.8% error comes from QCD uncertainties in box graphs, etc. (Erler, Kurylov, Ramsey-Musolf, PRD 68, (2003)) Q p W =  theoretically 0.8% error comes from QCD uncertainties in box graphs, etc. Anticipated Q p Weak Uncertainties 4% error on Q p W corresponds to ~0.3% precision on sin 2  W at Q 2 ~ 0.03 GeV 2

Constraints on A hadronic from other Measurements Quadrature sum of expected  A hadronic = 1.5% and  A axial = 1.2% errors contribute ~1.9% to error on Q p W hadronic: (31% of asymmetry) - contains G  E,M G Z E,M Constrained by HAPPEX, G 0, MAMI PVA4 hadronic: (31% of asymmetry) - contains G  E,M G Z E,M Constrained by HAPPEX, G 0, MAMI PVA4 axial: (4% of asymmetry) - contains G e A, has large electroweak radiative corrections. Constrained by G 0 and SAMPLE axial: (4% of asymmetry) - contains G e A, has large electroweak radiative corrections. Constrained by G 0 and SAMPLE Nucleon Structure Contributions to the Asymmetry

Region 3: Vertical Drift chambers Region 2: Horizontal drift chamber location Region 1: GEM Gas Electron Multiplier Quartz Cherenkov Bars (insensitive to non-relativistic particles) Collimator System Mini-torus QTOR Magnet Trigger Scintillator Lumi Monitors e - beam The Qweak Apparatus (Calibration Mode Only - Production & Calibration Modes) E beam = GeV I beam = 180 μ A Polarization ~85% Target = 2.5 KW

8 toroidal coils, 4.5m long along beam Resistive, similar to BLAST magnet Pb shielding between coils Coil holders & frame all Al  B  dl ~ 0.7 T-m bends elastic electrons ~ 10 o current ~ 9500 A Status:  coils wound in France  support stand under construction Q p Weak Toroidal Magnet - QTOR

View Along Beamline of Q p Weak Apparatus - Simulated Events Central scattering angle: ~8.4° ± 3° Phi Acceptance: > 50% of 2  Average Q²: GeV 2 Acceptance averaged asymmetry: –0.29 ppm Integrated Rate (per detector): ~801 MHz Inelastic/Elastic ratio: ~0.026% Central scattering angle: ~8.4° ± 3° Phi Acceptance: > 50% of 2  Average Q²: GeV 2 Acceptance averaged asymmetry: –0.29 ppm Integrated Rate (per detector): ~801 MHz Inelastic/Elastic ratio: ~0.026% Very clean elastic separation! rectangular quartz bar; 18 cm wide X 2 meters long rectangular quartz bar; 18 cm wide X 2 meters long Inelastic/Elastic Separation in Q p Weak

Target Concept: Similar in design to SAMPLE and G 0 targets  longitudinal liquid flow  high stream velocity achieved with perforated, tapered “windsock” Target Concept: Similar in design to SAMPLE and G 0 targets  longitudinal liquid flow  high stream velocity achieved with perforated, tapered “windsock” Q p Weak Target parameters/requirements: Length = 35 cm Beam current = 180  A Power = 2200 W beam W heater Raster size ~4 mm x ~4 mm square Flow velocity > 700 cm/s Density fluctuations (at 15 Hz) < 5x10 -5 Use reversal rate of 270 Hz Q p Weak Target parameters/requirements: Length = 35 cm Beam current = 180  A Power = 2200 W beam W heater Raster size ~4 mm x ~4 mm square Flow velocity > 700 cm/s Density fluctuations (at 15 Hz) < 5x10 -5 Use reversal rate of 270 Hz The Q p Weak Liquid Hydrogen Target

 P = P + – P - Y = Detector yield (P = beam parameter ~energy, position, angle, intensity) Example: Typical goals for run-averaged beam properties Intensity: Position: keep small with feedback and careful setup keep small with symmetrical detector setup Helicity Correlated Beam Properties: False Asymmetry Corrections

Region 3: Vertical Drift chambers Region 2: Horizontal drift chamber location Region 1: GEM Gas Electron Multiplier Quartz Cherenkov Bars (insensitive to non-relativistic particles) Trigger Scintillator e - beam Expected Q 2 distribution Region chambers --> determine value of Q 2 Region 3 chamber --> efficiency map of quartz detectors Q 2 Determination Use low beam current (~ few nA) to run in “pulse counting” mode with a tracking system to determine the “light-weighted” Q 2 distribution.

Hall C has existing ~1% precision Moller polarimeter Present limitations: -I Max ~ 10  A. -At higher currents the Fe target depolarizes. -Measurement is destructive Plan to upgrading Møller: -Measure P beam at 100  A or higher, quasi-continuously -Trick: kicker + strip or wire target (early tests look promising – tested up to 40  A so far) Schematic of planned new Hall C Compton polarimeter. Precision Polarimetry

e2ePV at 12 GeV E = 12 GeV 4000 hours L = 150 cm A PV = -40 ppb JLab could determine Qw(e) to 2.5% as a search for new physics or the best low energy determination of the weak mixing angle. Courtesy of D.J. Mack

e2ePV at 12 GeV Qw(e) would tightly constrain RPV SUSY (ie tree-level) Killer application of improved Qw(e) is to RPC SUSY (ie, loop-level) One of few ways to constrain RPC SUSY if it happens to conserve CP (hence SUSY EDM = 0). Direct associated- production of a pair of RPC SUSY particles might not be possible even at LHC. Theory contours 95% CL Expt bands 1σ Contours courtesy of Shufang Su (U. Arizona) ΔQw(e) ΔQw(p)  (Q e W ) SUSY / (Q e W ) SM

Future of the JLab Weak Charge Program Qw(p) finish construction (mid 2007) Run I (8%) (2008?) (lick wounds following embarrassing confrontation with Mother Nature) Run II (4%) (Potential 1% Qw(He) as cross-check on Cs APV?) What do we do when the LHC (or Atomic Physics) turns our world upside down? Will Run II be finished so JLab can respond? What do we do if we see a significant deviation in Run II? 2.5% Qw(p)/Qw(He) Constrain e-up and e-down quark couplings of ~TeV mass particles discovered by LHC. 2.5% Qw(e) at 12 GeV Constrain e-e couplings of ~TeV mass particles discovered by LHC. or If LHC finds the TeV-scale region is a desert, make world’s best measurement of the weak mixing angle at low energy. Courtesy of D.J. Mack

Completed low energy Standard Model tests are consistent with Standard Model “running of sin 2  W ” SLAC E158 (running verified at ~ 6  level) - leptonic Cs APV (running verified at ~ 4  level ) – semi-leptonic, “d-quark dominated” Upcoming Q p W Experiment Precision measurement of the proton’s weak charge in the simplest system. Sensitive search for new physics with CL of 95% at the ~ 2.3 TeV scale. Fundamental 10  measurement of the running of sin 2  W at low energy. Currently in process of 3 year construction cycle; goal is to have multiple runs in 2008 – 2009 timeframe Possible 12 GeV Parity-Violating Moller Experiment at JLAB Conceptual design indicates reduction of E158 error by ~5 may be possible at 12 GeV JLAB. weak charge triad  (Ramsey-Musolf) Summary