34
Experiences from Q weak David S. Armstrong College of William & Mary Physics Beyond the Standard Model and Precision Nucleon Structure Measurements with ParityBViolating Electron Scattering ECT*, Trento August 1 2016 08/01/2016 1 Armstrong ECT*

DSA Trento clean - William & Maryphysics.wm.edu/~armd/DSA_Trento_clean.pdfMeeting*PVES*Challenges 08/01/2016 Armstrong**ECT* 6 B 180*μA*beam*current****(JLabrecord) B High*power*cryogenic*target

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Page 1: DSA Trento clean - William & Maryphysics.wm.edu/~armd/DSA_Trento_clean.pdfMeeting*PVES*Challenges 08/01/2016 Armstrong**ECT* 6 B 180*μA*beam*current****(JLabrecord) B High*power*cryogenic*target

Experiences*from*Qweak

David*S.*ArmstrongCollege&of&William&&&Mary

Physics*Beyond*the*Standard*Model*and*Precision*Nucleon*Structure*Measurements*with*ParityBViolating*Electron*ScatteringECT*,&Trento&&&&&August&1&2016

08/01/2016 1Armstrong**ECT*

Page 2: DSA Trento clean - William & Maryphysics.wm.edu/~armd/DSA_Trento_clean.pdfMeeting*PVES*Challenges 08/01/2016 Armstrong**ECT* 6 B 180*μA*beam*current****(JLabrecord) B High*power*cryogenic*target

Caveat&Emptor

2

08/01/2016 Armstrong**ECT*

What%this%talk%%is not:

B Detailed*motivation/theory*review*for*the*Qweak experimentB No*new*physics*result:*we*are*not*ready*to*unblind (yet)

What%this%talk%%is:%

B Review*of*some*of*important*experimental*issues*&*where*the*analysis*stands*

B Emphasis*on*topics*that*were*unexpected*and/or*relevant*for*future*PVES*measurements

B My*own*(personal)*choice*of*emphasis

Page 3: DSA Trento clean - William & Maryphysics.wm.edu/~armd/DSA_Trento_clean.pdfMeeting*PVES*Challenges 08/01/2016 Armstrong**ECT* 6 B 180*μA*beam*current****(JLabrecord) B High*power*cryogenic*target

Weak*Charge

3

08/01/2016 Armstrong**ECT*

Electroweak*Lagrangian → ParityBViolating*electronBquark* term:*

←#Proton’s*Weak*Charge

For*forward*angle*scattering*at*low*Q2 :**

APV accesses

Page 4: DSA Trento clean - William & Maryphysics.wm.edu/~armd/DSA_Trento_clean.pdfMeeting*PVES*Challenges 08/01/2016 Armstrong**ECT* 6 B 180*μA*beam*current****(JLabrecord) B High*power*cryogenic*target

SM

Qweakkinematics Hadronic term*extracted* from*fit

Extracting*the*Weak*Charge

4

$%& = −)*+,

4./ 2+12 + 4 5, +, +,

Hadron structure*enters*here:*electromagnetic* and*electroweak* form*factors…

Previous*experiments*(strange*form*factor*program:*SAMPLE,*HAPPEX,*G0,*PVA4)*explored*hadron*structure;*allow*subtraction*of*hadronic*contribution

$789 =:;<:=

$> = −)*+,

4./√2

One*must*extrapolate*to*+, = 0.We*measure*APV

at*+, = 0.025#GeV,.*

Reduced*asymmetry*more*convenient: Data*rotated*to*5HIJ = 0

08/01/2016 Armstrong**ECT*

Precision*Standard*Model*test

Page 5: DSA Trento clean - William & Maryphysics.wm.edu/~armd/DSA_Trento_clean.pdfMeeting*PVES*Challenges 08/01/2016 Armstrong**ECT* 6 B 180*μA*beam*current****(JLabrecord) B High*power*cryogenic*target

Qweak ran*from*Fall*2010*– May*2012***(Hall*C*at*JLab)**Four*distinct*running*periods:

• Hardware*checkout*(Fall*2010BJanuary*2011)• Run*0*(JanBFeb*2011)• Run*1*(Feb*– May*2011)• Run*2*(Nov*2011*– May*2012)

First*result

5

We*have*completed*and*unblinded the*analysis*of*“Run*0”*(about*1/25th of*our*total*dataset).*

$%&2 = −279 ± 35 OPQP ± 29#(OSO) ppb +, = 0.0250± 0.0006#GeV,

VJ8IW = 1155#MeV 58ZZ = 7.90#°

08/01/2016 Armstrong**ECT*

D.%Androic et#al.###Phys.%Rev.%Lett.%111%(2013)141803.%

Good*agreement*with*Standard*Model*prediction

In*this*talk,**I*focus*on*the*Run*1*&*Run*2*data

Page 6: DSA Trento clean - William & Maryphysics.wm.edu/~armd/DSA_Trento_clean.pdfMeeting*PVES*Challenges 08/01/2016 Armstrong**ECT* 6 B 180*μA*beam*current****(JLabrecord) B High*power*cryogenic*target

Meeting*PVES*Challenges

608/01/2016 Armstrong**ECT*

B 180*μA*beam*current* ***(JLab record)B High*power*cryogenic*targetB Rapid*helicity*reversal* **(960*Hz)B Small*scattering*angle:**toroidal*magnet,*large*acceptanceB GHz*detected* rates:*dataBtaking*in*integrating*modeB Radiation*hard*detectorsB Low*noise*18Bbit*ADCsB Exquisite*control*of*helicityBcorrelated* beam*parametersB Four*different* kinds*of*helicity*reversal:

Rapid****(Pockels cell*at*source)*Slow********(insertable λ/2*plate)*Ultra*slow***(WienBreversal,* **gB2*spin*flip)

B Two*independent* highBprecision* beam*polarimetersB High*resolution* Beam*Current*monitorsB Dedicated*Tracking*system*for*kinematics*determination

Page 7: DSA Trento clean - William & Maryphysics.wm.edu/~armd/DSA_Trento_clean.pdfMeeting*PVES*Challenges 08/01/2016 Armstrong**ECT* 6 B 180*μA*beam*current****(JLabrecord) B High*power*cryogenic*target

The*Qweak Apparatus

7

Main%detectors8Bfold%symmetry

Vertical%drift%chambers%(VDC)

(rotate)

Trigger%scintillator

Shield%wall

Lintels%

QTOR%

Lead%collar%

Cleanup%collimators%

Target

Tungsten%plug Horizontal%drift%

chambers%(HDC)(rotate)

Acceptance%defining%collimator%

QTOR%

08/01/2016 Armstrong**ECT*

Page 8: DSA Trento clean - William & Maryphysics.wm.edu/~armd/DSA_Trento_clean.pdfMeeting*PVES*Challenges 08/01/2016 Armstrong**ECT* 6 B 180*μA*beam*current****(JLabrecord) B High*power*cryogenic*target

• Main*detectorsToroidal*magnet* focuses*elastic*electrons*onto*each*bar– 8*Quartz*Cerenkov*bars*– Azimuthal*symmetry*maximizes*rates*& reduces*systematic* uncertainties– 2*cm*lead*preBradiators:****a)*reduce*soft*backgrounds*discovered* in*commissioning* ******************

b)*boost*signal* size**(but*cost*to*energy*resolution)

Main*Detectors

8

Simulation* of*scattering* rate*MD*face

Close*up*of*one*detector* in&situ

Measured

08/01/2016 Armstrong**ECT*

(see*Michael*Gericke’s talk)

Page 9: DSA Trento clean - William & Maryphysics.wm.edu/~armd/DSA_Trento_clean.pdfMeeting*PVES*Challenges 08/01/2016 Armstrong**ECT* 6 B 180*μA*beam*current****(JLabrecord) B High*power*cryogenic*target

35*cm,*2.5*kW*liquid*hydrogen*target*(world’s*highest* power*cryotarget)*Designed* using*Computational* Fluid*Dynamics*(see*Silviu Covrig’s talk)***• Temperature* ~20*K• Pressure:*30B35*psia• Beam*at*150*– 180uA

Hydrogen*Target

9

960*Hz*helicity*reversal* rate**(240*Hz*quartets)1/960*Hz*=*1042*\ssettling*time*after*reversal:* *112*\sintegration*time:**928*\s****(89%*live)

LH2*statistical*width*(per*quartet):•Counting*statistics:* 200*ppm•Main*detector*resolution: 92*ppm•BCM*width: 50*ppm•Target*noise/boiling: 37*ppm

228*ppm

Target*boiling*might*have*been*problematic!

MD*LH2*Asymmetry

08/01/2016 Armstrong**ECT*

Redundant,* lowBnoise*Beam*Current*Monitors*essential* *(see*Mark*Pitt’s*talk)

Page 10: DSA Trento clean - William & Maryphysics.wm.edu/~armd/DSA_Trento_clean.pdfMeeting*PVES*Challenges 08/01/2016 Armstrong**ECT* 6 B 180*μA*beam*current****(JLabrecord) B High*power*cryogenic*target

Originally,*was*expected* to*be*largest*systematic*uncertainty.

10

Møller polarimeter– Precise,*but*invasive– Thin,*polarized*Fe*target– Brute*force*polarization– Limited* to*low*current

Compton*polarimeter– Installed* for*QBweak– Runs*continuously*at*high*currents– Statistical* precision:* 1%*per*hour– Electron*Detector:*Diamond*strips

Detect*both recoil*electron*and*photon.

08/01/2016 Armstrong**ECT*

Beam*Polarimetry

Page 11: DSA Trento clean - William & Maryphysics.wm.edu/~armd/DSA_Trento_clean.pdfMeeting*PVES*Challenges 08/01/2016 Armstrong**ECT* 6 B 180*μA*beam*current****(JLabrecord) B High*power*cryogenic*target

Beam*Polarimetry

11

Good*agreement* between*Møller & Compton*(electron* detector)* ********Compton*photon*detector:* **issues*with*PbWO4*calorimeter* *(afterglow?)

Systematics:**B Compton (Edet)* :*#∆P/P*=*0.42%*B Møller:* #∆P/P*=*0.65%Combined Total:*******∆P/P*=*0.61%**(systematics +&statistics +&scaling)

08/01/2016 Armstrong**ECT*

Compton:*A.*Narayan*et*al,*Phys.*Rev.*X*6.011013*(2016)

Preliminary*Run*2*PolarizationCompton* *(Edet)***Møller

(see*Bob*Michaels’*talk)

Page 12: DSA Trento clean - William & Maryphysics.wm.edu/~armd/DSA_Trento_clean.pdfMeeting*PVES*Challenges 08/01/2016 Armstrong**ECT* 6 B 180*μA*beam*current****(JLabrecord) B High*power*cryogenic*target

HelicityBCorrelated*Beam*Parameters

12

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B Beam*Intensity*asymmetry:*active* (≈ 60#s scale)*feedback*system*(Pockels cell*voltage)B Careful*alignment* of*Pockels cell* in*source*essential:* ********

#→ smallest* position* differences*after*photocathode* yet*seen*at*JLab

B Did*not*(generally)*benefit* from*“kinematic* damping”:* **********************(theoretical* reduction*factor*~60)

B MisBmatched* beam*transport*distorts*phaseBspace* ellipseB One*time,*we*devoted*significant* time* to*allow*good*“matching”:*

did*see*suppression* of**helicityBcorrelated* differences*

(see*Arne*Freyberger’s and*Caryn*Palatchi’s talks)

Page 13: DSA Trento clean - William & Maryphysics.wm.edu/~armd/DSA_Trento_clean.pdfMeeting*PVES*Challenges 08/01/2016 Armstrong**ECT* 6 B 180*μA*beam*current****(JLabrecord) B High*power*cryogenic*target

HelicityBCorrector*Magnets

13

08/01/2016 Armstrong**ECT*

B Set*of*fast*pulsed*magnets* (5*MeV*region*of*injector)B Kick*beam*trajectory*with*helicity* (position* and*angle)B Measured* response*at*target:*stable,* *as*long*as*accelerator*tune*unchangedB “grad*student* feedback”*(daily)

Helicity*magnets*turned*on*

No*need*for*different*size*kicks*for*different* IWHP*(slow*flip)*states:*Good*setup*of*polarized*source*

Helicity*magnets*used*for*much*of*our*2nd run.

Page 14: DSA Trento clean - William & Maryphysics.wm.edu/~armd/DSA_Trento_clean.pdfMeeting*PVES*Challenges 08/01/2016 Armstrong**ECT* 6 B 180*μA*beam*current****(JLabrecord) B High*power*cryogenic*target

HelicityBCorrelated*Beam*Parameter*Sensitivities

14

08/01/2016 Armstrong**ECT*

Natural:*Linear*regression* of*natural*beam*motionDriven:*Drive*sinusoidal*

beam*oscillations*with*large*amplitude

Need*to*determine* the*sensitivities:*

Page 15: DSA Trento clean - William & Maryphysics.wm.edu/~armd/DSA_Trento_clean.pdfMeeting*PVES*Challenges 08/01/2016 Armstrong**ECT* 6 B 180*μA*beam*current****(JLabrecord) B High*power*cryogenic*target

Beamline*Background

15

08/01/2016 Armstrong**ECT*

Concern:%SmallBangle* scattered*beam*interacting*with*downsteam beamline* components∴ smallBaperture*WBCu*“beam*collimator’* *(1.6*kW*deposited* power)

Page 16: DSA Trento clean - William & Maryphysics.wm.edu/~armd/DSA_Trento_clean.pdfMeeting*PVES*Challenges 08/01/2016 Armstrong**ECT* 6 B 180*μA*beam*current****(JLabrecord) B High*power*cryogenic*target

Beamline*Background:*Halo*

16

08/01/2016 Armstrong**ECT*

Beam%Halo:B measured* beam*outside* of*13*mm*diameter*(intrinsic* beam*spot*150*\m)*B typically*10B7 to**10B6**of*beam,*but*varied*up*to*10B3 in*uncontrolled*manner.B could*interact* in*beam*collimator,* *generating*backgrounds*in*Main*Detector

Measured*directly*by*blocking*signal*electrons* at*primary*collimator:Typical*background*yield:* *0.2%*of*signal

But:##Halo*had*helicityBcorrelated* component* (position* and/or*intensity)

Large*halo*asymmetry*(up*to*20*ppm)*scaled*down*by*small* fraction**(0.2%)

Was*largest*systematic* error*in*our*“Run*0”*published* result* (23*ppb).

Causes* helicityBcorrelated* beam*sensitivities* measured* using* linear*regression*to*be*unstable* and*to*differ*from*the*(stable)*sensitivities* measured*using*driven*beam*motion.

Page 17: DSA Trento clean - William & Maryphysics.wm.edu/~armd/DSA_Trento_clean.pdfMeeting*PVES*Challenges 08/01/2016 Armstrong**ECT* 6 B 180*μA*beam*current****(JLabrecord) B High*power*cryogenic*target

P.M. King; Qweak; APFB2014 8

Qweak ApparatusProduction Mode:180 mA, Integrating

e- beam

E = 1.16 GeVI = 180 mAP = 88% Acceptance-defining

Pb collimator

35 cm LH2 target

Toroidal Spectrometer

High-density concreteshielding wall

Quartz Bar Detectors8-fold symmetry

08/01/2016 Armstrong**ECT* 17

Qweak upstream%luminosity%monitors%~*50%*of*their*signal*comes*from**“beamline*background”

Qweak diffuse%background%monitors%B in*focal*plane*at*locations*where*minimal*direct*signal*b ≈ 10*– 70%*of*signal*from*“beamline*background”

Background%detectors%measured%large%(up%to%20%ppm)%false%(only%partly%cancels%with%slow%reversals)%asymmetries

Beamline*Background:*Monitors

Page 18: DSA Trento clean - William & Maryphysics.wm.edu/~armd/DSA_Trento_clean.pdfMeeting*PVES*Challenges 08/01/2016 Armstrong**ECT* 6 B 180*μA*beam*current****(JLabrecord) B High*power*cryogenic*target

Beamline*Background:*Correlations

1808/01/2016 Armstrong**ECT*

1)*Measure*Main*Detector*to*Background*Detector*asymmetry*correlation*duringdataBtaking*(long*timeBscale* averaging)

2)*Confirm*correlation*with*blockedBoctant* **study.

3)*Using*correlation*slope*and*background*detector*asymmetry,*make*corrections

Asymmetries* from*different*background*detectors*highly*correlated*

Page 19: DSA Trento clean - William & Maryphysics.wm.edu/~armd/DSA_Trento_clean.pdfMeeting*PVES*Challenges 08/01/2016 Armstrong**ECT* 6 B 180*μA*beam*current****(JLabrecord) B High*power*cryogenic*target

Beamline*Background:*Corrections

19

08/01/2016 Armstrong**ECT*

Correcting*for*beamline* background*improves*statistical* consistency*of*data(correction*size:*3.6*ppb)

Page 20: DSA Trento clean - William & Maryphysics.wm.edu/~armd/DSA_Trento_clean.pdfMeeting*PVES*Challenges 08/01/2016 Armstrong**ECT* 6 B 180*μA*beam*current****(JLabrecord) B High*power*cryogenic*target

Secondary*Scattering

20

08/01/2016 Armstrong**ECT*

• Spin*precession* of*scattered*electron* in*QTor magnet:*some*transverse*polarization* *PT

• PT& analyzed*by*scattering* in*Pb preBradiators* *→##transverse* asymmetry*in*detectors:* **opposite*sign*in*the*two*PMTs* (*+#& −#)*in*each*detector

Adiff =&&$d −#$e Parity*Signal*=**:f*d#:g,

∴ Effect* cancels*to*first*order

• Analyzing*power*in*Pb:*1. BeamBnormal* single*spin*asymmetry**(high*energy):*2h#exchange2. Mott*scattering* (low*energy*in*shower)

Adiff is*of*same*scale*(hundreds*of*ppb)*as APV

Page 21: DSA Trento clean - William & Maryphysics.wm.edu/~armd/DSA_Trento_clean.pdfMeeting*PVES*Challenges 08/01/2016 Armstrong**ECT* 6 B 180*μA*beam*current****(JLabrecord) B High*power*cryogenic*target

Secondary*Scattering

21

08/01/2016 Armstrong**ECT*

• This*transverse* asymmetry*couples*with*position*&*angle*dependence* of*optical*response*of*detectors*

• Any*nonBcancellation* between*+ and*–PMTs:*detector* imperfections* &*nonBsymmetric*flux*distributions

• Optical*properties* and*flux*distributions*measured*with*tracking*system

• Quantifying*any*nonBcancellation*with*detailed*GEANT*4*simulation

• Any*nonBcancellation* likely*averages*down*in*the*8*independent* detectors

Last significant*systematic*uncertainty* to*quantify*before*we*unblind

Page 22: DSA Trento clean - William & Maryphysics.wm.edu/~armd/DSA_Trento_clean.pdfMeeting*PVES*Challenges 08/01/2016 Armstrong**ECT* 6 B 180*μA*beam*current****(JLabrecord) B High*power*cryogenic*target

Target*Windows

22

08/01/2016 Armstrong**ECT*

Background*from*detected* electrons* that*scattered*from*thin*Aluminum*entrance*and*exit*windows:

1. Measure*≈1600*ppb*asymmetry*from*thick*dummy*target**(identical* Al*alloy).**2. Precisely*measure*that*≈#2.8%*“dilution”* from*windows.

• Net*correction*is*≈25%*of*hydrogen*signal

Statistical* error:*4.3%Systematic*error:*0.7%

Plan*to*extract*the*27Al*elastic* asymmetry,

Theoretical* support*from*Chuck*Horowitz.

Aluminum*ParityBViolating*AsymmetryTwo*kinds*of*slow*flips:* IHWP*at*source*(IN/OUT)*and*Wien*filter

Page 23: DSA Trento clean - William & Maryphysics.wm.edu/~armd/DSA_Trento_clean.pdfMeeting*PVES*Challenges 08/01/2016 Armstrong**ECT* 6 B 180*μA*beam*current****(JLabrecord) B High*power*cryogenic*target

Target*Windows

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08/01/2016 Armstrong**ECT*

Dilution:%• Reduce*beam*current*to**<*1*\A• “Counting*mode”*measurement* of*rates*from*empty*target**and*full* lH2 target• Simulation* to*account*for*radiative*effects*on*window*signal*due*to*hydrogen

At*present* dilution*uncertainty* *2.8%*(relative).* **Errors*shared*equally*between:*• BCM*calibration• Detector*deadtime (unexpectedly* large)• Simulation*

Working*on*an*alternate* approach*that*essentially* eliminates* the*first*two*of*these.* Uses* lowBdensity* lH2 gas*target*data.*Challenge* is*density*determination.

Radiative* Corrections*to*Asymmetry:• Simulation* to*account*for*small* (8%)*kinematic* shift*in*asymmetry*for*

upstream*Al*window,**due*to*presence* of*lH2

Net*target*window*correction:*5%*relative*error*(on*25%*correction):*1.2%*error,dominated* by*statistics* on*Al*asymmetry*determination

Page 24: DSA Trento clean - William & Maryphysics.wm.edu/~armd/DSA_Trento_clean.pdfMeeting*PVES*Challenges 08/01/2016 Armstrong**ECT* 6 B 180*μA*beam*current****(JLabrecord) B High*power*cryogenic*target

To*determine*+,,*we*go*to*“tracking”*mode:• Currents*~*50*pA• Use*Vertical*+*Horizontal*Drift*Chambers• Reconstruct* individual*scattering*events

24

Correct* for*radiative effects* in*target*with*Geant 4*simulations,*benchmarked*with*gasBtarget*&*solid*target*studies

$%& = −)*+,

4./ 2+12 + 4 5, +, +,

Simulation* blueData*red

08/01/2016 Armstrong**ECT*

Kinematics*(Q2)*determination

One*challenge:* *no*beam*position*monitors*at*50*pA

SimulationData

Page 25: DSA Trento clean - William & Maryphysics.wm.edu/~armd/DSA_Trento_clean.pdfMeeting*PVES*Challenges 08/01/2016 Armstrong**ECT* 6 B 180*μA*beam*current****(JLabrecord) B High*power*cryogenic*target

Lessons*Learned*Summary

25

08/01/2016 Armstrong**ECT*

Secondary*scattering* from*preBradiatorsHelicityBcorrelated* halo*(leading* to*beamline*background)B need*“blocked*octant”*capabilityB multiple*background*detectors*B generated* in*injector?

Accelerator* Optics*matching*(kinematic*damping)Helicity*magnetsDriven*Beam*modulation*not*just*linear*regression* of*natural*beam*motionB coupling*of*driven*modulation*and*accelerator* feedback* systems

Wien*reversal*– not*as*passive*as*one*would*likeRedundant*polarimetryBCMs*and*BPMs*for*low*current:* tracking,*dilution*measurementsDetector*Deadtime (dilution)*Target*– great*success* (need* rapid*helicity*reversal*– Pockels cell*settling*time)*

Page 26: DSA Trento clean - William & Maryphysics.wm.edu/~armd/DSA_Trento_clean.pdfMeeting*PVES*Challenges 08/01/2016 Armstrong**ECT* 6 B 180*μA*beam*current****(JLabrecord) B High*power*cryogenic*target

Error*Summary

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08/01/2016 Armstrong**ECT*

B Final*result*will*be*statisticsBlimited* ****25× as*much*data*as*Run*0*result

B One*remaining*systematic*error* to*nail*down:*secondary*scattering*effect

B Other* leading*systematics*(in*order*of*decreasing*size):

• Q2 calibration• Target*Window*(Aluminum)*asymmetry• Beamline*Background• Target*Window*(dilution)• Polarimetry

Anticipate*unblinding the*result* in*a**few*months.

Page 27: DSA Trento clean - William & Maryphysics.wm.edu/~armd/DSA_Trento_clean.pdfMeeting*PVES*Challenges 08/01/2016 Armstrong**ECT* 6 B 180*μA*beam*current****(JLabrecord) B High*power*cryogenic*target

Reduced*Asymmetry

Hadronic part*extracted* through*global*fit*of*PVES*data.

27

in*the*forwardBangle*limit* (θ=0)

Armstrong**ECT*08/01/2016

V

V

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0.0 0.1 0.2 0.3 0.4 0.5 0.60.0

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Q

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Page 28: DSA Trento clean - William & Maryphysics.wm.edu/~armd/DSA_Trento_clean.pdfMeeting*PVES*Challenges 08/01/2016 Armstrong**ECT* 6 B 180*μA*beam*current****(JLabrecord) B High*power*cryogenic*target

Reduced*Asymmetry

Hadronic part*extracted* through*global*fit*of*PVES*data.

28

in*the*forwardBangle*limit* (θ=0)

Armstrong**ECT*08/01/2016

V

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0.0 0.1 0.2 0.3 0.4 0.5 0.60.0

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Page 29: DSA Trento clean - William & Maryphysics.wm.edu/~armd/DSA_Trento_clean.pdfMeeting*PVES*Challenges 08/01/2016 Armstrong**ECT* 6 B 180*μA*beam*current****(JLabrecord) B High*power*cryogenic*target

The*C1q &*the*neutron’s*weak*charge

29Armstrong**ECT*08/01/2016

0.22

0.24

-0.70 -0.65 -0.60 -0.55 -0.50 -0.45 -0.40

0.18 0.17

0.16

0.15

0.14 0.13

0.12

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1d

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-

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-

-

-

-

-

-

-

0.20

0.26

133Cs APV PVES

Inner Ellipses - 68% CLOuter Ellipses - 95% CL

ZW

Combining* this*result*with*the*most*precise* atomic*parity*violation*experimentwe*also*extract,* for*the*first*time,*the*neutron’s*weak*charge:

Page 30: DSA Trento clean - William & Maryphysics.wm.edu/~armd/DSA_Trento_clean.pdfMeeting*PVES*Challenges 08/01/2016 Armstrong**ECT* 6 B 180*μA*beam*current****(JLabrecord) B High*power*cryogenic*target

“Teaser”

3008/01/2016 Armstrong**ECT*

Page 31: DSA Trento clean - William & Maryphysics.wm.edu/~armd/DSA_Trento_clean.pdfMeeting*PVES*Challenges 08/01/2016 Armstrong**ECT* 6 B 180*μA*beam*current****(JLabrecord) B High*power*cryogenic*target

“Teaser”

3108/01/2016

Anticipated#precision#of#full#data#set

Armstrong**ECT*

Page 32: DSA Trento clean - William & Maryphysics.wm.edu/~armd/DSA_Trento_clean.pdfMeeting*PVES*Challenges 08/01/2016 Armstrong**ECT* 6 B 180*μA*beam*current****(JLabrecord) B High*power*cryogenic*target

A*suite*of*Auxiliary*Measurements

3208/01/2016 Armstrong**ECT*

Qweak has*data*(under*analysis)*on*a*variety*of*observables*of*potential*interest* for*Hadron physics:

• PV*asymmetry*for*elastic/quasielastic from*27Al• Beam*normal*singleBspin* asymmetry**for*elastic* scattering*on*proton• Beam*normal*singleBspin* asymmetry*for*elastic* scattering* on*27Al*&**12C*• PV*asymmetry* in*the*j → Δ region.• Beam*normal*singleBspin* asymmetry* in*the*j → Δ region.• Beam*normal*singleBspin* asymmetry*near*W=*2.5*GeV*• Beam*normal*singleBspin* asymmetry* in*pion*photoproduction• PV*asymmetry* in*inelastic* region*near*W=2.5*GeV*(related*to*hl box*diagram)*• PV*asymmetry* in*pion*photoproduction

*:*aka vector*analyzing*power**aka transverse*asymmetry;*generated*by*imaginary*part*of*twoBphoton*exchange*amplitude*

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33

D. Androic,1 D.S. Armstrong,2 A. Asaturyan,3 T. Averett,2 J. Balewski,4 J. Beaufait,5 R.S. Beminiwattha,6 J. Benesch,5F. Benmokhtar,7 J. Birchall,8 R.D. Carlini,5, 2 G.D. Cates,9 J.C. Cornejo,2 S. Covrig,5 M.M. Dalton,9 C.A. Davis,10 W. Deconinck,2

J. Diefenbach,11 J.F. Dowd,2 J.A. Dunne,12 D. Dutta,12 W.S. Duvall,13 M. Elaasar,14 W.R. Falk,8 J.M. Finn,2, T. Forest,15, 16 D. Gaskell,5M.T.W. Gericke,8 J. Grames,5 V.M. Gray,2 K. Grimm,16, 2 F. Guo,4 J.R. Hoskins,2 K. Johnston,16 D. Jones,9 M. Jones,5 R. Jones,17

M. Kargiantoulakis,9 P.M. King,6 E. Korkmaz,18 S. Kowalski,4 J. Leacock,13 J. Leckey,2, A.R. Lee,13 J.H. Lee,6, 2, L. Lee,10

S. MacEwan,8 D. Mack,5 J.A. Magee,2 R. Mahurin,8 J. Mammei,13, J.W. Martin,19 M.J. McHugh,20 D. Meekins,5 J. Mei,5 R. Michaels,5A. Micherdzinska,20 A. Mkrtchyan,3 H. Mkrtchyan,3 N. Morgan,13 K.E. Myers,20 A. Narayan,12 L.Z. Ndukum,12 V. Nelyubin,9

Nuruzzaman,11, 12 W.T.H van Oers,10, 8 A.K. Opper,20 S.A. Page,8 J. Pan,8 K.D. Paschke,9 S.K. Phillips,21 M.L. Pitt,13 M. Poelker,5J.F. Rajotte,4 W.D. Ramsay,10, 8 J. Roche,6 B. Sawatzky,5 T. Seva,1 M.H. Shabestari,12 R. Silwal,9 N. Simicevic,16 G.R. Smith,5

P. Solvignon,5 D.T. Spayde,22 A. Subedi,12 R. Subedi,20 R. Suleiman,5 V. Tadevosyan,3 W.A. Tobias,9 V. Tvaskis,19, 8

B. Waidyawansa,6 P. Wang,8 S.P. Wells,16S.A. Wood,5 S. Yang,2 R.D. Young,23 and S. Zhamkochyan 3

Spokespersons Project Manager Grad Students

97 collaborators 23 grad students10 post docs 23 institutionsInstitutions:

1 University of Zagreb2 College of William and Mary3 A. I. Alikhanyan National Science Laboratory 4 Massachusetts Institute of Technology5 Thomas Jefferson National Accelerator Facility6 Ohio University7 Christopher Newport University8 University of Manitoba,9 University of Virginia10 TRIUMF11 Hampton University12 Mississippi State University13 Virginia Polytechnic Institute & State Univ14 Southern University at New Orleans15 Idaho State University16 Louisiana Tech University17 University of Connecticut18 University of Northern British Columbia 19 University of Winnipeg20 George Washington University21 University of New Hampshire22 Hendrix College, Conway23 University of Adelaide

08/01/2016 Armstrong**ECT*

Qweak Collaboration

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Summary

34

########################$%&### = −279± 35 OPQP ± 29#(OSO) ppb

08/01/2016 Armstrong**ECT*

First#result# ##(4%#of#data#set):

Expect*final*result*in*a*few*months.

Will*be*statisticsBdominated.

The#weak#charges:

+m2 =***0.064*±#0.012*********+m

2 (SM)***=* 0.0710

+mn ## =**B0.975*± 0.010********+mn (SM)***=***B0.9890