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The G 0 Experiment Allison Lung, Jefferson Lab representing the G 0 collaboration: Caltech, Carnegie-Mellon, William & Mary, Hampton, IPN- Orsay, ISN-Grenoble, JLab, Kentucky, LaTech, NMSU, TRIUMF, U Conn, UIUC, U Manitoba, U Maryland, U Mass, UNBC, VPI, Yerevan ~ 100 scientists from 19 institutions Our sponsors:

The G 0 Experiment Allison Lung, Jefferson Lab representing the G 0 collaboration: Caltech, Carnegie-Mellon, William & Mary, Hampton, IPN-Orsay, ISN-Grenoble,

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Page 1: The G 0 Experiment Allison Lung, Jefferson Lab representing the G 0 collaboration: Caltech, Carnegie-Mellon, William & Mary, Hampton, IPN-Orsay, ISN-Grenoble,

The G0 Experiment

Allison Lung, Jefferson Lab representing the G0 collaboration:

Caltech, Carnegie-Mellon, William & Mary, Hampton, IPN-Orsay, ISN-Grenoble, JLab, Kentucky, LaTech, NMSU, TRIUMF, U Conn,

UIUC, U Manitoba, U Maryland, U Mass, UNBC, VPI, Yerevan

~ 100 scientists from 19 institutions

Our sponsors:

Page 2: The G 0 Experiment Allison Lung, Jefferson Lab representing the G 0 collaboration: Caltech, Carnegie-Mellon, William & Mary, Hampton, IPN-Orsay, ISN-Grenoble,

What role do strange quarks play in nucleon properties?

Momentum ; Spin ; Mass ; Charge and Current

s

Main goal of G0 determine contributions of strange quark sea (s,s) to electromagnetic properties of the nucleon

"strange form factors"

Charge and current:

valence quarks

“non-strange” sea (u, u, d, d) quarks

“strange” sea (s, s) quarks

proton

gluon

uudu

u

s

?? | | sM

sE GGNssN

Page 3: The G 0 Experiment Allison Lung, Jefferson Lab representing the G 0 collaboration: Caltech, Carnegie-Mellon, William & Mary, Hampton, IPN-Orsay, ISN-Grenoble,

Z

N e

ZM

ZE

Z GGNJN , ||

neutral weak form factors

• Projected precision of NW form factors in 0.1 - 1 GeV2 Q2 range ~ 10% from the current generation of experiments (for magnetic)

Nucleon form factors measured in elastic e-N scattering• well defined experimental observables

• provide important benchmark for testing non-perturbative QCD structure of the nucleon

N e

ME GGNJN , ||

electromagnetic form factors

• Measured precision of EM form factors in 0.1 - 1 GeV2 Q2 range ~ 2 - 4%

Page 4: The G 0 Experiment Allison Lung, Jefferson Lab representing the G 0 collaboration: Caltech, Carnegie-Mellon, William & Mary, Hampton, IPN-Orsay, ISN-Grenoble,

STANDARDMODEL

COUPLINGS

Q QZ

u +2/3 1 8/3 sin2W

d 1/3 1 + 4/3 sin2W

s 1/3 1 + 4/3 sin2W

sin2W = 0.2312 ± 0.0002weak mixing angle

key parameter of Standard Model

sME

dME

uME

pZME

nME

pME GGGGGG ,,,

,,

,,

,, ,,,,

Invoke proton/neutron charge symmetry 3 equations, 3 unknowns

Neutral weak form factors strange form factors

psMEW

pdMEW

puMEW

pZME

Z

nsME

ndME

nuME

nME

psME

pdME

puME

pME

GGGGpJp

GGGGnJn

GGGGpJp

,,

2,,

2,,

2,,

,,

,,

,,

,,

,,

,,

,,

,,

sin3

41sin

3

41sin

3

81:||

3

1

3

1

3

2:||

3

1

3

1

3

2:||

Flavor decomposition of nucleon

E/M form factors:

ELECTROWEAKCURRENTS

i

iiZi

Z

iiii qqQJqqQJ

Page 5: The G 0 Experiment Allison Lung, Jefferson Lab representing the G 0 collaboration: Caltech, Carnegie-Mellon, William & Mary, Hampton, IPN-Orsay, ISN-Grenoble,

Parity Violating Electron Scattering - Probe of Neutral Weak Form Factors

polarized electrons, unpolarized target

unpol

AMEF

LR

LR AAAQGA

224

2

2

e e pp

)()()sin41()()()(

)()()(

222

222

22

QGQGAQGQGQA

QGQGA

MeAWA

MZMM

EZEE

eA

sM

sE

GGG

At a given Q2 , decomposition of GsE, Gs

M, GeA

requires 3 measurements:

Forward angle e + p (elastic)Backward angle e + p (elastic)Backward angle e + d (quasi-elastic)

Strange electric and magnetic

form factors,+ axial form factor

G0 will perform all threemeasurements at three

different Q2 values -0.3, 0.5, 0.8 GeV

Page 6: The G 0 Experiment Allison Lung, Jefferson Lab representing the G 0 collaboration: Caltech, Carnegie-Mellon, William & Mary, Hampton, IPN-Orsay, ISN-Grenoble,

The Nucleon's e-N Axial Form Factor GAe

eA

ZA

eA RFGG

Z0 has axial, as well as vector couplings we measure axial FF too

GAZ: neutral weak axial form

factor, determined from neutron decay and neutrino scattering

FA: nucleon’s anapole moment – parity-violating electromagnetic moment

Re: electroweak radiative corrections to e-N scattering

074.0~sin41gby multiplied 2ve W

+

+

Page 7: The G 0 Experiment Allison Lung, Jefferson Lab representing the G 0 collaboration: Caltech, Carnegie-Mellon, William & Mary, Hampton, IPN-Orsay, ISN-Grenoble,

Other Aspects of G0 Physics Program

NΔAG

Q2 (GeV2)

e + d quasielastic measurementsat back angles will map oute - N axial form factor GA

e

as a function of Q2

GAe (Q2) - e-N axial form factor

N Axial Transition Form Factor

data taken concurrently with backangle e + p elastic data-taking

• First measurement in neutral current process• sensitive to hadronic radiative corrections

Page 8: The G 0 Experiment Allison Lung, Jefferson Lab representing the G 0 collaboration: Caltech, Carnegie-Mellon, William & Mary, Hampton, IPN-Orsay, ISN-Grenoble,

Strange form factors - published results

SAMPLE at MIT-Bates:

40.035.014.0 )GeV1.0(

ppm60.070.055.7A :icquasielast d e

ppm73.061.092.4A :elastic p e

22

d

p

QG sM

HAPPEX at Jefferson Lab:

22 GeV 0.48 Qat

014.0020.0025.039.0

ppm56.098.005.15 :elastic p e

sM

sE

p

GG

A

D2

H2

Zhu

, et a

l.

(updated results, publication in progress)

Page 9: The G 0 Experiment Allison Lung, Jefferson Lab representing the G 0 collaboration: Caltech, Carnegie-Mellon, William & Mary, Hampton, IPN-Orsay, ISN-Grenoble,

G0 Experimental Program

• 1st Engineering Run we are here

• 2nd Engineering Run

• Forward angle measurement

• Expected Results: (GE

s + GMs) for 7 values of Q2 between 0.1 – 1.0 (GeV/c)2

• 3 Backward angle measurements• Expected Results: Separated GE

s , GMs , and GA

e for Q2 of 0.3, 0.5, and 0.8 (GeV/c)2

N axial transition form factor

Page 10: The G 0 Experiment Allison Lung, Jefferson Lab representing the G 0 collaboration: Caltech, Carnegie-Mellon, William & Mary, Hampton, IPN-Orsay, ISN-Grenoble,

Statistics (5% 1013 - 1014 events):• high e- polarization (70-80%) • high e- current (40 Amps)• high luminosity (2.1 x 1038 cm-2 s-1)• large acceptance detector (0.5-0.9 sr)• long target (20 cm)• high count rate capability detectors/electronics (1 MHz)

Systematics (reduce false asymmetries, accurately measure dilution factors):

• small helicity-correlated beam properties• ability to isolate elastic scattering from other processes

statistics ~55%-75% of total error on separated GEs and GM

s

General Experimental Requirements

measure APV ~ -3 to -40 ppm with precision APV /APV ~ 5%

Page 11: The G 0 Experiment Allison Lung, Jefferson Lab representing the G 0 collaboration: Caltech, Carnegie-Mellon, William & Mary, Hampton, IPN-Orsay, ISN-Grenoble,

The G0 Experiment in Jefferson Lab Hall C

All New Hall C Equipment:Superconducting toroidal magnet – Univ of Illinois

High power H2 /D2 targets – Caltech, UMd, JLab

Scintillator detector array – French/Canadian/NAmerican Custom electronics – Orsay, Grenoble, CMU

Jefferson Lab polarized source - JLab

Design and Construction (1993–2001)

Installation (Fall 2001–Fall 2002)

Page 12: The G 0 Experiment Allison Lung, Jefferson Lab representing the G 0 collaboration: Caltech, Carnegie-Mellon, William & Mary, Hampton, IPN-Orsay, ISN-Grenoble,

detector

April ‘02

G0 installed in Hall C at JLab

August ‘02

beamlinemonitors

magn

et

target service vessel

cryogenic supply

detectors (Ferris wheel)

Page 13: The G 0 Experiment Allison Lung, Jefferson Lab representing the G 0 collaboration: Caltech, Carnegie-Mellon, William & Mary, Hampton, IPN-Orsay, ISN-Grenoble,

G0 Forward Angle Measurement

• Electron beam energy = 3 GeV on 20 cm LH2 target

• Detect recoil protons ( ~ 62 - 78o corresponding to 15 - 5o

electrons)

• Magnet sorts protons by Q2 in focal plane detectors

• Full desired range of Q2 (0.16 - 1.0 GeV2) obtained in one setting

• Beam bunches 32 nsec apart (31.25 MHz = 499 MHz/16)

• Flight time separates p (about 20 ns) and + (about 8 ns)

lowest Q2

highest Q2

French octant

Page 14: The G 0 Experiment Allison Lung, Jefferson Lab representing the G 0 collaboration: Caltech, Carnegie-Mellon, William & Mary, Hampton, IPN-Orsay, ISN-Grenoble,

G0 Superconducting Magnet System

(2 0.44 ~ acceptance

35

Tm 6.1

bend

dlB

Superconducting toroidal magnet:

8 coils ; common cryostat

• Initial manufacturing defects repaired in early 2002 • Ran at 4500 A initially (Aug. - Dec. 2002)• Ran at full design current (5000 A) during Jan 2003 run

Page 15: The G 0 Experiment Allison Lung, Jefferson Lab representing the G 0 collaboration: Caltech, Carnegie-Mellon, William & Mary, Hampton, IPN-Orsay, ISN-Grenoble,

G0 Target

• 20 cm LH2 cell, 250 W heat load from beam at 40 A• High flow rate to minimize target density fluctuations• Observed target density fluctuations at 40 A negligible

Normal running

Heat Exchanger

Target cellCryogenic pump

High power heater

Page 16: The G 0 Experiment Allison Lung, Jefferson Lab representing the G 0 collaboration: Caltech, Carnegie-Mellon, William & Mary, Hampton, IPN-Orsay, ISN-Grenoble,

G0 Focal Plane Detectors (FPD)

• 8 octants ; 256 signals total• 16 pairs of arc-shaped scintillators each• back and front coincidences to eliminate neutrals• 4 PMTs (one at each end of each scintillator)• long light guides (PMT in low B field)

North American octant

Detector “Ferris Wheel"

front

back

Detector “Ferris Wheel"

Page 17: The G 0 Experiment Allison Lung, Jefferson Lab representing the G 0 collaboration: Caltech, Carnegie-Mellon, William & Mary, Hampton, IPN-Orsay, ISN-Grenoble,

G0 Forward Angle Electronics

PMT Left

PMT Right

PMT Left

PMT Right

MeanTimer

MeanTimer

Coinc

TDC /LTD

Time histogramming

Time resolution 250 ps / 1ns

Time of Flight measurement

Front

Back

NA LTD crate (1/2) French DMCH16 Module 1/8

• Custom electronics designed to provide high-rate histogramming• NA: mean timer latching time digitizer scalers (1 ns)• French: mean timer flash TDCs (0.25 ns)• Time histograms read out by DAQ system every 33 msec

Page 18: The G 0 Experiment Allison Lung, Jefferson Lab representing the G 0 collaboration: Caltech, Carnegie-Mellon, William & Mary, Hampton, IPN-Orsay, ISN-Grenoble,

G0 Beam• Requires unusual time structure: 31 MHz (32 nsec between pulses) (1/16 of usual CEBAF time structure of 499 MHz (2 nsec between pulses)

• Required new Ti:Sapphire laser in polarized electron gun

• Higher charge per bunch space charge effects complicated beam transport in injector (challenging beam optics problem)

• Beam quality closest to operating specs during Jan 2003 delivery• Beam current 40 A• Beam fluctuations at (30 Hz/4) ~ X, Y < 20 m I/I < 2000 ppm

• Ongoing Beam Work• multiple Hall delivery• beam position feedback• reliable control of helicity-correlated properties

CEBAF polarized injector

Page 19: The G 0 Experiment Allison Lung, Jefferson Lab representing the G 0 collaboration: Caltech, Carnegie-Mellon, William & Mary, Hampton, IPN-Orsay, ISN-Grenoble,

Data-taking and polarization flip sequenceData readout interval = ( 1 / 30 Hz ) = 33 msec detector TOF histograms recorded integrated values of beam monitors (charge and position) recorded

21212121

2121

1quartet

X x

s)differenceposition (beam sdifference : intensity)or yield(detector asymmetry

pattern) random-(pseudo sequence flipn polarizato beamelectron

XXXYYYY

YYYYA

x:x~ 9 m

y:y~ 10 m

AI:~ 870 ppm

Typical differenceand charge asymmetryhistograms

Page 20: The G 0 Experiment Allison Lung, Jefferson Lab representing the G 0 collaboration: Caltech, Carnegie-Mellon, William & Mary, Hampton, IPN-Orsay, ISN-Grenoble,

Systematics: from raw asymmetry to physics results

PPP

PAA

i

N

iiP

YYmeascorr i

where

1

21

2121

2121

YYYY

YYYYAmeas

Form raw measured asymmetry from the detector yields:

Correct for false asymmetries from helicity-correlated beam properties:

Correct for background and its asymmetry:

sig

backbackcorrsig f

fAAA

),,,(2 sM

sEMEphys GGGGfQA

• helicity-correlated beam properties• deadtime corrections

• background dilution factor correction

Correct for beam polarization and radiative corrections:

radbeam

corrphys RP

AA • electron beam polarization

• electromagnetic radiative corrections

Correct for measured Q2 and EM form factors:

• <Q2> determination• electromagnetic form factors

Page 21: The G 0 Experiment Allison Lung, Jefferson Lab representing the G 0 collaboration: Caltech, Carnegie-Mellon, William & Mary, Hampton, IPN-Orsay, ISN-Grenoble,

Time of Flight Spectra from G0 Engineering Run

16 detectors of a single octant-t.o.f recorded every 33 msec-good spectra for all octants, all detectors

1 2 3 4

6 7 8

9 10 11

12

13 14 15 16

5

pions

inelastic protons

elastic protons

Det 8

Page 22: The G 0 Experiment Allison Lung, Jefferson Lab representing the G 0 collaboration: Caltech, Carnegie-Mellon, William & Mary, Hampton, IPN-Orsay, ISN-Grenoble,

Behavior of raw asymmetry results underslow half wave plate reversal

North American detectors and electronics

French detectors and electronics

Based on51 hoursof data at40 A

Jan 2003EngineeringRun

No unexpected falseasymmetries seen

Page 23: The G 0 Experiment Allison Lung, Jefferson Lab representing the G 0 collaboration: Caltech, Carnegie-Mellon, William & Mary, Hampton, IPN-Orsay, ISN-Grenoble,

Asymmetry results from Jan. 2003 Engineering Run

• Based on 51 hours of data at 40 A (note: full production run will be 700 hours)

• Includes

• false asymmetry corrections• deadtime corrections• background corrections• beam polarization correction

increasing Q2

Page 24: The G 0 Experiment Allison Lung, Jefferson Lab representing the G 0 collaboration: Caltech, Carnegie-Mellon, William & Mary, Hampton, IPN-Orsay, ISN-Grenoble,

1st Engineering Run - successfully completed

Current Work– False Asymmetries

– Helicity correlated beam charge effects (goal <1ppm over 700 hours)

– Helicity correlated beam position effects (goal <20 nm over 700 hours)

– Deadtime– typical deadtime ~10% with rates of ~1-2 MHz/detector– causes false asymmetries when combined w/nonzero charge

asymmetry

– uncorrected effect ~15% ; after correction ~1% ; Afalse ~0.01ppm

– Background Determination– requires both yield and asymmetry of background– yield ~10-25% depending on detector

– |Aback| ~ |Aelastic| near elastic peak (preliminary)

Page 25: The G 0 Experiment Allison Lung, Jefferson Lab representing the G 0 collaboration: Caltech, Carnegie-Mellon, William & Mary, Hampton, IPN-Orsay, ISN-Grenoble,

G0 Backward Angle Measurement

• detect scattered electrons at e ~ 110o

• need three runs each for LH2 and LD2 at E = 424, 576, 799 MeV for Q2 = 0.3, 0.5, 0.8 (GeV/c)2

(total of 6 runs x 700 hours each)

Requires additional hardware:• Cryostat Exit Detectors (CED) to separate elastic and inelastic electrons used in coincidence with FPDs• Cerenkov detector for pion rejection (primarily for LD2 target)• additional electronics • LD2 target

Requires physical turn-around:

Electron beam

Detectors

Magnet

Page 26: The G 0 Experiment Allison Lung, Jefferson Lab representing the G 0 collaboration: Caltech, Carnegie-Mellon, William & Mary, Hampton, IPN-Orsay, ISN-Grenoble,

Near Future • 2nd G0 engineering run in Oct-Dec 2003• Forward angle production run in Feb 2004Hopefully by late 2004 we can compare world's forward angle data….

Page 27: The G 0 Experiment Allison Lung, Jefferson Lab representing the G 0 collaboration: Caltech, Carnegie-Mellon, William & Mary, Hampton, IPN-Orsay, ISN-Grenoble,

Back angle running starting early in 2005

…..and a few years later, we can present a wide Q2 range of separated form factors

Future

+ MAMI A4 data

Page 28: The G 0 Experiment Allison Lung, Jefferson Lab representing the G 0 collaboration: Caltech, Carnegie-Mellon, William & Mary, Hampton, IPN-Orsay, ISN-Grenoble,

SUMMARY• G0 has a broad experimental program that will

result in the first separated values of GEs, GM

s, and GA

e over a wide range of Q2

• 1st G0 Engineering Run successfully completed– all hardware operational

– obtained ~2 days of test asymmetry data

– clearly see weak interaction

– no unexpected false asymmetries seen

• On track to resume running in October 2003

• Look forward to first physics results late 2004