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Magnet Target Detectors Beam (Phase I) (Phase II) The G 0 experiment : Doug Beck Spokesperson. Collaboration : Caltech, Carnegie-Mellon, W&M, Hampton,

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Magnet

Target

Detectors

Beam Beam

(Phase I) (Phase II)

The G0 experiment : Doug Beck Spokesperson. Collaboration : Caltech, Carnegie-Mellon, W&M, Hampton, IPN-Orsay, Kentucky, LPSC-

Grenoble, LaTech, NMSU, JLab, TRIUMF, U. Conn, U. Illinois, Manitoba, Maryland, U. Mass., UNBC, VPI, Yerevan, Zagreb

Outline of the talk

1/ G0 backangle phase

(intro)

2/ Report on 2006 data

taking

3/ Summary and 2006 plans

PAVI06 Workshop, Milos (Greece), May 17th, 2006

Serge Kox, LPSC Grenoble

G0 Experiments : Backangle running

EM and Weak form factors Elastic scattering of electron probes the nucleon via (EM) or Z0 (Weak) exchange

Flavor decomposition (assumption : 3 lightest quarks and charge symmetry)

MZ << M in the GeV region PV asymmetries in polarized elastic e-N scattering to extract the weak form factors

Nucleon structure and EW probes

(Q2)

e

N N

e jμW ,e

W ,N

(Q2)

N N

e e jμEM,e

EM,N

< N |J

μEM |N > → GE

,N ,GM,N

< N |J μW |N > → GE

(Z,N )

,GM

(Z,N )

< N |J μ5W |N > → GA

(Z,N)

GE,M

s = (1 - 4sin2θW )GE,M,p -GE,M

,n -GE,MZ,p

Role of the strange quark in the EM nucleon structure Strange quarks are the lightest non valence quarks of the sea

Excellent candidate to study the dynamics and influence of the sea

Signal investigated in PV experiments Charge and magnetization distributions

Static properties (μs, s) near Q2 = 0

Wide Q2 range to scan spatial distributions

G0 program : Physics case

s

Proton

gluon

uudu

u

s(ms < QCD)

The axial part in e-N scattering Tree-level + EW radiative corrections Parity-violating electromagnetic moment (FA)

Difficult to predict (multi-quarks processes) Q2 dependence

N- transition (dependence with Q2 MA) and pion production (EW rad.

corrections)

+ +

CEBAF and Hall C Polarized beam properties

Polarization 75 85 % Beam parity quality

G0 backangle (E, M separation) 2 ns beam structure, Ibeam up to 80 μA Non-standard energies (< 800 MeV) Shielding and Moeller settings

G0 experiments @ Jefferson Laboratory

G0 backward : 2 measurements scheduled in 2006 PAC 28 : common strategy with HAPPEX III (0.8 0.6 GeV2) Small Q2 acceptance : 2 different beam energies Measurements on LH2 and LD2 targets (M, A separation) mid-March to May and mid-July to December !!

Ee (MeV) Q2 (GeV2)

362 0.23

686 0.62

G0 Backward angle configuration

Particle detection and identification Turn-around of the magnet

Detection of the electrons (θe ~ 110°)

Extensive simulation of background Need for new shielding around the target cell and at the magnet exit window

Cryostat Exit Detectors (CED) to separate elastic and inelastic electrons

Cherenkov detector /e separation (both are recorded)

5 cm aerogel, n= 1.03 (OK for p < 380 MeV/c), 90% efficient for e- and rejection factor 100 From cosmic muons and test beam : 5-8 p.e. Special design for Magnetic shielding (SMS fringe field)

e- beamtarget

CED + Cherenkov

FPD

G0 beammonitorin

g

Superconducting Magnet (SMS)

Detectors (Ferris wheel)

FPD

Spokesman

Target service module

G0 in Hall C : The key elements

Detectors (Mini-Ferris wheel)CED+Cherenkov

Polarized source 85% polarization has been reached routinely using superlattice GaAs cathodes New Fiber laser for Hall C (adjustable pulse repetition rate)

Allows flexible time structure (1-2h for setting) : 32 ns used for Cherenkov study 780 nm is at polarization peak (P ~ 85%) for superlattice GaAs

Beam properties Hall C instrumentation OK 60 μA of low energy beam

New optics, beam dump and halo handled Parity quality beam properties

Adiabatic damping, PITA, RWHP, IA 35 h IN and 42 h OUT at 60 μA (LH2) Room for improvement (position feedback) Halo within a 6 mm diameter was determined to be < 0.3 x 10-6 (spec : 10-

6 )

2006 running : polarized electron beam

Beam Param. Achieved in G0

(IN-OUT)Specs

Charge asym. -0.4 ± 0.24 ppm 2 ppm

X-Y position diff. 20-24 ± 5 nm 40 nm

X-Y angle diff. -2 to -4 ± 2 nrad 4 nrad

Energy diff. 2 ± 4 eV 30 eV

Polarimetry and target

Moeller polarimeter in Hall C Energy smaller than 800 MeV (design)

Need to move quadrupoles closer to target Difficult tune (beam position, magnet settings)

Finally successful at 686 MeV 1 um foil = -86.36 +/- 0.36% (stat) 4 um foil = -85.94 +/- 0.33% (stat) Systematic error 2 %, expected to be reduced

Target and Lumi detectors LH2 and LD2 target

(“Flyswatter” and gas target for cell contribution) Target boiling test with Lumi detectors

Intensity up to 60 μA Very flat behavior (rates/beam current) Ratio LD2:LH2:12C are the ones expected

Pions

60 μA, LH2 10 μA, LD2

Particle ID : CED-FPD plane

(rates in Hz/μA per octant)

Electrons

Loss/random issue

Fraction (%) of loss I

LH2

60 μA

LD2

10 μA

Fraction (%) of random I2

Asymmetries : Electron and LH2 target

IN OUT

Asymmetries : Electron and LH2

IN OUT

(very) preliminary and unblinded

Summary of first data taking in 2006

First period of running at 682 MeV Commissioning and data taking … in a row !!

As usual a risky business and a scary/tough period !!

Many new features handled successfully Beam : low energy … but no compromise on intensity and Parity Quality New settings (polarimeter, target, …) New set-up (CED, Cherenkov, electronics …)

Analysis underway (remember this ended … 15 days ago !!)

Remained to be fixed for running in the Fall

Work/tests underway to reach 60 μA with LD2 Cherenkov (anode current and random coincidences)

Gas flow in diffusion box (CO2), gain/HV reduction, M > 2 CED-FPD (random/loss)

Use backplane scintillators of FPD counters (factor 5-10 reduction)

G0 Backward angle … What’s next in 2006

Still a long way to go … and maybe some new challenges at 362 MeV Halo issue (if due to processes in residual gas)

Test run underway this week at Jlab. May 16th : 60 μA delivered with small halo !!

Adiabatic damping More work on Moeller polarimeter

Hopefully by the end of 2006 …

+

Backup slides

Asymmetries : Pion plane and LH2

IN OUT

• Careful setup procedures for the Pockels cell using “HAPPEx method” were used• Special accelerator tuning techniques to achieve “adiabatic damping” were used• Position differences and charge asymmetries were minimized using the rotating half wave plate (RHWP) and adjusting Pockels cell voltages (PITA)• Further reduction in charge asymmetries was done with IA (intensity attenuator) cell• No position feedback was done; a “slow” feedback using PITA will be implemented in next run

• Beam “halo”: The fraction of the beam outside a diameter of 6 mm was determined to be < .3 x 10-6 under good running conditions.

Parity Quality Beam During G0 Backangle Run

Uses 1560 nm seed laser and amplifier commonly used in the telecommunications industry Electrical gain-switching avoids phase lock problems experienced with earlier optically modelocked systems Second harmonic generation device yields some 780 nm light from the 1560 nm light 780 nm is at polarization peak (P ~ 85%) for superlattice GaAs

slide courtesy of M. Poelker

New Fiber-Based Laser Used During G0 Backangle Running

Almost on-line from JLab

Tests performed at 362 MeV (but of interest for 686 MeV) Random/loss reduction in FPD

Octants 4 and 5 modified and factor 5-10 reduction indeed observed (left) LD2 target

pion/electron ratio decreased by a factor of 10 (right)