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Lepton Polarisation at HERA

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A brief overview of lepton polarisation - its use and measurement at HERA, ... Telescope resolution and beam collimation are small factors in comparison to MCS ... – PowerPoint PPT presentation

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Title: Lepton Polarisation at HERA


1
Lepton Polarisation at HERA
  • A brief overview of lepton polarisation - its use
    and measurement at HERA, including testbeam
    analysis of the performance of the upgraded
    Transverse Polarimeter (TPOL).
  • Chris Collins-Tooth (ZEUS, IC-London)

2
Outline
  • Lepton Beam Polarisation - how, why?
  • Measurement of Polarisation - currently, and in
    the future.
  • Test Beam setup of the Telescope and Transverse
    Polarimeter
  • What is the Telescope and what does it do?
  • What data was gathered?
  • Analysis of the data
  • Multiple Coulomb Scattering, Beam spread, and
    Telescope resolution
  • Relative rotations
  • between parts of the Telescope
  • between the Telescope and the TPOL silicon
  • What can be done about these factors?
  • What does this tell us about the TPOL silicon -
    resolution,efficiency?
  • Conclusions

3
Lepton Beam Polarisation
  • Relativistic e/- emit synchrotron radiation in
    curved portions of a storage ring.
  • Emission can cause spin flip.
  • and flip rates differ.
  • e- become polarised antiparallel to the guide
    field, e become polarised parallel to field.
  • P(t) Pst 1-exp(-t/Tst) (N
    -N )/(N N )
  • Pst was 0.51 at HERA
  • Tsttime-constant 20min

60
P()
50
40
30
20
10
0
-10
t(min)
4
Why is polarisation important?
  • More accurate knowledge of polarisation state of
    beam will allow new physics to be investigated
    e.g.
  • Standard Model no right handed Charged Currents
    (WL / W-R ).
  • Plotting sCCobs(P) allows direct measurement of
    right-handed W-R mass. - present limit is 720GeV
    set in 10/2000 by D0.
  • Neutral Current (Z0,g ) cross sections split into
    4 at high Q2 if Leptons polarised.
  • This allows measurement light quark Neutral
    Current couplings vu vd au ad .
    (complimentary to LEP b,c quarks).

5
How is polarisation currently measured?
  • Transversely polarised leptons collide with
    circularly polarised laser light to give
    angular asymmetry.
  • Angular asymmetry translates to spatial
    asymmetry.
  • Compton-scattered photons enter calorimeter.
  • Calorimeter is in two halves to measure up-down
    energy asymm.
  • Polarisations measured to 6 (photon position
    measured to within 1000 mm)
  • Upgrade will improve accuracy.

6
What does the prototype TPOL look like?
  • Only changes to calorimeter section of TPOL.
  • New 1cm2 Si strip detector in front of
    calorimeter (80 mm pitch for horizontal strips).
  • Due to small beam spot radiation damage may
    occur.
  • Movable scintillating fibre to calibrate Si
    response over 5yr lifetime.
  • Production TPOL has 6x6cm2 Si strip detector,
    with horizontal and vertical strips (just tested
    at CERN).

7
Test Beam setup
TPOL
Telescope
  • 6 GeV e- beam enters from left
  • e- beam passes through Telescope then moves into
    the TPOL
  • Telescope mounted as close to TPOL as possible on
    movable table
  • Telescope has 3 position sensitive detectors
    T1,T2 and T3 (Td was dead material being used
    for a second experiment)

8
The Telescope
  • Previously, degree of polarisation estimated
    using energy asymmetry in calorimeter
    (Calorimeter resolution 1000 ?m)
  • Now measure polarisation using 80 ?m pitch Si
  • Something more accurate needed to probe TPOL
    silicon resolution - the Telescope.
  • 3 planes of 50 ?m pitch Si, with horizontal and
    vertical strips.
  • T1,T2,T3 detectors roughly 3cm 3cm (TPOL
    silicon 1 cm2)

9
The data
  • T1,T2,T3 used to predict Si strip to fire.
  • As expected, fitted line has slope 1 ? 0.01
  • Offset simply due to T1,2,3 being physically
    larger than TPOL Silicon
  • Width of data about fitted line gives indication
    of TPOL resolution

10
The width
  • Width 132.15 2.93 ?m
  • TPOL Silicon strip pitch 80 ?m
  • Intrinsic resolution 80/?12 ?m

0
0
400
-400
800
-800
11
Analysis of the data
  • Observed width does not relate directly to the
    TPOL resolution
  • Multiple Coulomb Scattering (MCS) of e- beam at
    T1,Td,T2,T3 and TPOL Aluminium Box
  • Finite resolution of the Telescope
  • e- beam not 100 collimated
  • Misalignments of the Telescope detectors T1,T2,T3
  • Misalignments of the Telescope (as a whole) and
    the TPOL

12
Telescope internal misalignment
  • T1,T2 and T3 could all be misaligned with respect
    to each other.
  • Rotations would produce systematic shifts of
    predicted minus actual strip firing from
    left-to-right
  • Most important are rotations about beam-axis
    (pictured). A 0.08o rotation would cause a shift
    of 1 strip across breadth of detector

13
Predicted minus Actual shifts for T3,T2 and T1
from L?R
T3
T2
T1
  • Using T1,T2 to predict T3 (left) we observe a
    shift from left to right of approximately 50
    microns

14
Correction of misalignment
  • Iterative process invoked
  • Rotating T3 by 0.27o flattened off all the plots
    (to within errors)

15
TPOL misalignment
  • The TPOL silicon had no vertical strips
  • Track through T1,T2,T3 used to predict vertical
    strip to fire to give indication of horizontal
    position of impact
  • No discernable shift observed before or after T3
    rotation applied
  • Correction for rotations caused no discernable
    reduction in observed width

16
MCS, Telescope resolution and beam collimation
  • Simple Monte-Carlo simulation using PDG formula
    for MCS with gaussian width
    ?s(13.6MeV/?cp) ?(x/Xo) (10.038 ?n x/ Xo)
  • Telescope resolution and beam collimation are
    small factors in comparison to MCS
  • Together, all these factors contribute 102 ?m to
    the width
  • Subtracting in quadrature, the TPOL resolution
    obtained is ?(1322-1022) ?83 ?m
  • But - MCS is not actually gaussian.
  • Attempted to use GEANT to improve estimate

17
GEANT v3.13
  • Geant v3.13 used to simulate MCS through 5
    surfaces
  • Gives width of 138 ?m 1.5
  • cf Observed width 132 ?m 3
  • There are other errors on this simulation, 1.5 ?m
    only statistical error.
  • Consistent with good performance of TPOL Silicon.

18
Error propagation
T1
T2
Td
T3
Al
T4 (TPOL)
m3
m3
m3?3
z
  • Alternative approach to Monte-Carlo
  • Use errors introduced by MCS etc., and propagate
    them to the TPOL silicon
  • T4T3Z4m3Z4?3(Z4-ZAl)?Al
  • ?Var(T4)Var(T3)Z42Var(m3)Z42Var(?3)(Z4-ZAl)2Va
    r(?Al)Z4Cov(T3,m3)
  • T3T1-Z1m3-Zd?d-Z2?2
  • ?Var(m3)(1/Z12)(T1-T3-Zd?d-Z2?2)
  • Variances are calculated, (e.g.
    Var(T1,T2,T3)?2T1,T2,T3 208 ?m)
  • ?T4?Var(T4)120 ?m Error on TPOL Si due to
    uncertainties in Telescope
  • Resolution of TPOL Si ?1322-120255 ?m

19
TPOL Resolution
  • Obviously other effects (eg MCS) mask the
    resolution, so we can only say that TPOL Si
    results are consistent with theory.
  • From Monte-Carlo Simulation with PDG formula we
    obtain RTPOL? 83 ?m
  • From Error Propagation we obtain RTPOL? 55 ?m

20
TPOL Silicon Efficiency
Ratio of hits NOT registering in TPOL
  • Telescope used to predict TPOL events
  • Efficiency is the ratio of
  • events with TPOL Silicon signal
  • events predicted by Telescope
  • TPOL Silicon edges found by looking at ratio of
    hits not registering in the TPOL as a function of
    position
  • Log plot reveals edges where Telescope predicts
    TPOL hits but TPOL does not register
  • Horizontal edges at 13000 20000 ?m
  • Vertical edges at 11000 18000 ?m
  • Consistent with active area of Silicon

Horizontal Position (?m)
Vertical Position (?m)
21
Efficiency cuts
  • Using the edges from previous slide, we must
    remove predicted events from efficiency
    calculations where they miss the boundaries of
    the TPOL Si
  • Figures show
  • events predicted by the Telescope and registered
    by the TPOL (black)
  • For effect, events in red are added. They are
    predicted events which had no TPOL response, but
    the event was inside the opposite direction
    boundary, and so should have registered.
  • Clearly, the boundaries look correct.

22
Final Efficiency
  • With the positional cuts made, the efficiency of
    the TPOL silicon can be calculated
  • This is the ratio of
  • events with a TPOL silicon response
  • all predicted events inside the boundary
  • The efficiency is uniform across the detector, at
    97.8

23
Conclusions
  • Upgrade should improve accuracy of asymmetry
    measurement.
  • Currently aiming for better than 1 error on P(t)
  • Misalignments, Coulomb Scattering and other
    factors contribute significantly to observed
    width of 132 ?m.
  • TPOL Silicon resolution TBA but preliminary
    studies suggest 55 and 83 ?m
  • TPOL Silicon efficiency spatially uniform at
    97.8
  • More accurate knowledge of polarisation state of
    beam will allow new physics to be investigated
    e.g.
  • Standard Model no right handed Charged Currents
    (WL / W-R ).
  • Plotting sCCobs(P) allows direct measurement of
    right-handed W-R mass. - present limit is 720GeV
    set in 10/2000 by D0.
  • Neutral Current (Z0,g ) cross sections split into
    4 at high Q2 if Leptons polarised.
  • This allows measurement light quark Neutral
    Current couplings vu vd au ad . (complimentary to
    LEP b,c quarks).

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