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The BESIII Luminosity Monitor

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Dept. of Modern Physics,USTC. P.O.Box 4 Hefei, 230027. BES-III Workshop ... Track distribution 20 cm away from the Al surface. Effective Al thickness = 35 mm ... – PowerPoint PPT presentation

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Title: The BESIII Luminosity Monitor


1
The BESIII Luminosity Monitor
  • High Energy Physics Group
  • Dept. of Modern Physics,USTC
  • P.O.Box 4 Hefei, 230027

2
Side view of the near IP region
3
(No Transcript)
4
Channels to Measure Luminosity
  • The Bhabha Channel
  • ee- ? ee- (? ) at small angle with
  • respect to the IP and beam
  • Lowest Order Diff. Cross Section
  • d? /dcos? ? ?2(3cos2 ?)2/8Eb2(1-cos?)2

5
Event rate estimation for 3 ? regions(Assume L
1033cm-2s-1, Ebeam1.55GeV, ? 2 ? covered)
  • Extreme Forward Region (5o to 16o )
  • Event Rate 12743 Hz
  • End Cap Region (21o to 34o )
  • Event Rate 412 Hz
  • Barrel Region (34o to 146o)
  • Event Rate 423 Hz

6
LUM Type I Extremely Forward Luminosity Monitor
  • The Defining and Complimentary Counter
  • Dimension of ? Scintillation fiber
  • or Silicon
    Strips
  • Dimension of f Plastic scintillator
  • The Calorimeter
  • BGO / PWO Crystal

7
Requirement on space resolution
  • The precision requirement on the inner edge of
    the tracker part should be 160 ?m for
  • a tracker put at Z 41.6cm To make the
    Bhabha event accepted within a 1 change
  • (This also sets installation precision of
    the micro-beta magnet If it is around 1 mm,
    error of luminosity measured gt 6)

8
Arrangement of the EFLM
9
LUM Arrangement(Tracker not plotted)
10
Front View of Defining/Complimentary Counter
11
Cross Section of Fiber Bunch
12
Separation Power of the Calorimeter
13
Effects of the support Al structure of the MDC
  • Effective thickness of the Al plate and tube
  • 25 to 50 mm for different angles
  • Al plate 20 mm , Al tube surround the beam pipe
    2mm
  • R.M.S of the track smearing for the case
  • of 45mm thick Al case 0.905 mm
  • Corresponding to a 7 of error in event count

14
Track distribution 20 cm away from the Al
surfaceEffective Al thickness 35 mm
15
Track deflection by the AlEffective thickness
45 mm
16
Secondary charge track numbers due to
AlEffective Al thickness 45 mm
17
Error estimate for track smearingand
installation precision
  • Track smearing due to Al
  • 6
  • Assuming a 1mm error in the installation
    precision of the micro-beta magnet
  • 6
  • Total effect
  • gt 8

18
LUM Type IIZero Degree Luminosity Monitor
  • Luminosity Monitor Based on e-(e)single
    Bremsstrahlung(SB)
  • The photons ? are emitted along the e-(e)
    direction within a cone of total aperture of
    (me/Eb) with cylindrical symmetry, where Eb and
    me is energy of beam and mass of electron
    respectively.

19
Position of the ZDLM
20
Photon energy
  • Maximum energy
  • ? is the total energy in the center of
    momentum system. For BES3 of BEPC2, the cone of
    total aperture of photon radiated is about 0.33
    mrad.and kmax is 1550MeV
  • if Ebeam 1.55GeV

21
Formula for Luminosity calculation
  • If a photon detector is located coaxially
    with the incident beam line and is subtended to
    IP with a solid angle of ?D, the counting rate of
    NsB(kt) is measured the luminosity can be
    obtained by

22
Photon energy spectrum with different Kt
23
Angular distribution for different Kt
24
The acceptance and the rate estimationSuppose a
calorimeter is located behind the splitter
magnets at the position of 10 meter away from the
IP. An aperture of ?20 mm lead collimator coaxial
with the incident beam line is assembled in the
cross sections of the calorimeter with various
photon energy cuts kt
25
kt dependence of FAC(kt). Its shown that the
total aperture of 2 mrad for the calorimeter is
able to accept more than 87 of the SB-photons
for ?lt 1mrad. 66 for ?lt0.5mrad.
26
(No Transcript)
27
Background
  • Beam gas Bremsstrahlung (GB) background. The
    calorimeter faces the direction of the incident
    ebeam, so that the beam gas Bremsstrahlung in
    the IP region (30meter straight part) is the
    main background of SB photonGB-background. GB
    has a very similar energy spectrum and angular
    distribution with the SB photon

28
Energy spectrum of GB photonsAssuming 10-7 mmHg
vacuum in the 30 m long chamber
29
Background caused by beam lost
  • The lost beam (BL) hits the vacuum chamber, the
    spread secondary photons and electrons would be
    another background source of SB counting. A veto
    counter, which is sensitive to charged particles
    in the front of the calorimeter, could
    effectively suppress the secondary charged
    particles and make the beam lost background
    negligible.

30
Calorimeter system
  • The SB photon rates are so high, Its
    difficult to count photons one by one, doing
    energy analysis is apparently impossible. We
    could not be able to set kt cut for readout
    electronics. So absolute luminosity measurement
    based on SB process is hardly to do. High SB
    photon flux is an advantage for relative
    luminosity monitoring, the integrated currents
    output from the photon calorimeter will be a
    relative measurement for the real time luminosity.

31
  • Detector GSO crystal 5515cm3 coupled
    with photodiode.
  • The high flux of SB photons (from 10 to
    1550 MeV) will deposit their energies in the
    crystal and the absorb dose will be up to 0.23
    Mrad/day. So that the radiation hardness of GSO
    should be good.

32
The photo-diode Hamamstsu S3584-09 will be
coupled through the air light guide and concave
mirror to the GSO like the Belle design
33
The sensitivity to the parameters of IP,
transverse positions (x,y) and crossing angles
  • Fixing the e beam 11mrad relative to z axis
    and the e- beam 11mrad relative to z axis, the
    axis of the calorimeter, which faces the IP and
    subtends a half angle of ?,is coincided with the
    axis of incident e- beam, steering the e- beams
    axis deviated from the original axis with an
    amount of ??

34
Factor of photons accepted changes due to
crossing angle error (1mrad acceptance)
35
Factor of photons accepted changes due to
crossing angle error (0.5mrad acceptance)
36
The relative acceptance changes with the ?x
(1mrad acceptance)
37
The relative acceptance changes with the ?x
(0.5mrad acceptance)
38
Conclusion
  • The EFLM can be used as a relative luminosity
    online monitor for BESIII while
  • the precise value of luminosity can be
    completed by end cap and barrel detectors.
  • SB photons measurement by the ZDLM can be used
    as a sensitive real time and relative luminosity
    monitor for BEPC2
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