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Precision luminosity for Z0 lineshape measurements with a silicon-tungsten calorimeter

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Precision luminosity for Z0 lineshape measurements with a silicon-tungsten calorimeter. / OPAL Collaboration.
In: European Physical Journal C: Particles and Fields, Vol. 14, No. 3, 06.2000, p. 373-425.

Research output: Contribution to Journal/MagazineJournal articlepeer-review

Harvard

OPAL Collaboration 2000, 'Precision luminosity for Z0 lineshape measurements with a silicon-tungsten calorimeter', European Physical Journal C: Particles and Fields, vol. 14, no. 3, pp. 373-425. https://doi.org/10.1007/s100520000353

APA

OPAL Collaboration (2000). Precision luminosity for Z0 lineshape measurements with a silicon-tungsten calorimeter. European Physical Journal C: Particles and Fields, 14(3), 373-425. https://doi.org/10.1007/s100520000353

Vancouver

OPAL Collaboration. Precision luminosity for Z0 lineshape measurements with a silicon-tungsten calorimeter. European Physical Journal C: Particles and Fields. 2000 Jun;14(3):373-425. doi: 10.1007/s100520000353

Author

OPAL Collaboration. / Precision luminosity for Z0 lineshape measurements with a silicon-tungsten calorimeter. In: European Physical Journal C: Particles and Fields. 2000 ; Vol. 14, No. 3. pp. 373-425.

Bibtex

@article{e690038bac26490a9e18ddae0398b08e,
title = "Precision luminosity for Z0 lineshape measurements with a silicon-tungsten calorimeter",
abstract = "The measurement of small–angle Bhabha scattering is used to determine the luminosity at the OPAL interaction point for the LEP I data recorded between 1993 and 1995. The measurement is based on the OPAL Silicon-Tungsten Luminometer which is composed of two calorimeters encircling the LEP beam pipe, on opposite sides of the interaction point. The luminometer detects electrons from small–angle Bhabha scattering at angles between 25 and 58 mrad. At LEP center-of-mass energies around the Z0, about half of all Bhabha electrons entering the detector fall within a 79 nb fiducial acceptance region. The electromagnetic showers generated in the stack of 1 radiation length tungsten absorber plates are sampled by 608 silicon detectors with 38,912 radial pads of 2.5 mm width. The fine segmentation of the detector, combined with the precise knowledge of its physical dimensions, allows the trajectories of incoming 45 GeV electrons or photons to be determined with a total systematic error of less than 7 microns. We have quantified all significant sources of systematic experimental error in the luminosity determination by direct physical measurement. All measured properites of the luminosity event sample are found to be in agreement with current theoretical expectations. The total systematic measurement uncertainty is 3.4×10−4, significantly below the theoretical error of 5.4×10−4 currently assigned to the QED calculation of the Bhabha acceptance, and contributes negligibly to the total uncertainty in the OPAL measurement of Γinv/Γℓ+ℓ−, a quantity of basic physical interest which depends crucially on the luminosity measurement.",
author = "Vakhtang Kartvelishvili and {OPAL Collaboration}",
year = "2000",
month = jun,
doi = "10.1007/s100520000353",
language = "English",
volume = "14",
pages = "373--425",
journal = "European Physical Journal C: Particles and Fields",
issn = "1434-6044",
publisher = "SPRINGER",
number = "3",

}

RIS

TY - JOUR

T1 - Precision luminosity for Z0 lineshape measurements with a silicon-tungsten calorimeter

AU - Kartvelishvili, Vakhtang

AU - OPAL Collaboration

PY - 2000/6

Y1 - 2000/6

N2 - The measurement of small–angle Bhabha scattering is used to determine the luminosity at the OPAL interaction point for the LEP I data recorded between 1993 and 1995. The measurement is based on the OPAL Silicon-Tungsten Luminometer which is composed of two calorimeters encircling the LEP beam pipe, on opposite sides of the interaction point. The luminometer detects electrons from small–angle Bhabha scattering at angles between 25 and 58 mrad. At LEP center-of-mass energies around the Z0, about half of all Bhabha electrons entering the detector fall within a 79 nb fiducial acceptance region. The electromagnetic showers generated in the stack of 1 radiation length tungsten absorber plates are sampled by 608 silicon detectors with 38,912 radial pads of 2.5 mm width. The fine segmentation of the detector, combined with the precise knowledge of its physical dimensions, allows the trajectories of incoming 45 GeV electrons or photons to be determined with a total systematic error of less than 7 microns. We have quantified all significant sources of systematic experimental error in the luminosity determination by direct physical measurement. All measured properites of the luminosity event sample are found to be in agreement with current theoretical expectations. The total systematic measurement uncertainty is 3.4×10−4, significantly below the theoretical error of 5.4×10−4 currently assigned to the QED calculation of the Bhabha acceptance, and contributes negligibly to the total uncertainty in the OPAL measurement of Γinv/Γℓ+ℓ−, a quantity of basic physical interest which depends crucially on the luminosity measurement.

AB - The measurement of small–angle Bhabha scattering is used to determine the luminosity at the OPAL interaction point for the LEP I data recorded between 1993 and 1995. The measurement is based on the OPAL Silicon-Tungsten Luminometer which is composed of two calorimeters encircling the LEP beam pipe, on opposite sides of the interaction point. The luminometer detects electrons from small–angle Bhabha scattering at angles between 25 and 58 mrad. At LEP center-of-mass energies around the Z0, about half of all Bhabha electrons entering the detector fall within a 79 nb fiducial acceptance region. The electromagnetic showers generated in the stack of 1 radiation length tungsten absorber plates are sampled by 608 silicon detectors with 38,912 radial pads of 2.5 mm width. The fine segmentation of the detector, combined with the precise knowledge of its physical dimensions, allows the trajectories of incoming 45 GeV electrons or photons to be determined with a total systematic error of less than 7 microns. We have quantified all significant sources of systematic experimental error in the luminosity determination by direct physical measurement. All measured properites of the luminosity event sample are found to be in agreement with current theoretical expectations. The total systematic measurement uncertainty is 3.4×10−4, significantly below the theoretical error of 5.4×10−4 currently assigned to the QED calculation of the Bhabha acceptance, and contributes negligibly to the total uncertainty in the OPAL measurement of Γinv/Γℓ+ℓ−, a quantity of basic physical interest which depends crucially on the luminosity measurement.

U2 - 10.1007/s100520000353

DO - 10.1007/s100520000353

M3 - Journal article

VL - 14

SP - 373

EP - 425

JO - European Physical Journal C: Particles and Fields

JF - European Physical Journal C: Particles and Fields

SN - 1434-6044

IS - 3

ER -