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Title: Scintillator Replacement Option for BaBar

Abstract

A replacement technology for the muon detection system in BaBar using scintillator bars with Wavelength Shifting (WLS) fibers and Avalanche Photo Diodes (APDs). APDs must be used in BaBar due to the high magnetic fields that disrupt the electron multiplying effects of Photo Multiplier Tubes (PMTs). Muons passing through scintillator cause fluors in the scintillator to emit photons, which are captured by WLS fibers and then re-emitted at the ends of the fibers to awaiting APDs. The detector configuration that will produce the largest Light Yield (LY) and produce a clear APD signal that will be larger than background noise is the main goal of the study. Bar dimensions, number of WLS fibers, and placement of fibers are parameters that may be adjusted to produce the largest LY. Additionally, good timing resolution is needed to determine where a muon passed through the detector along the long direction of the bar. A scintillator bar 2cm x 4cm in x-y with four round lmm fibers produced the largest LY out of four different configurations with a timing resolution of 25cm. A Monte Carlo simulation confirmed the relative LY compared to other detectors. This detector was able to produce a 40mV pulse frommore » the APD that was easily discernable above the 2-SmV background noise. Refinement of the fabrication process could produced higher LYs and better timing resolutions, while a redesign of the electronics may increase the signal to noise ratio.« less

Authors:
Publication Date:
Research Org.:
SLAC National Accelerator Lab., Menlo Park, CA (United States)
Sponsoring Org.:
USDOE Office of Science (US)
OSTI Identifier:
826728
Report Number(s):
SLAC-PUB-9398
TRN: US0404143
DOE Contract Number:  
AC03-76SF00515
Resource Type:
Technical Report
Resource Relation:
Other Information: PBD: 5 Feb 2004
Country of Publication:
United States
Language:
English
Subject:
72 PHYSICS OF ELEMENTARY PARTICLES AND FIELDS; BACKGROUND NOISE; CONFIGURATION; DIMENSIONS; ELECTRON MULTIPLIERS; ELECTRONS; FIBERS; MAGNETIC FIELDS; MUON DETECTION; MUONS; PHOSPHORS; PHOTONS; RESOLUTION; SIGNAL-TO-NOISE RATIO; WAVELENGTHS

Citation Formats

Lometti, m. Scintillator Replacement Option for BaBar. United States: N. p., 2004. Web. doi:10.2172/826728.
Lometti, m. Scintillator Replacement Option for BaBar. United States. https://doi.org/10.2172/826728
Lometti, m. 2004. "Scintillator Replacement Option for BaBar". United States. https://doi.org/10.2172/826728. https://www.osti.gov/servlets/purl/826728.
@article{osti_826728,
title = {Scintillator Replacement Option for BaBar},
author = {Lometti, m},
abstractNote = {A replacement technology for the muon detection system in BaBar using scintillator bars with Wavelength Shifting (WLS) fibers and Avalanche Photo Diodes (APDs). APDs must be used in BaBar due to the high magnetic fields that disrupt the electron multiplying effects of Photo Multiplier Tubes (PMTs). Muons passing through scintillator cause fluors in the scintillator to emit photons, which are captured by WLS fibers and then re-emitted at the ends of the fibers to awaiting APDs. The detector configuration that will produce the largest Light Yield (LY) and produce a clear APD signal that will be larger than background noise is the main goal of the study. Bar dimensions, number of WLS fibers, and placement of fibers are parameters that may be adjusted to produce the largest LY. Additionally, good timing resolution is needed to determine where a muon passed through the detector along the long direction of the bar. A scintillator bar 2cm x 4cm in x-y with four round lmm fibers produced the largest LY out of four different configurations with a timing resolution of 25cm. A Monte Carlo simulation confirmed the relative LY compared to other detectors. This detector was able to produce a 40mV pulse from the APD that was easily discernable above the 2-SmV background noise. Refinement of the fabrication process could produced higher LYs and better timing resolutions, while a redesign of the electronics may increase the signal to noise ratio.},
doi = {10.2172/826728},
url = {https://www.osti.gov/biblio/826728}, journal = {},
number = ,
volume = ,
place = {United States},
year = {Thu Feb 05 00:00:00 EST 2004},
month = {Thu Feb 05 00:00:00 EST 2004}
}