Implementation of Silicon Photomultipliers in Cosmic Ray Detection

ORAL

Abstract

A cosmic ray detector has been constructed which uses the silicon photomultiplier (SiPM) rather than the standard photomultiplier (PMT). Two scintillators have been cut and polished with grooves embedded into them. The design utilizes optical fibers, which are planted into the grooves, to collect light emitted from the scintillator and transmit them to the surface of the SiPM. One goal of this project is to determine the differences in performance of the photomultiplier and the silicon photomultiplier. Once construction is completed, data will be taken which compares the frequency of counts, the output gains, cost of the setup, etc. of the two detectors. The second goal is to create a manual with a detailed description of the construction so that it will be easily replicable to students or professionals, reduce the cost of the construction of the cosmic ray detector, which will make this device more useful to anyone interested in duplicating this design.

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Authors

  • Marcus Wade

    Hartnell College

  • Sergey Savrasov

    Hartnell College, Cal State Univ- Long Beach, University of California, Davis, School of Natural Science, University of California, Merced, Seagate Technology, Materials Science and Engineering, National Tsing Hua University, Taiwan, University of California - Berkeley, University of Colorado, Boulder -- Dept of Physics, University of California, Berkeley -- Dept of Chemistry, UC Merced, California State University, Fresno, California Institute of Technology, California State University, Long Beach, La Canada Flintridge, CA, Department of Physics, Florida A\&M University, Tallahassee, FL-32307, Physical and Life Sciences, Lawrence Livermore National Laboratory, Livermore, CA-94550, Cal State Univ East Bay, American River College, UC Santa Cruz, Notre Dame High School, Benedict College, Lawrence Livermore National Laboratory, Tuskegee University, California State University, Dominguez Hills, Sonoma State University, Carnegie Observatories, University of California, Los Angeles, Institute of Astronomy, University of Cambridge, UK, University of California, Santa Barbara, University of Alabama, MPIfR, Bonn, Germany, Stanford University, University of California - Davis