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Characterization of an MPPC-Based Scintillator Telescope and Measurement of Cosmic Muon Angular Distribution

Sahla Manithottathil, Anuj Gupta, Mudit Kumar, Navaneeth Poonthottathil

Abstract

This report presents the design, characterization, and application of a high-sensitivity optical detection system based on plastic scintillators coupled to Multi-Pixel Photon Counters (MPPCs). The primary objective was to evaluate the performance of MPPCs (Silicon Photomultipliers) as robust, low-voltage alternatives to traditional photomultiplier tubes for detecting faint scintillation light. The optoelectronic properties of the sensors were analyzed, including single-photoelectron gain calibration and dark count rate measurements, to optimize the signal-to-noise ratio. By embedding wavelength-shifting fibers to enhance light collection efficiency, the system was configured into a three-fold coincidence telescope. The angular distribution of the cosmic ray muon flux was measured to validate the detector's stability and geometric acceptance. Fitting the experimental data to a $\bm{\cos^n(θ)}$ distribution yielded an angular exponent of $\bm{n = 1.44 \pm 0.06}$, consistent with literature values. These results demonstrate the efficacy of the MPPC-scintillator coupling for precise photon counting and timing applications in high-energy physics instrumentation.

Characterization of an MPPC-Based Scintillator Telescope and Measurement of Cosmic Muon Angular Distribution

Abstract

This report presents the design, characterization, and application of a high-sensitivity optical detection system based on plastic scintillators coupled to Multi-Pixel Photon Counters (MPPCs). The primary objective was to evaluate the performance of MPPCs (Silicon Photomultipliers) as robust, low-voltage alternatives to traditional photomultiplier tubes for detecting faint scintillation light. The optoelectronic properties of the sensors were analyzed, including single-photoelectron gain calibration and dark count rate measurements, to optimize the signal-to-noise ratio. By embedding wavelength-shifting fibers to enhance light collection efficiency, the system was configured into a three-fold coincidence telescope. The angular distribution of the cosmic ray muon flux was measured to validate the detector's stability and geometric acceptance. Fitting the experimental data to a distribution yielded an angular exponent of , consistent with literature values. These results demonstrate the efficacy of the MPPC-scintillator coupling for precise photon counting and timing applications in high-energy physics instrumentation.
Paper Structure (39 sections, 12 equations, 14 figures, 10 tables)

This paper contains 39 sections, 12 equations, 14 figures, 10 tables.

Figures (14)

  • Figure 1: Schematic representation of a cosmic ray air shower. The primary proton p initiates the cascade. The Muons ($\bm{\mu}$) are highlighted in red as they are the penetrating particles detected in this setup.
  • Figure 2: The complete experimental setup. (a) Laptop station for data acquisition. (b) RIGOL DHO924 oscilloscope. (c) Interface box for bias voltage distribution and signal readout. (d) The three-fold scintillator telescope assembly (containing the scintillators, WLS fibers, and MPPCs). (e) DC power supply. (f) Light-proof black sheet used to cover the detector assembly during operation to ensure complete darkness.
  • Figure 3: Stopping power ($dE/dx$) as a function of muon momentum. The curve shows the characteristic minimum, defining the Minimum Ionizing Particle (MIP) region yau2008cosmic.
  • Figure 4: Photograph of the Hamamatsu MPPC sensors used in the experiment.
  • Figure 5: Conceptual diagram of the three-fold coincidence technique. A valid event is recorded only when a single muon passes through all three detectors simultaneously, generating overlapping electrical pulses. This logic effectively filters out random background noise.
  • ...and 9 more figures