Optical calibration systems of the Pacific Ocean Neutrino Experiment
M. Agostini, A. Alexander Wight, M. Altomare, K. Ba\c{s}, N. Baily, P. S. Barbeau, A. J. Baron, S. Bash, C. Bellenghi, M. Boehmer, M. Brandenburg, P. Bunton, N. Cedarblade-Jones, B. Crudele, M. Danninger, T. DeYoung, A. G\"artner, J. Garriz, D. Ghuman, L. Ginzkey, T. Glukler

TL;DR
This paper details the design, development, and performance testing of novel optical calibration systems for the Pacific Ocean Neutrino Experiment, including innovative light-pulse drivers and isotropic calibration modules, validated through simulations and experiments.
Contribution
It introduces new gallium nitride-based light-pulse driver circuitry and optimized isotropic calibration modules for neutrino detection calibration.
Findings
Achieved emission intensities up to 10^11 photons
Pulse widths as small as 1.4 ns
Simulated isotropy grade of 1.00 ± 0.01
Abstract
This work presents the design and performance characterization of the optical calibration systems produced for the Pacific Ocean Neutrino Experiment (P-ONE). These include novel light-pulse driver circuitry based on gallium nitride field-effect transistor technology and its application to directional and isotropic, self-monitoring optical calibration instruments. A total of 330 directional light pulsers and two isotropic, 17-inch calibration modules (P-CALs) were produced for the first P-ONE line. We present the designs and performance of both the directional and isotropic calibration devices and perform detailed optical characterizations of both full-production batches. In a wavelength range of nm, our developed driver circuits achieve emission intensities up to photons and pulse widths as small as ns, respectively. Light-pulse drivers and self-monitoring…
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Taxonomy
TopicsNeutrino Physics Research · Astrophysics and Cosmic Phenomena · Radiation Detection and Scintillator Technologies
