Exploration of optimized front-end readout circuit for time measurement of large-area SiPM arrays

Abstract The detector of TRopIcal DEep-sea Neutrino Telescope (TRIDENT) will use large-area silicon photomultiplier (SiPM) arrays combined with photomultiplier tubes to boost photon detection efficiency and pointing capability. An application-specific integrated circuit (ASIC) is being developed to aim at high-resolution time measurement of large-area SiPM arrays. This work investigates four architectures of readout circuits including different input stages (common gate stage and negative feedback common gate stage) and discriminators (two types of current discriminator and one voltage discriminator) using a 180 nm CMOS process for optimizing time resolution. The experimental measurements show that single photon time resolutions performed using Hamamatsu S13360-3050PE SiPMs are around 260 ps full width at half maximum (FWHM). A timing jitter less than 500 ps FWHM when connecting a 6 × 6 mm 2 SiPM array is achieved. The power consumption is less than 7 mW/channel. Additionally, a digital summation is applied to reduce the number of output interfaces. The measured performances of the ASIC cater to the TRIDENT application requirements.

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Publication Details

Journal
Journal of Instrumentation
Published
2025-08-01
DOI
https://doi.org/10.1088/1748-0221/20/08/t08002
Citations
1
Primary Topic
Astrophysics and Cosmic Phenomena
Type
article
Field-Weighted Citation Impact
1.87
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article

Exploration of optimized front-end readout circuit for time measurement of large-area SiPM arrays

Y. Liu, D. L. Xu, W. Zhi, Junni Tang et al.
1 citations
Journal of Instrumentation
Astrophysics and Cosmic Phenomena
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article

Exploration of optimized front-end readout circuit for time measurement of large-area SiPM arrays

Y. Liu, D. L. Xu, W. Zhi, Junni Tang, M.X. Wang, Yuxin Tan, Weihao Wu, Zizhen Zhou
article en
1 citations

Abstract

Abstract The detector of TRopIcal DEep-sea Neutrino Telescope (TRIDENT) will use large-area silicon photomultiplier (SiPM) arrays combined with photomultiplier tubes to boost photon detection efficiency and pointing capability. An application-specific integrated circuit (ASIC) is being developed to aim at high-resolution time measurement of large-area SiPM arrays. This work investigates four architectures of readout circuits including different input stages (common gate stage and negative feedback common gate stage) and discriminators (two types of current discriminator and one voltage discriminator) using a 180 nm CMOS process for optimizing time resolution. The experimental measurements show that single photon time resolutions performed using Hamamatsu S13360-3050PE SiPMs are around 260 ps full width at half maximum (FWHM). A timing jitter less than 500 ps FWHM when connecting a 6 × 6 mm 2 SiPM array is achieved. The power consumption is less than 7 mW/channel. Additionally, a digital summation is applied to reduce the number of output interfaces. The measured performances of the ASIC cater to the TRIDENT application requirements.

Journal of InstrumentationVol. 20(08)
Shanghai Jiao Tong University (CN), Kavli Institute for Particle Astrophysics and Cosmology (US)
Openalex Percentile: Top 12%
Astrophysics and Cosmic Phenomena
1.87
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