13–17 Apr 2026
Clarion Hotel Malmö Live
Europe/Stockholm timezone

The Research of Large-Area Scintillator Neutron Detectors at the China Spallation Neutron Source (CSNS)

16 Apr 2026, 11:40
20m
Live 1 (Clarion Hotel Malmö Live)

Live 1

Clarion Hotel Malmö Live

Oral Presentation Technical talks

Speaker

Bin TANG (Institute of High Energy Physics, Chinese Academy of Sciences)

Description

The China Spallation Neutron Source (CSNS) is a multidisciplinary user facility requiring large quantities of position-sensitive neutron detectors for scattering and imaging instruments. To mitigate the global shortage and cost of 3He, CSNS has developed and deployed multiple generations of large-area scintillator neutron detectors.
The first-generation system uses 6LiF/ZnS(Ag) scintillation screens coupled to crossed wavelength-shifting fiber (WLSF) arrays and multi-anode photomultiplier tubes (MA-PMT). This flat-panel detector has been routinely operated at the General Purpose Powder Diffractometer (GPPD) since 2018, providing a typical pixel size of 4×4mm2 and stable performance for diffraction measurements.
To improve efficiency and scalability, a second-generation “louver” detector was developed using oblique 6LiF/ZnS(Ag) scintillator screens with silicon photomultiplier (SiPM) readout. This design has been implemented for the Engineering Materials Diffractometer (EMD) and the Energy-Resolved Neutron Imaging instrument (ERNI), achieving a total active area exceeding 6 m2. The louver geometry increases the effective converter thickness, improving the efficiency from ~38% to ~62% at 1.4 Å, and supports elongated pixels (e.g., 3 mm × 50 mm and 3 mm × 200 mm) tailored to instrument needs.
A third-generation scintillator detector is under development to reach sub-millimeter spatial resolution for single-crystal neutron diffraction. Current R&D focuses on compact optical coupling, optimized photosensor arrays, and scalable readout electronics for future CSNS instruments.

Author

Bin TANG (Institute of High Energy Physics, Chinese Academy of Sciences)

Co-authors

Mrs Hong Xu (Institute of High Energy Physics, Chinese Academy of Sciences) Dr Jiawei Liang (Institute of High Energy Physics, Chinese Academy of Sciences) Mr Shaojia Chen (Institute of High Energy Physics, Chinese Academy of Sciences) Mr Xiuku Wang (Institute of High Energy Physics, Chinese Academy of Sciences) Prof. Zhijia Sun (Institute of High Energy Physics, Chinese Academy of Sciences)

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