Abstract

In this chapter, the fundamental principles of high-energy radiation detection and recent progress in the emerging field of metal halide perovskite (MHP)-based direct and indirect X-ray and γ-ray detectors are discussed. The chapter first introduces the underlying principles of high-energy radiation detection, with emphasis on the key performance metrics. This is followed by a comprehensive summary of the recent progress made in the field of perovskite-based radiation detector technologies. Finally, the chapter ends with an overview of current issues and future perspectives on MHP-based direct and indirect (scintillators) radiation detector technologies.

Highlights

  • Key to this is the ability of Metal halide perovskites (MHPs) to accommodate heavy elements while being able to form large, high-quality crystals and polycrystalline layers, making them one of the most promising emerging X-ray and γ-ray detector the cuboctahedral cavity formed by nearestneighbor X atoms in an AX12 polyhedron.[5]

  • We aim to provide the reader first with an introduction to the basic principles of high-energy radiation detection, and second, with a critical review of the progress achieved to date in the rapidly advancing area of X-ray and γ-ray detectors based on MHPs

  • The resulting crystals were of high quality as verified by X-ray diffraction (XRD) measurements, while capacitance–frequency (C–f) measurements highlighted the presence of a low trap density of 1.4 × 1010 cm−3, which is comparable to 3D MHPs (1010–1013 cm−3)[108] and significantly lower than commercial inorganic materials (1015–1016 cm−3).[108,109]

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Summary

High-Energy Radiation Detectors

There are two primary types of high-energy radiation detectors and are classified depending on the detection principle: I) direct detectors, and II) indirect detectors.[52]. Direct detectors rely on photoconductive materials that are sensitive to particular high energy radiation. Indirect detectors employ scintillator materials that convert, in energy, the absorbed high energy X-rays (0.1–100 keV) or γ-rays (0.1–10 MeV) (Figure 2) to ultraviolet light (UV) or visible (vis), which is subsequently detected by standard photodiode/array.[53–55]. We aim to provide the reader first with an introduction to the basic principles of high-energy radiation detection, and second, with a critical review of the progress achieved to date in the rapidly advancing area of X-ray and γ-ray detectors based on MHPs. Technologies covered include direct and indirect high-energy photon detectors, with emphasis on the

Direct X-Ray Detection
Indirect X-Ray Detection
Gamma-Ray (γ) Detectors
Metal Halide Perovskites for High-Energy Radiation Detection
Direct X-Ray Detectors
Low-Dimensional Perovskites
Large-Area Perovskite-Based Direct X-Ray Detectors
Indirect Metal Halide Perovskite X-Ray Detectors
Direct Gamma-Ray Detectors
Indirect Gamma-Ray Detectors
Summary and Future Perspective
Findings
Conflict of Interest
Full Text
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