<p>All-inorganic CsPbCl<InlineEquation ID="IEq3"> <EquationSource Format="TEX">\(_3\)</EquationSource> <EquationSource Format="MATHML"><math> <mmultiscripts> <mrow /> <mn>3</mn> <mrow /> </mmultiscripts> </math></EquationSource> </InlineEquation> perovskite is a promising material for high-performance radiation detection owing to its extraordinary photoelectric properties and chemical stability. The critical challenge in developing wide-bandgap CsPbCl<InlineEquation ID="IEq4"> <EquationSource Format="TEX">\(_3\)</EquationSource> <EquationSource Format="MATHML"><math> <mmultiscripts> <mrow /> <mn>3</mn> <mrow /> </mmultiscripts> </math></EquationSource> </InlineEquation> perovskite lies in the quantitative assessment of its charge transport properties, which regulate its performance optimization. Herein, we report the first spectroscopic <InlineEquation ID="IEq5"> <EquationSource Format="TEX">\(\upalpha\)</EquationSource> <EquationSource Format="MATHML"><math> <mi mathvariant="normal">α</mi> </math></EquationSource> </InlineEquation> particles using CsPbCl<InlineEquation ID="IEq6"> <EquationSource Format="TEX">\(_3\)</EquationSource> <EquationSource Format="MATHML"><math> <mmultiscripts> <mrow /> <mn>3</mn> <mrow /> </mmultiscripts> </math></EquationSource> </InlineEquation> detectors with asymmetric contact. CsPbCl<InlineEquation ID="IEq7"> <EquationSource Format="TEX">\(_3\)</EquationSource> <EquationSource Format="MATHML"><math> <mmultiscripts> <mrow /> <mn>3</mn> <mrow /> </mmultiscripts> </math></EquationSource> </InlineEquation> single crystals (<InlineEquation ID="IEq8"> <EquationSource Format="TEX">\(\upphi\)</EquationSource> <EquationSource Format="MATHML"><math> <mi mathvariant="normal">ϕ</mi> </math></EquationSource> </InlineEquation> 15&#xa0;mm&#xa0;<InlineEquation ID="IEq9"> <EquationSource Format="TEX">\(\times\)</EquationSource> <EquationSource Format="MATHML"><math> <mo>×</mo> </math></EquationSource> </InlineEquation> 50&#xa0;mm) were successfully grown using the Bridgman melt method and subsequently fabricated into Schottky-type Bi/CsPbCl<InlineEquation ID="IEq10"> <EquationSource Format="TEX">\(_3\)</EquationSource> <EquationSource Format="MATHML"><math> <mmultiscripts> <mrow /> <mn>3</mn> <mrow /> </mmultiscripts> </math></EquationSource> </InlineEquation>/Au detectors. Owing to its high electrical resistivity of 1.25 <InlineEquation ID="IEq11"> <EquationSource Format="TEX">\(\times\)</EquationSource> <EquationSource Format="MATHML"><math> <mo>×</mo> </math></EquationSource> </InlineEquation> 10<InlineEquation ID="IEq12"> <EquationSource Format="TEX">\(^9\)</EquationSource> <EquationSource Format="MATHML"><math> <mmultiscripts> <mrow /> <mrow /> <mn>9</mn> </mmultiscripts> </math></EquationSource> </InlineEquation> <InlineEquation ID="IEq13"> <EquationSource Format="TEX">\(\Omega\)</EquationSource> <EquationSource Format="MATHML"><math> <mi mathvariant="normal">Ω</mi> </math></EquationSource> </InlineEquation> <InlineEquation ID="IEq14"> <EquationSource Format="TEX">\(\cdot\)</EquationSource> <EquationSource Format="MATHML"><math> <mo>·</mo> </math></EquationSource> </InlineEquation> cm, the CsPbCl<InlineEquation ID="IEq15"> <EquationSource Format="TEX">\(_3\)</EquationSource> <EquationSource Format="MATHML"><math> <mmultiscripts> <mrow /> <mn>3</mn> <mrow /> </mmultiscripts> </math></EquationSource> </InlineEquation> detector demonstrated a low dark current density (<InlineEquation ID="IEq16"> <EquationSource Format="TEX">\(\sim\)</EquationSource> <EquationSource Format="MATHML"><math> <mo>∼</mo> </math></EquationSource> </InlineEquation>870 nA/cm<InlineEquation ID="IEq17"> <EquationSource Format="TEX">\(^2\)</EquationSource> <EquationSource Format="MATHML"><math> <mmultiscripts> <mrow /> <mrow /> <mn>2</mn> </mmultiscripts> </math></EquationSource> </InlineEquation>) and stable performance. The CsPbCl<InlineEquation ID="IEq18"> <EquationSource Format="TEX">\(_3\)</EquationSource> <EquationSource Format="MATHML"><math> <mmultiscripts> <mrow /> <mn>3</mn> <mrow /> </mmultiscripts> </math></EquationSource> </InlineEquation> detector was also capable of resolving both the <InlineEquation ID="IEq19"> <EquationSource Format="TEX">\(\upalpha\)</EquationSource> <EquationSource Format="MATHML"><math> <mi mathvariant="normal">α</mi> </math></EquationSource> </InlineEquation> particle (5.5 MeV) and <InlineEquation ID="IEq20"> <EquationSource Format="TEX">\(\upgamma\)</EquationSource> <EquationSource Format="MATHML"><math> <mi mathvariant="normal">γ</mi> </math></EquationSource> </InlineEquation>-ray (59.5 keV) peaks from the <InlineEquation ID="IEq21"> <EquationSource Format="TEX">\(^{241}\)</EquationSource> <EquationSource Format="MATHML"><math> <mmultiscripts> <mrow /> <mrow /> <mn>241</mn> </mmultiscripts> </math></EquationSource> </InlineEquation>Am radioactive isotope. Furthermore, the carrier transport properties of CsPbCl<InlineEquation ID="IEq22"> <EquationSource Format="TEX">\(_3\)</EquationSource> <EquationSource Format="MATHML"><math> <mmultiscripts> <mrow /> <mn>3</mn> <mrow /> </mmultiscripts> </math></EquationSource> </InlineEquation> were evaluated quantitatively by the time-of-flight technology using <InlineEquation ID="IEq23"> <EquationSource Format="TEX">\(^{241}\)</EquationSource> <EquationSource Format="MATHML"><math> <mmultiscripts> <mrow /> <mrow /> <mn>241</mn> </mmultiscripts> </math></EquationSource> </InlineEquation>Am <InlineEquation ID="IEq24"> <EquationSource Format="TEX">\(\upalpha\)</EquationSource> <EquationSource Format="MATHML"><math> <mi mathvariant="normal">α</mi> </math></EquationSource> </InlineEquation> particle response, revealing the hole and electron mobilities as <InlineEquation ID="IEq25"> <EquationSource Format="TEX">\(\sim\)</EquationSource> <EquationSource Format="MATHML"><math> <mo>∼</mo> </math></EquationSource> </InlineEquation>11.12 and <InlineEquation ID="IEq26"> <EquationSource Format="TEX">\(\sim\)</EquationSource> <EquationSource Format="MATHML"><math> <mo>∼</mo> </math></EquationSource> </InlineEquation>12.92 cm<InlineEquation ID="IEq27"> <EquationSource Format="TEX">\(^2\)</EquationSource> <EquationSource Format="MATHML"><math> <mmultiscripts> <mrow /> <mrow /> <mn>2</mn> </mmultiscripts> </math></EquationSource> </InlineEquation> <InlineEquation ID="IEq28"> <EquationSource Format="TEX">\(\cdot\)</EquationSource> <EquationSource Format="MATHML"><math> <mo>·</mo> </math></EquationSource> </InlineEquation>V<InlineEquation ID="IEq29"> <EquationSource Format="TEX">\(^{-1}\)</EquationSource> <EquationSource Format="MATHML"><math> <mmultiscripts> <mrow /> <mrow /> <mrow> <mo>-</mo> <mn>1</mn> </mrow> </mmultiscripts> </math></EquationSource> </InlineEquation> <InlineEquation ID="IEq30"> <EquationSource Format="TEX">\(\cdot\)</EquationSource> <EquationSource Format="MATHML"><math> <mo>·</mo> </math></EquationSource> </InlineEquation>s<InlineEquation ID="IEq31"> <EquationSource Format="TEX">\(^{-1}\)</EquationSource> <EquationSource Format="MATHML"><math> <mmultiscripts> <mrow /> <mrow /> <mrow> <mo>-</mo> <mn>1</mn> </mrow> </mmultiscripts> </math></EquationSource> </InlineEquation>, respectively. Meanwhile, the hole and electron mobility–lifetime products were obtained as <InlineEquation ID="IEq32"> <EquationSource Format="TEX">\(\sim\)</EquationSource> <EquationSource Format="MATHML"><math> <mo>∼</mo> </math></EquationSource> </InlineEquation>1.72 <InlineEquation ID="IEq33"> <EquationSource Format="TEX">\(\times\)</EquationSource> <EquationSource Format="MATHML"><math> <mo>×</mo> </math></EquationSource> </InlineEquation> 10<InlineEquation ID="IEq34"> <EquationSource Format="TEX">\(^{-4}\)</EquationSource> <EquationSource Format="MATHML"><math> <mmultiscripts> <mrow /> <mrow /> <mrow> <mo>-</mo> <mn>4</mn> </mrow> </mmultiscripts> </math></EquationSource> </InlineEquation> and <InlineEquation ID="IEq35"> <EquationSource Format="TEX">\(\sim\)</EquationSource> <EquationSource Format="MATHML"><math> <mo>∼</mo> </math></EquationSource> </InlineEquation>1.04 <InlineEquation ID="IEq36"> <EquationSource Format="TEX">\(\times\)</EquationSource> <EquationSource Format="MATHML"><math> <mo>×</mo> </math></EquationSource> </InlineEquation> 10<InlineEquation ID="IEq37"> <EquationSource Format="TEX">\(^{-4}\)</EquationSource> <EquationSource Format="MATHML"><math> <mmultiscripts> <mrow /> <mrow /> <mrow> <mo>-</mo> <mn>4</mn> </mrow> </mmultiscripts> </math></EquationSource> </InlineEquation> cm<InlineEquation ID="IEq38"> <EquationSource Format="TEX">\(^2\)</EquationSource> <EquationSource Format="MATHML"><math> <mmultiscripts> <mrow /> <mrow /> <mn>2</mn> </mmultiscripts> </math></EquationSource> </InlineEquation> <InlineEquation ID="IEq39"> <EquationSource Format="TEX">\(\cdot\)</EquationSource> <EquationSource Format="MATHML"><math> <mo>·</mo> </math></EquationSource> </InlineEquation>V<InlineEquation ID="IEq40"> <EquationSource Format="TEX">\(^{-1}\)</EquationSource> <EquationSource Format="MATHML"><math> <mmultiscripts> <mrow /> <mrow /> <mrow> <mo>-</mo> <mn>1</mn> </mrow> </mmultiscripts> </math></EquationSource> </InlineEquation>, respectively. The planar CsPbCl<InlineEquation ID="IEq41"> <EquationSource Format="TEX">\(_3\)</EquationSource> <EquationSource Format="MATHML"><math> <mmultiscripts> <mrow /> <mn>3</mn> <mrow /> </mmultiscripts> </math></EquationSource> </InlineEquation> detector achieved an excellent energy resolution of <InlineEquation ID="IEq42"> <EquationSource Format="TEX">\(\sim\)</EquationSource> <EquationSource Format="MATHML"><math> <mo>∼</mo> </math></EquationSource> </InlineEquation>14.9% at 122 keV under <InlineEquation ID="IEq43"> <EquationSource Format="TEX">\(\upgamma\)</EquationSource> <EquationSource Format="MATHML"><math> <mi mathvariant="normal">γ</mi> </math></EquationSource> </InlineEquation>-ray exposure, which is the highest energy resolution reported to date for CsPbCl<InlineEquation ID="IEq44"> <EquationSource Format="TEX">\(_3\)</EquationSource> <EquationSource Format="MATHML"><math> <mmultiscripts> <mrow /> <mn>3</mn> <mrow /> </mmultiscripts> </math></EquationSource> </InlineEquation> detectors. This study highlights the considerable potential of inorganic perovskite detectors for radiation detection and provides a practical approach for the future development of perovskite materials.</p>

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Assessment of carrier transport properties of perovskite CsPbCl\(_3\) single crystal with time-of-flight alpha-particle response

  • Qi-Hao Sun,
  • Zhou Wu,
  • Shu-Quan Wei,
  • Yu-Quan Wang,
  • Xu-Chang He,
  • Bao Xiao,
  • Nan-Nan Shen,
  • Jian-Fu Zhang,
  • Yi-Hui He

摘要

All-inorganic CsPbCl \(_3\) 3 perovskite is a promising material for high-performance radiation detection owing to its extraordinary photoelectric properties and chemical stability. The critical challenge in developing wide-bandgap CsPbCl \(_3\) 3 perovskite lies in the quantitative assessment of its charge transport properties, which regulate its performance optimization. Herein, we report the first spectroscopic \(\upalpha\) α particles using CsPbCl \(_3\) 3 detectors with asymmetric contact. CsPbCl \(_3\) 3 single crystals ( \(\upphi\) ϕ 15 mm  \(\times\) × 50 mm) were successfully grown using the Bridgman melt method and subsequently fabricated into Schottky-type Bi/CsPbCl \(_3\) 3 /Au detectors. Owing to its high electrical resistivity of 1.25 \(\times\) × 10 \(^9\) 9 \(\Omega\) Ω \(\cdot\) · cm, the CsPbCl \(_3\) 3 detector demonstrated a low dark current density ( \(\sim\) 870 nA/cm \(^2\) 2 ) and stable performance. The CsPbCl \(_3\) 3 detector was also capable of resolving both the \(\upalpha\) α particle (5.5 MeV) and \(\upgamma\) γ -ray (59.5 keV) peaks from the \(^{241}\) 241 Am radioactive isotope. Furthermore, the carrier transport properties of CsPbCl \(_3\) 3 were evaluated quantitatively by the time-of-flight technology using \(^{241}\) 241 Am \(\upalpha\) α particle response, revealing the hole and electron mobilities as \(\sim\) 11.12 and \(\sim\) 12.92 cm \(^2\) 2 \(\cdot\) · V \(^{-1}\) - 1 \(\cdot\) · s \(^{-1}\) - 1 , respectively. Meanwhile, the hole and electron mobility–lifetime products were obtained as \(\sim\) 1.72 \(\times\) × 10 \(^{-4}\) - 4 and \(\sim\) 1.04 \(\times\) × 10 \(^{-4}\) - 4 cm \(^2\) 2 \(\cdot\) · V \(^{-1}\) - 1 , respectively. The planar CsPbCl \(_3\) 3 detector achieved an excellent energy resolution of \(\sim\) 14.9% at 122 keV under \(\upgamma\) γ -ray exposure, which is the highest energy resolution reported to date for CsPbCl \(_3\) 3 detectors. This study highlights the considerable potential of inorganic perovskite detectors for radiation detection and provides a practical approach for the future development of perovskite materials.