Published October 29, 2007
| Version v1
Journal article
X-ray diamond detectors with energy resolution
- 1. General Physics Institute, Russian Academy of Science, Vavilova Str. 38, 119991 Moscow (Russian Federation)
- 2. Department of Electronic Engineering and CNISM, University of Rome 'Roma Tre', Via della Vasca Navale, 84--00146 Rome (Italy)
Description
Polycrystalline diamond detectors with energy resolving capability of the impinging beam were realized and tested by using a miniature pyroelectric x-ray pulse generator. Microstrip structures were defined by photolithography aimed to reduce parasitic capacitances and to perform characterization measurements in a sandwich configuration. Leakage currents as low as 20 pA at 500 V were measured on a 270 μm thick device. Pulse height distributions were carried out around Ta Lα (8.14 keV) and Cu Kα (8.05 keV) characteristic lines of the source. Energy resolution at 200 V was found equal to 9% with an increase to 11% at 500 V. When the bias was increased to the maximum voltage the sample shows an Ohmic behavior
Additional details
Identifiers
- DOI
- 10.1063/1.2805221;
Publishing Information
- Journal Title
- Applied Physics Letters
- Journal Volume
- 91
- Journal Issue
- 18
- Journal Page Range
- p. 183515-183515.3
- ISSN
- 0003-6951
- CODEN
- APPLAB
INIS
- Country of Publication
- United States
- Country of Input or Organization
- International Atomic Energy Agency (IAEA)
- INIS RN
- 39035955
- Subject category
- S46: INSTRUMENTATION RELATED TO NUCLEAR SCIENCE AND TECHNOLOGY;
- Descriptors DEI
- CAPACITANCE; DIAMONDS; ELECTRIC POTENTIAL; ENERGY RESOLUTION; KEV RANGE 01-10; LEAKAGE CURRENT; POLYCRYSTALS; PULSE GENERATORS; X RADIATION; X-RAY DETECTION
- Descriptors DEC
- CARBON; CRYSTALS; CURRENTS; DETECTION; ELECTRIC CURRENTS; ELECTRICAL PROPERTIES; ELECTROMAGNETIC RADIATION; ELECTRONIC EQUIPMENT; ELEMENTS; ENERGY RANGE; EQUIPMENT; FUNCTION GENERATORS; IONIZING RADIATIONS; KEV RANGE; MINERALS; NONMETALS; PHYSICAL PROPERTIES; RADIATION DETECTION; RADIATIONS; RESOLUTION
Optional Information
- Notes
- (c) 2007 American Institute of Physics