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A Wide Energy Band Compound Pixelated Photon Detector

A Wide Energy Band Compound Pixelated Photon Detector
Upendra Desai, Larry Orwig Code 682, NASA/GSFC We present a new concept of a stacked detector that provides high spectral resolution over a wide energy band (keV-MeV). The concept is to use detectors of appropriate energy bandwidth to avoid saturation effects of single detectors normally used. It also provides identification whether the interaction is photoelectric or compton interaction. Multiple comptons can also be identified. It enables rejection of energetic particle tracks. For the energy range from sub keV to 20 keV we use silicon PIN detectors. To cover energies from 20 keV to 60 keV we use a 2-mm-thick CZT detector beneath the "Si" PIN detector. To extend the energy range above 60 keV we incorporated another 5-mm-thick CZT. To achieve the response to MeV photons we incorporate a 2-cm-thick scintillator viewed by a PIN photo diode as the last element of the stack. The significant advantages of this concept over a single detector would be (1) charged particle rejection capability, (2) low internal noise, and (3) identification of Compton interactions. Over the last couple of years, a significant improvement in energy resolution of solid-state detectors for soft and hard x-rays has been achieved. Even at room temperature, one can achieve less than one keV resolution in commercially available silicon diodes for soft x-rays up to 15 - 20 keV. With a thermoelectric cooling, one can achieve resolution of 150 eV for silicon detectors for soft x-rays. High 'Z' solid state detectors like Cadmium Zinc Teluride (CZT) are also available commercially, providing less than 2 keV resolution at 122 keV. This is made possible primarily because of very low leakage currents of the detectors with high resistivity improved materials, and low capacitance because of their small sizes. These detectors are presently available in sizes less than one cm2 area. The size and the thickness of these detectors are major limitations for their use in wide band energy measurements. We have evaluated silicon diode detectors with 1 cm2 area and thickness from 300 јm to 2 mm. In 1996, we evaluated a stacked configuration of silicon detectors to increase detector efficiency at higher energies as well as to reduce the charged particle contribution. The stacked configuration also provides the capability to reduce pile up problems encountered in a single wide energy hand detector. When the spectrum to be observed is steep (power law index of -3 to -5), saturation of the detector is a very serious problem in the deconvolution of the data. Measurements made in narrow energy bands by individual members of the stack avoid this problem. The stacking enables one to identify whether there was a photoelectric interaction, as revealed by a response in only one element of the stack or a Compton scattering as recorded by signals in multiple elements of the stack. We propose now to use different detector elements in a stacked configuration to enhance the total energy bandwidth. We propose to have silicon elements for low energy photons - below which we propose to use CZT elements to cover energies up to 100 keV. To achieve high detection efficiencies up to a few tens of MeV, we propose to have a CSI scintillator viewed by an avalanche photo-diode (APD). We have evaluated all the individual elements - Silicon PINs (thin & thick), CZT (2 mm -5mm thickness), and CSI (4 cm x 1 cm x 1 cm). The single pixel area would then be 1 cm x 1 cm covering the energy range from a keV to 10 MeV. The resolution in the 1 - 15 keV band will be sub keV in the silicon detectors. CZT will offer high detection efficiencies up to 200 - 300 keV with an energy resolution of a few keV. The last element, a CSI scintillator viewed by a avalanche photo-diode (APD) provides high detection efficiency for photons with energy up to 10 MeV. The energy resolution at 660 keV is around 10%.

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A Wide Energy Band Compound Pixelated Photon Detector

file:///C|/Nadia/space_detectors/photon detector poster.htm (2 of 2) [8/21/2001 5:56:45 PM]