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" Sampling the Universe above 10 keV"

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Presentation on theme: "" Sampling the Universe above 10 keV""— Presentation transcript:

1 " Sampling the Universe above 10 keV"
The Extreme Sky " Sampling the Universe above 10 keV"   October 2009 Otranto Recent Trends in the Development of CdTe and CdZnTe Semiconductor Detectors for Astrophysical Applications S. Del Sordo1, L. Abbene1,2, N. Auricchio 1 ,E. Caroli1, M. Quadrini1, J.B. Stephen1 , A. Zappettini3, R.M. Curado Da Silva4, O. Limousin5, A. Meuris5 and P. Ubertini1 1IASF-INAF, Italy 2DiFTeR Università di Palermo, Palermo, Italy 3IMEM-CNR, Parma, Italy 4Departmento de Física, Universidade de Coimbra, Coimbra, Portugal 5CEA – DSM - Irfu - Service d’Astrophysique, Saclay, France

2 Outline Scenario (projects and collaborations)
CdTe / CdZnTe X-ray and gamma ray detectors Detector prototypes Work in progress and future developments Conclusions

3 The Italian collaboration
Projects and Collaborations Progetto ASI Alte Energie (Study for the Gamma Ray Imager mission) Progetto PRIN INAF SGRIP (funded by INAF) Development of an high efficiency wide band 3D CZT detector prototype for Laue telescope focal plane Progetto PRIN (funded by MIUR) Growth technologies and spectroscopic optimization for X and Gamma ray detectors based on CdTe/CdZnTe. International collaborations The Italian collaboration ESRF Grenoble Leicester University DTU Space Copenaghen Coimbra University CEA Saclay Paris ICE-CSIC Barcelona IASF-INAF (Milano Bologna Roma Palermo) IMEM-CNR di Parma (crystal growth) Università di Lecce (crystal growth and bonding) IMM-CNR di Lecce (bonding and electrical characterization) DIFTER Università di Palermo (medical applications) 3

4 CdTe and CdZnTe I High Z semiconductors (Zmax = 52)
Wide band gap semiconductors Del Sordo S. et al., Sensors, Vol. 9, , 2009.

5 CdTe and CdZnTe II Critical Issues
Poor transport properties of the charge carriers: hh ~ cm2/ V ee ~ cm2/V) Small electrical signals at the electrodes Small crystal size: typically < 2 cm3 Development of single charge carrier sensing detectors (pixel, strip, Frisch grid, multiple electrodes) to overcome the poor transport properties of the holes is mandatory. 1 mm L. Abbene et al., NIM A 583 (2007)

6 A. Zappettini et al., IEEE Nucl. Sci. Symp. Conf. Rec. 2008, 118-121.
CdTe and CdZnTe III Suppliers of Spectrometer grade crystals Italian group at IMEM-CNR (A. Zappettini): CdZnTe crystals grown by the boron oxide encapsulated vertical Bridgman technique 1.1 mm A. Zappettini et al., IEEE Nucl. Sci. Symp. Conf. Rec. 2008, 2-inch CdZnTe crystal

7 DETECTORS CHARACTERISTICS
CdZnTe detector prototypes CZT pixel detectors DETECTORS CHARACTERISTICS Pixel detectors CZT (eV Products) Geometric surface 10×10 mm2 Active area 8×8 mm2 Thickness 1 mm and 2 mm Number of pixels 256 Pitch 0.5 mm (0.45 mm anodes, 0.05 mm gap) focal plane detector prototypes for Hard X-ray multilayer telescopes ( keV)

8 CZT pixel detectors performance
CdZnTe detector prototypes CZT pixel detectors performance Energy (keV) Energy resolution (%) Peak to valley ratio (2 x FWHM) 59.5 5.80 ± 0.16 28.1 ± 1.1 88,1 3.9 ± 0.2 19.5 ± 1.1 L. Abbene et al., JAP, Vol. 105, 2009.

9 CdZnTe detector prototypes
CZT pixel detectors performance 2 mm thick detector vs 1 mm thickness 1 mm 2 mm energy resolution (%) (59.5 keV) 5.80 ± 0.16 5.50 ± 0.10 energy resolution (%) (88.1 keV) 3.9 ± 0.2 3.50 ± 0.13 deviation of the FW.1M/FWHM ratio from the Gaussian ratio (1.82) (59.5 keV) 8 % 5 % deviation of the FW.1M/FWHM ratio from the Gaussian ratio (1.82) (88.1 keV) 16 % 10 % “Small pixel effect” H. Barrett, J. Eskin, H. Barber, Phys. Rev. Lett. 75 (1995) 156

10 CdZnTe detector prototypes
CZT pixel detector for the POLCA II Experiment (POLarimetry with CdZnTe Arrays) Detector CZT Imarad 4x4 cm2, 5 mm thick HV = -600 V 16x16 pix with 2.5 mm pitch 11x pix used Readout Electronics 8 eV products ASIC 16 channels/chip 33/50/100/200 sel. Gain 0.6/1.2/2.4/4 μs shaping time The POLCA quick look S/W user interface (LABVIEW)

11 Counts maps (scattered events)
CdZnTe detector prototypes Polca experiment: Set-up at ESRF beam line ID15B and Results Counts maps (scattered events) pixel 186, Energy 200 keV, Angle 0, 45 degree

12 CdZnTe detector prototypes
Small 3D CZT position sensitive spectrometer (SmallGRIPrototype) 3D detector prototype packaging scheme: The detector assembly is built with 8 identical modules packed together (64 anodes and 32 cathodes). I/O pads Alumina support Basic sensitive CZT unit ▶External Dimensions: 10×10×2.5 mm3 Anode side: 8 anodes strips 0.15 mm wide (pitch=2.5 mm) correcting field strips 0.15 mm wide gap between strips=0.15 mm Cathode side: 4 cathodes strips 2.4 mm wide gap between strips=0.10 mm Front end electronics board Redout Electronics NOVARAD Rena3 data handling and logic board See Poster E. Caroli et al. SGRIP …

13 CdTe Schottky detector
Future Developments The POLCaliste experiment CdTe Schottky detector Caliste Module Low noise readout electronics r.m.s. 80 e-

14 Energy resolution 1.5 % (FWHM) @ 59.5 keV
Future Developments The POLCaliste experiment POLCaliste Experiment (POLarimetry with Caliste) Caliste module performance Energy resolution 1.5 % 59.5 keV T = -15 °C Polarimetric measurements at ESRF with the PolCaliste prototype are foreseen in We foresee to use in a first run the 64 ch device and in a next step the new 256 ch device. The device thickness will be 0.5, 1, 2 mm

15 Conclusions (I) Italian CZT detector development (crystal growth and detectors assembly) activities are in progress with quite good expectations. Experimental activities devoted to characterize imaging spectrometer operative in the keV energy band are in progress. The SGRIP experiment (considered as a pathfinder for GRI) is in an advanced realization phase. The study of the prototype performances, foreseen in the 2010, will allow the optimization of the main operative parameters for a detector operative up to 800 keV in stack configuration. The polarimetric performances of the POLCAII experiment are under evaluation. Measurements with the improved POLCaliste experiment are foreseen in the 2010 at ESRF.

16 Conclusions (II) Very recently ASI funded a technological project named : “LAUE - A Gamma Ray Lens”. In this project our collaboration has the responsibility of the focal plane detector (4 x 4 cm2 , 0.5 mm spatial resolution, good energy resolution) for the test of the lens prototypes. In this framework one of the most appealing possibilities will be the use of an array of Calliste detectors in the new 256 channel version.


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