CUBE - XGLab
Transcription
CUBE - XGLab
High rate X-Ray spectroscopy with Silicon Drift Detectors coupled with “CUBE” front-end electronics L. Bombelli(1,2), R. Alberti(2), C. Fiorini(1), T. Frizzi(2), R. Quaglia(1) (1) Politecnico di Milano, Dip. Elettronica e Informazione, Piazza L. da Vinci 32, I-20133, Milano, Italy (2) XGLab SRL, via Moretto da Brescia 23, I-20133, Milano, Italy, ph. +390249660460, [email protected] Summary The development of radiation detectors for high-resolution X-ray spectroscopy is a research field of continuously growing interest, for its application either in scientific research (e.g. in synchrotron experiments) or in industrial applications like X-ray fluorescence, X-ray diffraction and microanalysis with SEM, just to make few examples. In most of the applications, especially when a mapping analysis is required, the general trend is to increase the count-rate. This reduces the measurement time or increases the accuracy thanks to the higher statistics. As a consequence, the performances of the system at short processing time are of primary concern. In this work, we compare the performances of our CUBE circuit with respect to the typical performances of the external JFET transistor. We will show that CUBE enables to get superior energy resolution at short shaping time. These CUBE characteristics lead to practical advantages in several industrial applications already cited, like the possibility to get high-rate spectroscopy still preserving enough energy resolution to identify light elements. CUBE’s main features Preamplifier design to replace the front-end JFET Advantages High signal level at the output of the module. No sensible loop outside the module. Possibility to drive “long” connection. Very low series noise. Superior performance respect to all the front-end JFET available at short shaping time. cooler Erengy resolution FWHM [eV] peaking time 0.5 us 170 1 us 160 2.2us 150 140 130 120 1 10 100 1000 30 Input Count rate [kcps] Mn-Ka shift [eV] Measures shows the possibility to have contextually close-to-optimum energy resolution and the highest counting rate. The shift of the Mn-Ka lines contains both potential changes of CUBE gains and gain/offset variation on the DPP. 1 10 170 160 0.1us 1 2 3 4 5 6 7 8 100 1000000 XRF measurement at Elettra synchrotron Sample: Zn deposition with trace of Ga Same detector type and assembly The CUBE advantages become evident in applications where a very fast analysis is required, like in XRF mapping applications. 0 -30 180 XRF applications 2.2 us -20 A Stable operation up to 1.5Mcps has been measured 190 Peaking time [us] 1 us -10 200 0 0.5 us 10 210 120 peaking time 20 JFET-based preamplifier 220 130 In application where an high flux of photons is available. The classical trade-off is the maximum output-count rate Vs. energy resolution. CUBE makes possible to readout the detector with a very short peaking time with an excellent energy resolution, in the past only possible with longer peaking times. 25mm2 SDD @ -30°C DPP with Trapezoidal filter The performances has been confirmed by testing CUBE with different SDD area, different SDD manufacturer and measurement conditions. The figure on the left report a comparison of the energy resolution at the Mn-Ka line measured with the same type of SDD (a circular 25mm2 SDD at -50° C) with CUBE and a more standard JFET readout. A commercial digital pulse processor with trapezoidal filter has been used. CUBE 230 140 High count-rate measurements with CUBE 180 0.2us 240 150 The possibility to have a small, low-power and monolithic preamplifier enable the readout of multi-channel detector even in 2-D pixelated detector. CUBE 250 1000 Measurement condition (A) Peaking time= 1us Input count rate = 100 kcps Output count rate = 73 kcps Dead time = 27% Energy resolution CUBE: 132eV @ Mn-ka JFET: 152eV @ Mn-ka CUBE Zn-Ka JFET 100000 Ga-Ka Zn-Kb 10000 Counts SDD 260 Escape Ga-Kb 1000 100 Primary Fe Ar Ca Al 10 1 1000 3000 5000 Measurement condition (B) Peaking time= 0,3us Input count rate = 800 kcps Output count rate = 360 kcps Dead time = 54% Energy resolution CUBE: 138eV @ Mn-ka JFET: N/A 7000 ADU 1000000 9000 Zn-Ka Zn-Kb JFET 100000 11000 Ga-Ka CUBE Escape Ga-Kb Primary 10000 Counts radiation entrance window 750um x 750um x 250um <6mW 3.4el ENC 4.4el ENC 7ns <30ns <125eV @ 6keV FWHM Mn-Ka Physical size Power Consumption Measured Noise (no SDD) Measured noise (with SDD) Rise time (no SDD) Rise time (with SDD) Best energy resolution Design TO8 Compatible Simulation shows that CUBE is a suitable CMOS preamplifier for SDD with external front-end readout. The best energy resolution achievable with a standard SDD is close to the state-of-the-art performances. The energy resolution at short shaping time is one of the best results reported so far for a SDD (147eV at 100ns peaking time) Fe 1000 Ar Ca Al 100 In collaboration with XAFS Beamline ELETTRA Trieste Dr. Olivi 10 1000 Input Count rate [kcps] 3000 5000 7000 9000 11000 ADU SDD operation with CUBE at warm temperature.... 165 155 150 145 T=-10°C 140 T=-30°C 135 T=-35°C T=-50°C 130 125 Advantages of full CMOS readout It is known that the operation of bipolar or JFET transistor is affected by extremely low temperature. The CMOS technology in intrinsically more robust respect to low temperature. The measured energy resolution below shows that CUBE work perfectly even when cooled down to a temperature of 50 K. Not only, the optimal resolution gets better due to the evident reduction of SDD leakage current. Also the CUBE performances improve with lower temperature due to an increase in the Mosfets trasconductance. 160 120 Square area SDD with 60 mm2 active area The SDD in not collimated. 155 0,5 1 1,5 2 2,5 3 3,5 4 4,5 Peaking Time (us) 152 eV resolution with large area SDD Cooled at only –10 °C with 0.5us peaking time. Fe spectrum 60 mm2 SDD SDD/CUBE at 50 K 220 55 210 Fe Energy resolution for a 80 mm2 collimated detector 55 200 190 180 T=-10 °C 170 T=-20 °C 160 T=-30 °C 150 T=-35 °C 140 130 150 Resolution FWHM (eV) 0 Resolution FWHM (eV) Resolution FWHM (eV) Advantages of very-low series noise Possibility to operate large-area SDDs with no resolution penalty. Higher thermal budget. Better high count-rate measurements. In handheld applications: less sensitive to room temperature, faster operation settling time, low-power Peltier required. 55 Fe Energy resolution for a 30 mm2 collimated detector 160 ...and at cryogenic temperature 145 240 K 140 200 K 160 K 110 K 135 50 K 130 125 120 120 0 0 0,5 1 1,5 2 2,5 Peaking Time (us) 3 3,5 4 4,5 0,5 1 1,5 2 2,5 3 3,5 4 Peaking time [us] The CUBE is suited for operation in Liquid Nitrogen in application with Ge detectors. to contact us [email protected]