A low noise and wide dynamic range preamplifier for HPGe detectors
Purpose HPGe detectors can be used for both dark matter search and neutrinoless double beta decay experiments. However, signal amplitudes of these two experiments are quite different. This paper presents the development of a wide dynamic range CMOS preamplifier for HPGe detectors, which can also be...
Ausführliche Beschreibung
Gespeichert in:
| Autor*in: |
Hao, Jiajun [verfasserIn] Cheng, Zhengxi [verfasserIn] Ye, Xiangke [verfasserIn] He, Li [verfasserIn] Deng, Zhi [verfasserIn] |
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| Format: |
E-Artikel |
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| Sprache: |
Englisch |
| Erschienen: |
2024 |
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| Schlagwörter: |
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| Anmerkung: |
© The Author(s), under exclusive licence to Institute of High Energy Physics, Chinese Academy of Sciences 2024. Springer Nature or its licensor (e.g. a society or other partner) holds exclusive rights to this article under a publishing agreement with the author(s) or other rightsholder(s); author self-archiving of the accepted manuscript version of this article is solely governed by the terms of such publishing agreement and applicable law. |
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| Übergeordnetes Werk: |
Enthalten in: Radiation detection technology and methods - Springer Nature Singapore, 2017, 8(2024), 3 vom: 23. Apr., Seite 1413-1421 |
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| Übergeordnetes Werk: |
volume:8 ; year:2024 ; number:3 ; day:23 ; month:04 ; pages:1413-1421 |
| Links: |
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| DOI / URN: |
10.1007/s41605-024-00461-0 |
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| Katalog-ID: |
SPR057375720 |
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| 520 | |a Purpose HPGe detectors can be used for both dark matter search and neutrinoless double beta decay experiments. However, signal amplitudes of these two experiments are quite different. This paper presents the development of a wide dynamic range CMOS preamplifier for HPGe detectors, which can also be used for low light level photon detection. Methods The structure of a dual-stage dual-gain amplifier was adopted to receive the signals with charges ranging from ~ 0.01 fC to 500 fC. A novel “pre-reset” technique has been proposed to reduce the dead time ratio for large signals. A prototype chip was fabricated and tested. Results A minimum ENC of 43 electrons has been achieved for the high-gain channel at 77 K and the maximum charge of the input signal could be up to 500 fC for the low-gain channel, corresponding to a dynamic range above 90 dB. Conclusions The dual-gain structure of the preamplifier and the “pre-reset” method have been successfully verified, which can be used for HPGe detectors for dark matter and neutrino experiments in the future. | ||
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| 650 | 4 | |a Wide dynamic range |7 (dpeaa)DE-He213 | |
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| 650 | 4 | |a Cryogenic electronics |7 (dpeaa)DE-He213 | |
| 650 | 4 | |a HPGe detector |7 (dpeaa)DE-He213 | |
| 700 | 1 | |a Cheng, Zhengxi |e verfasserin |4 aut | |
| 700 | 1 | |a Ye, Xiangke |e verfasserin |4 aut | |
| 700 | 1 | |a He, Li |e verfasserin |4 aut | |
| 700 | 1 | |a Deng, Zhi |e verfasserin |0 (orcid)0000-0003-2767-1923 |4 aut | |
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10.1007/s41605-024-00461-0 doi (DE-627)SPR057375720 (SPR)s41605-024-00461-0-e DE-627 ger DE-627 rakwb eng 530 VZ 530 VZ Hao, Jiajun verfasserin aut A low noise and wide dynamic range preamplifier for HPGe detectors 2024 Text txt rdacontent Computermedien c rdamedia Online-Ressource cr rdacarrier © The Author(s), under exclusive licence to Institute of High Energy Physics, Chinese Academy of Sciences 2024. Springer Nature or its licensor (e.g. a society or other partner) holds exclusive rights to this article under a publishing agreement with the author(s) or other rightsholder(s); author self-archiving of the accepted manuscript version of this article is solely governed by the terms of such publishing agreement and applicable law. Purpose HPGe detectors can be used for both dark matter search and neutrinoless double beta decay experiments. However, signal amplitudes of these two experiments are quite different. This paper presents the development of a wide dynamic range CMOS preamplifier for HPGe detectors, which can also be used for low light level photon detection. Methods The structure of a dual-stage dual-gain amplifier was adopted to receive the signals with charges ranging from ~ 0.01 fC to 500 fC. A novel “pre-reset” technique has been proposed to reduce the dead time ratio for large signals. A prototype chip was fabricated and tested. Results A minimum ENC of 43 electrons has been achieved for the high-gain channel at 77 K and the maximum charge of the input signal could be up to 500 fC for the low-gain channel, corresponding to a dynamic range above 90 dB. Conclusions The dual-gain structure of the preamplifier and the “pre-reset” method have been successfully verified, which can be used for HPGe detectors for dark matter and neutrino experiments in the future. Low noise (dpeaa)DE-He213 Wide dynamic range (dpeaa)DE-He213 Charge sensitive preamplifier (dpeaa)DE-He213 CMOS ASIC (dpeaa)DE-He213 Cryogenic electronics (dpeaa)DE-He213 HPGe detector (dpeaa)DE-He213 Cheng, Zhengxi verfasserin aut Ye, Xiangke verfasserin aut He, Li verfasserin aut Deng, Zhi verfasserin (orcid)0000-0003-2767-1923 aut Enthalten in Radiation detection technology and methods Springer Nature Singapore, 2017 8(2024), 3 vom: 23. Apr., Seite 1413-1421 (DE-627)886059038 (DE-600)2893569-X 2509-9949 nnns volume:8 year:2024 number:3 day:23 month:04 pages:1413-1421 https://dx.doi.org/10.1007/s41605-024-00461-0 X:SPRINGER Resolving-System lizenzpflichtig Volltext SYSFLAG_0 GBV_SPRINGER GBV_ILN_11 GBV_ILN_20 GBV_ILN_22 GBV_ILN_23 GBV_ILN_24 GBV_ILN_31 GBV_ILN_32 GBV_ILN_39 GBV_ILN_40 GBV_ILN_60 GBV_ILN_62 GBV_ILN_63 GBV_ILN_65 GBV_ILN_69 GBV_ILN_70 GBV_ILN_73 GBV_ILN_74 GBV_ILN_90 GBV_ILN_95 GBV_ILN_100 GBV_ILN_101 GBV_ILN_105 GBV_ILN_110 GBV_ILN_120 GBV_ILN_138 GBV_ILN_150 GBV_ILN_151 GBV_ILN_152 GBV_ILN_161 GBV_ILN_170 GBV_ILN_171 GBV_ILN_187 GBV_ILN_213 GBV_ILN_224 GBV_ILN_230 GBV_ILN_250 GBV_ILN_266 GBV_ILN_281 GBV_ILN_285 GBV_ILN_293 GBV_ILN_370 GBV_ILN_602 GBV_ILN_636 GBV_ILN_702 GBV_ILN_2001 GBV_ILN_2003 GBV_ILN_2004 GBV_ILN_2005 GBV_ILN_2006 GBV_ILN_2007 GBV_ILN_2009 GBV_ILN_2010 GBV_ILN_2011 GBV_ILN_2014 GBV_ILN_2015 GBV_ILN_2020 GBV_ILN_2021 GBV_ILN_2025 GBV_ILN_2026 GBV_ILN_2027 GBV_ILN_2031 GBV_ILN_2034 GBV_ILN_2037 GBV_ILN_2038 GBV_ILN_2039 GBV_ILN_2044 GBV_ILN_2048 GBV_ILN_2049 GBV_ILN_2050 GBV_ILN_2055 GBV_ILN_2056 GBV_ILN_2057 GBV_ILN_2059 GBV_ILN_2061 GBV_ILN_2064 GBV_ILN_2065 GBV_ILN_2068 GBV_ILN_2088 GBV_ILN_2093 GBV_ILN_2106 GBV_ILN_2107 GBV_ILN_2108 GBV_ILN_2110 GBV_ILN_2111 GBV_ILN_2112 GBV_ILN_2113 GBV_ILN_2118 GBV_ILN_2122 GBV_ILN_2129 GBV_ILN_2143 GBV_ILN_2144 GBV_ILN_2147 GBV_ILN_2148 GBV_ILN_2152 GBV_ILN_2153 GBV_ILN_2188 GBV_ILN_2190 GBV_ILN_2232 GBV_ILN_2336 GBV_ILN_2446 GBV_ILN_2470 GBV_ILN_2472 GBV_ILN_2507 GBV_ILN_2522 GBV_ILN_2548 GBV_ILN_4035 GBV_ILN_4037 GBV_ILN_4046 GBV_ILN_4112 GBV_ILN_4125 GBV_ILN_4126 GBV_ILN_4242 GBV_ILN_4246 GBV_ILN_4249 GBV_ILN_4251 GBV_ILN_4305 GBV_ILN_4306 GBV_ILN_4307 GBV_ILN_4313 GBV_ILN_4322 GBV_ILN_4323 GBV_ILN_4324 GBV_ILN_4325 GBV_ILN_4326 GBV_ILN_4328 GBV_ILN_4333 GBV_ILN_4334 GBV_ILN_4335 GBV_ILN_4336 GBV_ILN_4338 GBV_ILN_4393 GBV_ILN_4700 AR 8 2024 3 23 04 1413-1421 |
| spelling |
10.1007/s41605-024-00461-0 doi (DE-627)SPR057375720 (SPR)s41605-024-00461-0-e DE-627 ger DE-627 rakwb eng 530 VZ 530 VZ Hao, Jiajun verfasserin aut A low noise and wide dynamic range preamplifier for HPGe detectors 2024 Text txt rdacontent Computermedien c rdamedia Online-Ressource cr rdacarrier © The Author(s), under exclusive licence to Institute of High Energy Physics, Chinese Academy of Sciences 2024. Springer Nature or its licensor (e.g. a society or other partner) holds exclusive rights to this article under a publishing agreement with the author(s) or other rightsholder(s); author self-archiving of the accepted manuscript version of this article is solely governed by the terms of such publishing agreement and applicable law. Purpose HPGe detectors can be used for both dark matter search and neutrinoless double beta decay experiments. However, signal amplitudes of these two experiments are quite different. This paper presents the development of a wide dynamic range CMOS preamplifier for HPGe detectors, which can also be used for low light level photon detection. Methods The structure of a dual-stage dual-gain amplifier was adopted to receive the signals with charges ranging from ~ 0.01 fC to 500 fC. A novel “pre-reset” technique has been proposed to reduce the dead time ratio for large signals. A prototype chip was fabricated and tested. Results A minimum ENC of 43 electrons has been achieved for the high-gain channel at 77 K and the maximum charge of the input signal could be up to 500 fC for the low-gain channel, corresponding to a dynamic range above 90 dB. Conclusions The dual-gain structure of the preamplifier and the “pre-reset” method have been successfully verified, which can be used for HPGe detectors for dark matter and neutrino experiments in the future. Low noise (dpeaa)DE-He213 Wide dynamic range (dpeaa)DE-He213 Charge sensitive preamplifier (dpeaa)DE-He213 CMOS ASIC (dpeaa)DE-He213 Cryogenic electronics (dpeaa)DE-He213 HPGe detector (dpeaa)DE-He213 Cheng, Zhengxi verfasserin aut Ye, Xiangke verfasserin aut He, Li verfasserin aut Deng, Zhi verfasserin (orcid)0000-0003-2767-1923 aut Enthalten in Radiation detection technology and methods Springer Nature Singapore, 2017 8(2024), 3 vom: 23. Apr., Seite 1413-1421 (DE-627)886059038 (DE-600)2893569-X 2509-9949 nnns volume:8 year:2024 number:3 day:23 month:04 pages:1413-1421 https://dx.doi.org/10.1007/s41605-024-00461-0 X:SPRINGER Resolving-System lizenzpflichtig Volltext SYSFLAG_0 GBV_SPRINGER GBV_ILN_11 GBV_ILN_20 GBV_ILN_22 GBV_ILN_23 GBV_ILN_24 GBV_ILN_31 GBV_ILN_32 GBV_ILN_39 GBV_ILN_40 GBV_ILN_60 GBV_ILN_62 GBV_ILN_63 GBV_ILN_65 GBV_ILN_69 GBV_ILN_70 GBV_ILN_73 GBV_ILN_74 GBV_ILN_90 GBV_ILN_95 GBV_ILN_100 GBV_ILN_101 GBV_ILN_105 GBV_ILN_110 GBV_ILN_120 GBV_ILN_138 GBV_ILN_150 GBV_ILN_151 GBV_ILN_152 GBV_ILN_161 GBV_ILN_170 GBV_ILN_171 GBV_ILN_187 GBV_ILN_213 GBV_ILN_224 GBV_ILN_230 GBV_ILN_250 GBV_ILN_266 GBV_ILN_281 GBV_ILN_285 GBV_ILN_293 GBV_ILN_370 GBV_ILN_602 GBV_ILN_636 GBV_ILN_702 GBV_ILN_2001 GBV_ILN_2003 GBV_ILN_2004 GBV_ILN_2005 GBV_ILN_2006 GBV_ILN_2007 GBV_ILN_2009 GBV_ILN_2010 GBV_ILN_2011 GBV_ILN_2014 GBV_ILN_2015 GBV_ILN_2020 GBV_ILN_2021 GBV_ILN_2025 GBV_ILN_2026 GBV_ILN_2027 GBV_ILN_2031 GBV_ILN_2034 GBV_ILN_2037 GBV_ILN_2038 GBV_ILN_2039 GBV_ILN_2044 GBV_ILN_2048 GBV_ILN_2049 GBV_ILN_2050 GBV_ILN_2055 GBV_ILN_2056 GBV_ILN_2057 GBV_ILN_2059 GBV_ILN_2061 GBV_ILN_2064 GBV_ILN_2065 GBV_ILN_2068 GBV_ILN_2088 GBV_ILN_2093 GBV_ILN_2106 GBV_ILN_2107 GBV_ILN_2108 GBV_ILN_2110 GBV_ILN_2111 GBV_ILN_2112 GBV_ILN_2113 GBV_ILN_2118 GBV_ILN_2122 GBV_ILN_2129 GBV_ILN_2143 GBV_ILN_2144 GBV_ILN_2147 GBV_ILN_2148 GBV_ILN_2152 GBV_ILN_2153 GBV_ILN_2188 GBV_ILN_2190 GBV_ILN_2232 GBV_ILN_2336 GBV_ILN_2446 GBV_ILN_2470 GBV_ILN_2472 GBV_ILN_2507 GBV_ILN_2522 GBV_ILN_2548 GBV_ILN_4035 GBV_ILN_4037 GBV_ILN_4046 GBV_ILN_4112 GBV_ILN_4125 GBV_ILN_4126 GBV_ILN_4242 GBV_ILN_4246 GBV_ILN_4249 GBV_ILN_4251 GBV_ILN_4305 GBV_ILN_4306 GBV_ILN_4307 GBV_ILN_4313 GBV_ILN_4322 GBV_ILN_4323 GBV_ILN_4324 GBV_ILN_4325 GBV_ILN_4326 GBV_ILN_4328 GBV_ILN_4333 GBV_ILN_4334 GBV_ILN_4335 GBV_ILN_4336 GBV_ILN_4338 GBV_ILN_4393 GBV_ILN_4700 AR 8 2024 3 23 04 1413-1421 |
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10.1007/s41605-024-00461-0 doi (DE-627)SPR057375720 (SPR)s41605-024-00461-0-e DE-627 ger DE-627 rakwb eng 530 VZ 530 VZ Hao, Jiajun verfasserin aut A low noise and wide dynamic range preamplifier for HPGe detectors 2024 Text txt rdacontent Computermedien c rdamedia Online-Ressource cr rdacarrier © The Author(s), under exclusive licence to Institute of High Energy Physics, Chinese Academy of Sciences 2024. Springer Nature or its licensor (e.g. a society or other partner) holds exclusive rights to this article under a publishing agreement with the author(s) or other rightsholder(s); author self-archiving of the accepted manuscript version of this article is solely governed by the terms of such publishing agreement and applicable law. Purpose HPGe detectors can be used for both dark matter search and neutrinoless double beta decay experiments. However, signal amplitudes of these two experiments are quite different. This paper presents the development of a wide dynamic range CMOS preamplifier for HPGe detectors, which can also be used for low light level photon detection. Methods The structure of a dual-stage dual-gain amplifier was adopted to receive the signals with charges ranging from ~ 0.01 fC to 500 fC. A novel “pre-reset” technique has been proposed to reduce the dead time ratio for large signals. A prototype chip was fabricated and tested. Results A minimum ENC of 43 electrons has been achieved for the high-gain channel at 77 K and the maximum charge of the input signal could be up to 500 fC for the low-gain channel, corresponding to a dynamic range above 90 dB. Conclusions The dual-gain structure of the preamplifier and the “pre-reset” method have been successfully verified, which can be used for HPGe detectors for dark matter and neutrino experiments in the future. Low noise (dpeaa)DE-He213 Wide dynamic range (dpeaa)DE-He213 Charge sensitive preamplifier (dpeaa)DE-He213 CMOS ASIC (dpeaa)DE-He213 Cryogenic electronics (dpeaa)DE-He213 HPGe detector (dpeaa)DE-He213 Cheng, Zhengxi verfasserin aut Ye, Xiangke verfasserin aut He, Li verfasserin aut Deng, Zhi verfasserin (orcid)0000-0003-2767-1923 aut Enthalten in Radiation detection technology and methods Springer Nature Singapore, 2017 8(2024), 3 vom: 23. Apr., Seite 1413-1421 (DE-627)886059038 (DE-600)2893569-X 2509-9949 nnns volume:8 year:2024 number:3 day:23 month:04 pages:1413-1421 https://dx.doi.org/10.1007/s41605-024-00461-0 X:SPRINGER Resolving-System lizenzpflichtig Volltext SYSFLAG_0 GBV_SPRINGER GBV_ILN_11 GBV_ILN_20 GBV_ILN_22 GBV_ILN_23 GBV_ILN_24 GBV_ILN_31 GBV_ILN_32 GBV_ILN_39 GBV_ILN_40 GBV_ILN_60 GBV_ILN_62 GBV_ILN_63 GBV_ILN_65 GBV_ILN_69 GBV_ILN_70 GBV_ILN_73 GBV_ILN_74 GBV_ILN_90 GBV_ILN_95 GBV_ILN_100 GBV_ILN_101 GBV_ILN_105 GBV_ILN_110 GBV_ILN_120 GBV_ILN_138 GBV_ILN_150 GBV_ILN_151 GBV_ILN_152 GBV_ILN_161 GBV_ILN_170 GBV_ILN_171 GBV_ILN_187 GBV_ILN_213 GBV_ILN_224 GBV_ILN_230 GBV_ILN_250 GBV_ILN_266 GBV_ILN_281 GBV_ILN_285 GBV_ILN_293 GBV_ILN_370 GBV_ILN_602 GBV_ILN_636 GBV_ILN_702 GBV_ILN_2001 GBV_ILN_2003 GBV_ILN_2004 GBV_ILN_2005 GBV_ILN_2006 GBV_ILN_2007 GBV_ILN_2009 GBV_ILN_2010 GBV_ILN_2011 GBV_ILN_2014 GBV_ILN_2015 GBV_ILN_2020 GBV_ILN_2021 GBV_ILN_2025 GBV_ILN_2026 GBV_ILN_2027 GBV_ILN_2031 GBV_ILN_2034 GBV_ILN_2037 GBV_ILN_2038 GBV_ILN_2039 GBV_ILN_2044 GBV_ILN_2048 GBV_ILN_2049 GBV_ILN_2050 GBV_ILN_2055 GBV_ILN_2056 GBV_ILN_2057 GBV_ILN_2059 GBV_ILN_2061 GBV_ILN_2064 GBV_ILN_2065 GBV_ILN_2068 GBV_ILN_2088 GBV_ILN_2093 GBV_ILN_2106 GBV_ILN_2107 GBV_ILN_2108 GBV_ILN_2110 GBV_ILN_2111 GBV_ILN_2112 GBV_ILN_2113 GBV_ILN_2118 GBV_ILN_2122 GBV_ILN_2129 GBV_ILN_2143 GBV_ILN_2144 GBV_ILN_2147 GBV_ILN_2148 GBV_ILN_2152 GBV_ILN_2153 GBV_ILN_2188 GBV_ILN_2190 GBV_ILN_2232 GBV_ILN_2336 GBV_ILN_2446 GBV_ILN_2470 GBV_ILN_2472 GBV_ILN_2507 GBV_ILN_2522 GBV_ILN_2548 GBV_ILN_4035 GBV_ILN_4037 GBV_ILN_4046 GBV_ILN_4112 GBV_ILN_4125 GBV_ILN_4126 GBV_ILN_4242 GBV_ILN_4246 GBV_ILN_4249 GBV_ILN_4251 GBV_ILN_4305 GBV_ILN_4306 GBV_ILN_4307 GBV_ILN_4313 GBV_ILN_4322 GBV_ILN_4323 GBV_ILN_4324 GBV_ILN_4325 GBV_ILN_4326 GBV_ILN_4328 GBV_ILN_4333 GBV_ILN_4334 GBV_ILN_4335 GBV_ILN_4336 GBV_ILN_4338 GBV_ILN_4393 GBV_ILN_4700 AR 8 2024 3 23 04 1413-1421 |
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10.1007/s41605-024-00461-0 doi (DE-627)SPR057375720 (SPR)s41605-024-00461-0-e DE-627 ger DE-627 rakwb eng 530 VZ 530 VZ Hao, Jiajun verfasserin aut A low noise and wide dynamic range preamplifier for HPGe detectors 2024 Text txt rdacontent Computermedien c rdamedia Online-Ressource cr rdacarrier © The Author(s), under exclusive licence to Institute of High Energy Physics, Chinese Academy of Sciences 2024. Springer Nature or its licensor (e.g. a society or other partner) holds exclusive rights to this article under a publishing agreement with the author(s) or other rightsholder(s); author self-archiving of the accepted manuscript version of this article is solely governed by the terms of such publishing agreement and applicable law. Purpose HPGe detectors can be used for both dark matter search and neutrinoless double beta decay experiments. However, signal amplitudes of these two experiments are quite different. This paper presents the development of a wide dynamic range CMOS preamplifier for HPGe detectors, which can also be used for low light level photon detection. Methods The structure of a dual-stage dual-gain amplifier was adopted to receive the signals with charges ranging from ~ 0.01 fC to 500 fC. A novel “pre-reset” technique has been proposed to reduce the dead time ratio for large signals. A prototype chip was fabricated and tested. Results A minimum ENC of 43 electrons has been achieved for the high-gain channel at 77 K and the maximum charge of the input signal could be up to 500 fC for the low-gain channel, corresponding to a dynamic range above 90 dB. Conclusions The dual-gain structure of the preamplifier and the “pre-reset” method have been successfully verified, which can be used for HPGe detectors for dark matter and neutrino experiments in the future. Low noise (dpeaa)DE-He213 Wide dynamic range (dpeaa)DE-He213 Charge sensitive preamplifier (dpeaa)DE-He213 CMOS ASIC (dpeaa)DE-He213 Cryogenic electronics (dpeaa)DE-He213 HPGe detector (dpeaa)DE-He213 Cheng, Zhengxi verfasserin aut Ye, Xiangke verfasserin aut He, Li verfasserin aut Deng, Zhi verfasserin (orcid)0000-0003-2767-1923 aut Enthalten in Radiation detection technology and methods Springer Nature Singapore, 2017 8(2024), 3 vom: 23. Apr., Seite 1413-1421 (DE-627)886059038 (DE-600)2893569-X 2509-9949 nnns volume:8 year:2024 number:3 day:23 month:04 pages:1413-1421 https://dx.doi.org/10.1007/s41605-024-00461-0 X:SPRINGER Resolving-System lizenzpflichtig Volltext SYSFLAG_0 GBV_SPRINGER GBV_ILN_11 GBV_ILN_20 GBV_ILN_22 GBV_ILN_23 GBV_ILN_24 GBV_ILN_31 GBV_ILN_32 GBV_ILN_39 GBV_ILN_40 GBV_ILN_60 GBV_ILN_62 GBV_ILN_63 GBV_ILN_65 GBV_ILN_69 GBV_ILN_70 GBV_ILN_73 GBV_ILN_74 GBV_ILN_90 GBV_ILN_95 GBV_ILN_100 GBV_ILN_101 GBV_ILN_105 GBV_ILN_110 GBV_ILN_120 GBV_ILN_138 GBV_ILN_150 GBV_ILN_151 GBV_ILN_152 GBV_ILN_161 GBV_ILN_170 GBV_ILN_171 GBV_ILN_187 GBV_ILN_213 GBV_ILN_224 GBV_ILN_230 GBV_ILN_250 GBV_ILN_266 GBV_ILN_281 GBV_ILN_285 GBV_ILN_293 GBV_ILN_370 GBV_ILN_602 GBV_ILN_636 GBV_ILN_702 GBV_ILN_2001 GBV_ILN_2003 GBV_ILN_2004 GBV_ILN_2005 GBV_ILN_2006 GBV_ILN_2007 GBV_ILN_2009 GBV_ILN_2010 GBV_ILN_2011 GBV_ILN_2014 GBV_ILN_2015 GBV_ILN_2020 GBV_ILN_2021 GBV_ILN_2025 GBV_ILN_2026 GBV_ILN_2027 GBV_ILN_2031 GBV_ILN_2034 GBV_ILN_2037 GBV_ILN_2038 GBV_ILN_2039 GBV_ILN_2044 GBV_ILN_2048 GBV_ILN_2049 GBV_ILN_2050 GBV_ILN_2055 GBV_ILN_2056 GBV_ILN_2057 GBV_ILN_2059 GBV_ILN_2061 GBV_ILN_2064 GBV_ILN_2065 GBV_ILN_2068 GBV_ILN_2088 GBV_ILN_2093 GBV_ILN_2106 GBV_ILN_2107 GBV_ILN_2108 GBV_ILN_2110 GBV_ILN_2111 GBV_ILN_2112 GBV_ILN_2113 GBV_ILN_2118 GBV_ILN_2122 GBV_ILN_2129 GBV_ILN_2143 GBV_ILN_2144 GBV_ILN_2147 GBV_ILN_2148 GBV_ILN_2152 GBV_ILN_2153 GBV_ILN_2188 GBV_ILN_2190 GBV_ILN_2232 GBV_ILN_2336 GBV_ILN_2446 GBV_ILN_2470 GBV_ILN_2472 GBV_ILN_2507 GBV_ILN_2522 GBV_ILN_2548 GBV_ILN_4035 GBV_ILN_4037 GBV_ILN_4046 GBV_ILN_4112 GBV_ILN_4125 GBV_ILN_4126 GBV_ILN_4242 GBV_ILN_4246 GBV_ILN_4249 GBV_ILN_4251 GBV_ILN_4305 GBV_ILN_4306 GBV_ILN_4307 GBV_ILN_4313 GBV_ILN_4322 GBV_ILN_4323 GBV_ILN_4324 GBV_ILN_4325 GBV_ILN_4326 GBV_ILN_4328 GBV_ILN_4333 GBV_ILN_4334 GBV_ILN_4335 GBV_ILN_4336 GBV_ILN_4338 GBV_ILN_4393 GBV_ILN_4700 AR 8 2024 3 23 04 1413-1421 |
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10.1007/s41605-024-00461-0 doi (DE-627)SPR057375720 (SPR)s41605-024-00461-0-e DE-627 ger DE-627 rakwb eng 530 VZ 530 VZ Hao, Jiajun verfasserin aut A low noise and wide dynamic range preamplifier for HPGe detectors 2024 Text txt rdacontent Computermedien c rdamedia Online-Ressource cr rdacarrier © The Author(s), under exclusive licence to Institute of High Energy Physics, Chinese Academy of Sciences 2024. Springer Nature or its licensor (e.g. a society or other partner) holds exclusive rights to this article under a publishing agreement with the author(s) or other rightsholder(s); author self-archiving of the accepted manuscript version of this article is solely governed by the terms of such publishing agreement and applicable law. Purpose HPGe detectors can be used for both dark matter search and neutrinoless double beta decay experiments. However, signal amplitudes of these two experiments are quite different. This paper presents the development of a wide dynamic range CMOS preamplifier for HPGe detectors, which can also be used for low light level photon detection. Methods The structure of a dual-stage dual-gain amplifier was adopted to receive the signals with charges ranging from ~ 0.01 fC to 500 fC. A novel “pre-reset” technique has been proposed to reduce the dead time ratio for large signals. A prototype chip was fabricated and tested. Results A minimum ENC of 43 electrons has been achieved for the high-gain channel at 77 K and the maximum charge of the input signal could be up to 500 fC for the low-gain channel, corresponding to a dynamic range above 90 dB. Conclusions The dual-gain structure of the preamplifier and the “pre-reset” method have been successfully verified, which can be used for HPGe detectors for dark matter and neutrino experiments in the future. Low noise (dpeaa)DE-He213 Wide dynamic range (dpeaa)DE-He213 Charge sensitive preamplifier (dpeaa)DE-He213 CMOS ASIC (dpeaa)DE-He213 Cryogenic electronics (dpeaa)DE-He213 HPGe detector (dpeaa)DE-He213 Cheng, Zhengxi verfasserin aut Ye, Xiangke verfasserin aut He, Li verfasserin aut Deng, Zhi verfasserin (orcid)0000-0003-2767-1923 aut Enthalten in Radiation detection technology and methods Springer Nature Singapore, 2017 8(2024), 3 vom: 23. Apr., Seite 1413-1421 (DE-627)886059038 (DE-600)2893569-X 2509-9949 nnns volume:8 year:2024 number:3 day:23 month:04 pages:1413-1421 https://dx.doi.org/10.1007/s41605-024-00461-0 X:SPRINGER Resolving-System lizenzpflichtig Volltext SYSFLAG_0 GBV_SPRINGER GBV_ILN_11 GBV_ILN_20 GBV_ILN_22 GBV_ILN_23 GBV_ILN_24 GBV_ILN_31 GBV_ILN_32 GBV_ILN_39 GBV_ILN_40 GBV_ILN_60 GBV_ILN_62 GBV_ILN_63 GBV_ILN_65 GBV_ILN_69 GBV_ILN_70 GBV_ILN_73 GBV_ILN_74 GBV_ILN_90 GBV_ILN_95 GBV_ILN_100 GBV_ILN_101 GBV_ILN_105 GBV_ILN_110 GBV_ILN_120 GBV_ILN_138 GBV_ILN_150 GBV_ILN_151 GBV_ILN_152 GBV_ILN_161 GBV_ILN_170 GBV_ILN_171 GBV_ILN_187 GBV_ILN_213 GBV_ILN_224 GBV_ILN_230 GBV_ILN_250 GBV_ILN_266 GBV_ILN_281 GBV_ILN_285 GBV_ILN_293 GBV_ILN_370 GBV_ILN_602 GBV_ILN_636 GBV_ILN_702 GBV_ILN_2001 GBV_ILN_2003 GBV_ILN_2004 GBV_ILN_2005 GBV_ILN_2006 GBV_ILN_2007 GBV_ILN_2009 GBV_ILN_2010 GBV_ILN_2011 GBV_ILN_2014 GBV_ILN_2015 GBV_ILN_2020 GBV_ILN_2021 GBV_ILN_2025 GBV_ILN_2026 GBV_ILN_2027 GBV_ILN_2031 GBV_ILN_2034 GBV_ILN_2037 GBV_ILN_2038 GBV_ILN_2039 GBV_ILN_2044 GBV_ILN_2048 GBV_ILN_2049 GBV_ILN_2050 GBV_ILN_2055 GBV_ILN_2056 GBV_ILN_2057 GBV_ILN_2059 GBV_ILN_2061 GBV_ILN_2064 GBV_ILN_2065 GBV_ILN_2068 GBV_ILN_2088 GBV_ILN_2093 GBV_ILN_2106 GBV_ILN_2107 GBV_ILN_2108 GBV_ILN_2110 GBV_ILN_2111 GBV_ILN_2112 GBV_ILN_2113 GBV_ILN_2118 GBV_ILN_2122 GBV_ILN_2129 GBV_ILN_2143 GBV_ILN_2144 GBV_ILN_2147 GBV_ILN_2148 GBV_ILN_2152 GBV_ILN_2153 GBV_ILN_2188 GBV_ILN_2190 GBV_ILN_2232 GBV_ILN_2336 GBV_ILN_2446 GBV_ILN_2470 GBV_ILN_2472 GBV_ILN_2507 GBV_ILN_2522 GBV_ILN_2548 GBV_ILN_4035 GBV_ILN_4037 GBV_ILN_4046 GBV_ILN_4112 GBV_ILN_4125 GBV_ILN_4126 GBV_ILN_4242 GBV_ILN_4246 GBV_ILN_4249 GBV_ILN_4251 GBV_ILN_4305 GBV_ILN_4306 GBV_ILN_4307 GBV_ILN_4313 GBV_ILN_4322 GBV_ILN_4323 GBV_ILN_4324 GBV_ILN_4325 GBV_ILN_4326 GBV_ILN_4328 GBV_ILN_4333 GBV_ILN_4334 GBV_ILN_4335 GBV_ILN_4336 GBV_ILN_4338 GBV_ILN_4393 GBV_ILN_4700 AR 8 2024 3 23 04 1413-1421 |
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Springer Nature or its licensor (e.g. a society or other partner) holds exclusive rights to this article under a publishing agreement with the author(s) or other rightsholder(s); author self-archiving of the accepted manuscript version of this article is solely governed by the terms of such publishing agreement and applicable law.</subfield></datafield><datafield tag="520" ind1=" " ind2=" "><subfield code="a">Purpose HPGe detectors can be used for both dark matter search and neutrinoless double beta decay experiments. However, signal amplitudes of these two experiments are quite different. This paper presents the development of a wide dynamic range CMOS preamplifier for HPGe detectors, which can also be used for low light level photon detection. Methods The structure of a dual-stage dual-gain amplifier was adopted to receive the signals with charges ranging from ~ 0.01 fC to 500 fC. A novel “pre-reset” technique has been proposed to reduce the dead time ratio for large signals. A prototype chip was fabricated and tested. Results A minimum ENC of 43 electrons has been achieved for the high-gain channel at 77 K and the maximum charge of the input signal could be up to 500 fC for the low-gain channel, corresponding to a dynamic range above 90 dB. Conclusions The dual-gain structure of the preamplifier and the “pre-reset” method have been successfully verified, which can be used for HPGe detectors for dark matter and neutrino experiments in the future.</subfield></datafield><datafield tag="650" ind1=" " ind2="4"><subfield code="a">Low noise</subfield><subfield code="7">(dpeaa)DE-He213</subfield></datafield><datafield tag="650" ind1=" " ind2="4"><subfield code="a">Wide dynamic range</subfield><subfield code="7">(dpeaa)DE-He213</subfield></datafield><datafield tag="650" ind1=" " ind2="4"><subfield code="a">Charge sensitive preamplifier</subfield><subfield code="7">(dpeaa)DE-He213</subfield></datafield><datafield tag="650" ind1=" " ind2="4"><subfield code="a">CMOS ASIC</subfield><subfield code="7">(dpeaa)DE-He213</subfield></datafield><datafield tag="650" ind1=" " ind2="4"><subfield code="a">Cryogenic electronics</subfield><subfield code="7">(dpeaa)DE-He213</subfield></datafield><datafield tag="650" ind1=" " ind2="4"><subfield code="a">HPGe detector</subfield><subfield code="7">(dpeaa)DE-He213</subfield></datafield><datafield tag="700" ind1="1" ind2=" "><subfield code="a">Cheng, Zhengxi</subfield><subfield code="e">verfasserin</subfield><subfield code="4">aut</subfield></datafield><datafield tag="700" ind1="1" ind2=" "><subfield code="a">Ye, Xiangke</subfield><subfield code="e">verfasserin</subfield><subfield code="4">aut</subfield></datafield><datafield tag="700" ind1="1" ind2=" "><subfield code="a">He, Li</subfield><subfield code="e">verfasserin</subfield><subfield code="4">aut</subfield></datafield><datafield tag="700" ind1="1" ind2=" "><subfield code="a">Deng, Zhi</subfield><subfield code="e">verfasserin</subfield><subfield code="0">(orcid)0000-0003-2767-1923</subfield><subfield code="4">aut</subfield></datafield><datafield tag="773" ind1="0" ind2="8"><subfield code="i">Enthalten in</subfield><subfield code="t">Radiation detection technology and methods</subfield><subfield code="d">Springer Nature Singapore, 2017</subfield><subfield code="g">8(2024), 3 vom: 23. 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Hao, Jiajun |
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530 VZ A low noise and wide dynamic range preamplifier for HPGe detectors Low noise (dpeaa)DE-He213 Wide dynamic range (dpeaa)DE-He213 Charge sensitive preamplifier (dpeaa)DE-He213 CMOS ASIC (dpeaa)DE-He213 Cryogenic electronics (dpeaa)DE-He213 HPGe detector (dpeaa)DE-He213 |
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ddc 530 misc Low noise misc Wide dynamic range misc Charge sensitive preamplifier misc CMOS ASIC misc Cryogenic electronics misc HPGe detector |
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a low noise and wide dynamic range preamplifier for hpge detectors |
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A low noise and wide dynamic range preamplifier for HPGe detectors |
| abstract |
Purpose HPGe detectors can be used for both dark matter search and neutrinoless double beta decay experiments. However, signal amplitudes of these two experiments are quite different. This paper presents the development of a wide dynamic range CMOS preamplifier for HPGe detectors, which can also be used for low light level photon detection. Methods The structure of a dual-stage dual-gain amplifier was adopted to receive the signals with charges ranging from ~ 0.01 fC to 500 fC. A novel “pre-reset” technique has been proposed to reduce the dead time ratio for large signals. A prototype chip was fabricated and tested. Results A minimum ENC of 43 electrons has been achieved for the high-gain channel at 77 K and the maximum charge of the input signal could be up to 500 fC for the low-gain channel, corresponding to a dynamic range above 90 dB. Conclusions The dual-gain structure of the preamplifier and the “pre-reset” method have been successfully verified, which can be used for HPGe detectors for dark matter and neutrino experiments in the future. © The Author(s), under exclusive licence to Institute of High Energy Physics, Chinese Academy of Sciences 2024. Springer Nature or its licensor (e.g. a society or other partner) holds exclusive rights to this article under a publishing agreement with the author(s) or other rightsholder(s); author self-archiving of the accepted manuscript version of this article is solely governed by the terms of such publishing agreement and applicable law. |
| abstractGer |
Purpose HPGe detectors can be used for both dark matter search and neutrinoless double beta decay experiments. However, signal amplitudes of these two experiments are quite different. This paper presents the development of a wide dynamic range CMOS preamplifier for HPGe detectors, which can also be used for low light level photon detection. Methods The structure of a dual-stage dual-gain amplifier was adopted to receive the signals with charges ranging from ~ 0.01 fC to 500 fC. A novel “pre-reset” technique has been proposed to reduce the dead time ratio for large signals. A prototype chip was fabricated and tested. Results A minimum ENC of 43 electrons has been achieved for the high-gain channel at 77 K and the maximum charge of the input signal could be up to 500 fC for the low-gain channel, corresponding to a dynamic range above 90 dB. Conclusions The dual-gain structure of the preamplifier and the “pre-reset” method have been successfully verified, which can be used for HPGe detectors for dark matter and neutrino experiments in the future. © The Author(s), under exclusive licence to Institute of High Energy Physics, Chinese Academy of Sciences 2024. Springer Nature or its licensor (e.g. a society or other partner) holds exclusive rights to this article under a publishing agreement with the author(s) or other rightsholder(s); author self-archiving of the accepted manuscript version of this article is solely governed by the terms of such publishing agreement and applicable law. |
| abstract_unstemmed |
Purpose HPGe detectors can be used for both dark matter search and neutrinoless double beta decay experiments. However, signal amplitudes of these two experiments are quite different. This paper presents the development of a wide dynamic range CMOS preamplifier for HPGe detectors, which can also be used for low light level photon detection. Methods The structure of a dual-stage dual-gain amplifier was adopted to receive the signals with charges ranging from ~ 0.01 fC to 500 fC. A novel “pre-reset” technique has been proposed to reduce the dead time ratio for large signals. A prototype chip was fabricated and tested. Results A minimum ENC of 43 electrons has been achieved for the high-gain channel at 77 K and the maximum charge of the input signal could be up to 500 fC for the low-gain channel, corresponding to a dynamic range above 90 dB. Conclusions The dual-gain structure of the preamplifier and the “pre-reset” method have been successfully verified, which can be used for HPGe detectors for dark matter and neutrino experiments in the future. © The Author(s), under exclusive licence to Institute of High Energy Physics, Chinese Academy of Sciences 2024. Springer Nature or its licensor (e.g. a society or other partner) holds exclusive rights to this article under a publishing agreement with the author(s) or other rightsholder(s); author self-archiving of the accepted manuscript version of this article is solely governed by the terms of such publishing agreement and applicable law. |
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| container_issue |
3 |
| title_short |
A low noise and wide dynamic range preamplifier for HPGe detectors |
| url |
https://dx.doi.org/10.1007/s41605-024-00461-0 |
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| author2 |
Cheng, Zhengxi Ye, Xiangke He, Li Deng, Zhi |
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Cheng, Zhengxi Ye, Xiangke He, Li Deng, Zhi |
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10.1007/s41605-024-00461-0 |
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2024-09-19T04:49:44.069Z |
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| score |
7.3988304 |