Performance of novel VUV-sensitive Silicon Photo-Multipliers for nEXO
Abstract Liquid xenon time projection chambers are promising detectors to search for neutrinoless double beta decay (0%$\nu \beta \beta %$), due to their response uniformity, monolithic sensitive volume, scalability to large target masses, and suitability for extremely low background operations. The...
Ausführliche Beschreibung
Gespeichert in:
| Autor*in: |
Gallina, G. [verfasserIn] |
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| Format: |
E-Artikel |
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| Sprache: |
Englisch |
| Erschienen: |
2022 |
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| Anmerkung: |
© The Author(s) 2022 |
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| Übergeordnetes Werk: |
Enthalten in: The European physical journal - Berlin : Springer, 1998, 82(2022), 12 vom: 13. Dez. |
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| Übergeordnetes Werk: |
volume:82 ; year:2022 ; number:12 ; day:13 ; month:12 |
| Links: |
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| DOI / URN: |
10.1140/epjc/s10052-022-11072-8 |
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| Katalog-ID: |
SPR049502352 |
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| 041 | |a eng | ||
| 100 | 1 | |a Gallina, G. |e verfasserin |0 (orcid)0000-0002-9878-6499 |4 aut | |
| 245 | 1 | 0 | |a Performance of novel VUV-sensitive Silicon Photo-Multipliers for nEXO |
| 264 | 1 | |c 2022 | |
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| 500 | |a © The Author(s) 2022 | ||
| 520 | |a Abstract Liquid xenon time projection chambers are promising detectors to search for neutrinoless double beta decay (0%$\nu \beta \beta %$), due to their response uniformity, monolithic sensitive volume, scalability to large target masses, and suitability for extremely low background operations. The nEXO collaboration has designed a tonne-scale time projection chamber that aims to search for 0%$\nu \beta \beta %$ of %$^{136}%$Xe with projected half-life sensitivity of %$1.35\times 10^{28}%$ yr. To reach this sensitivity, the design goal for nEXO is %$\le %$1% energy resolution at the decay Q-value (%$2458.07\pm 0.31%$ keV). Reaching this resolution requires the efficient collection of both the ionization and scintillation produced in the detector. The nEXO design employs Silicon Photo-Multipliers (SiPMs) to detect the vacuum ultra-violet, 175 nm scintillation light of liquid xenon. This paper reports on the characterization of the newest vacuum ultra-violet sensitive Fondazione Bruno Kessler VUVHD3 SiPMs specifically designed for nEXO, as well as new measurements on new test samples of previously characterised Hamamatsu VUV4 Multi Pixel Photon Counters (MPPCs). Various SiPM and MPPC parameters, such as dark noise, gain, direct crosstalk, correlated avalanches and photon detection efficiency were measured as a function of the applied over voltage and wavelength at liquid xenon temperature (163 K). The results from this study are used to provide updated estimates of the achievable energy resolution at the decay Q-value for the nEXO design. | ||
| 700 | 1 | |a Guan, Y. |4 aut | |
| 700 | 1 | |a Retiere, F. |4 aut | |
| 700 | 1 | |a Cao, G. |4 aut | |
| 700 | 1 | |a Bolotnikov, A. |4 aut | |
| 700 | 1 | |a Kotov, I. |4 aut | |
| 700 | 1 | |a Rescia, S. |4 aut | |
| 700 | 1 | |a Soma, A. K. |4 aut | |
| 700 | 1 | |a Tsang, T. |4 aut | |
| 700 | 1 | |a Darroch, L. |4 aut | |
| 700 | 1 | |a Brunner, T. |4 aut | |
| 700 | 1 | |a Bolster, J. |4 aut | |
| 700 | 1 | |a Cohen, J. R. |4 aut | |
| 700 | 1 | |a Franco, T. Pinto |4 aut | |
| 700 | 1 | |a Gillis, W. C. |4 aut | |
| 700 | 1 | |a Smalley, H. Peltz |4 aut | |
| 700 | 1 | |a Thibado, S. |4 aut | |
| 700 | 1 | |a Pocar, A. |4 aut | |
| 700 | 1 | |a Bhat, A. |4 aut | |
| 700 | 1 | |a Jamil, A. |4 aut | |
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| 700 | 1 | |a Adhikari, G. |4 aut | |
| 700 | 1 | |a Kharusi, S. Al |4 aut | |
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10.1140/epjc/s10052-022-11072-8 doi (DE-627)SPR049502352 (SPR)s10052-022-11072-8-e DE-627 ger DE-627 rakwb eng Gallina, G. verfasserin (orcid)0000-0002-9878-6499 aut Performance of novel VUV-sensitive Silicon Photo-Multipliers for nEXO 2022 Text txt rdacontent Computermedien c rdamedia Online-Ressource cr rdacarrier © The Author(s) 2022 Abstract Liquid xenon time projection chambers are promising detectors to search for neutrinoless double beta decay (0%$\nu \beta \beta %$), due to their response uniformity, monolithic sensitive volume, scalability to large target masses, and suitability for extremely low background operations. The nEXO collaboration has designed a tonne-scale time projection chamber that aims to search for 0%$\nu \beta \beta %$ of %$^{136}%$Xe with projected half-life sensitivity of %$1.35\times 10^{28}%$ yr. To reach this sensitivity, the design goal for nEXO is %$\le %$1% energy resolution at the decay Q-value (%$2458.07\pm 0.31%$ keV). Reaching this resolution requires the efficient collection of both the ionization and scintillation produced in the detector. The nEXO design employs Silicon Photo-Multipliers (SiPMs) to detect the vacuum ultra-violet, 175 nm scintillation light of liquid xenon. This paper reports on the characterization of the newest vacuum ultra-violet sensitive Fondazione Bruno Kessler VUVHD3 SiPMs specifically designed for nEXO, as well as new measurements on new test samples of previously characterised Hamamatsu VUV4 Multi Pixel Photon Counters (MPPCs). Various SiPM and MPPC parameters, such as dark noise, gain, direct crosstalk, correlated avalanches and photon detection efficiency were measured as a function of the applied over voltage and wavelength at liquid xenon temperature (163 K). The results from this study are used to provide updated estimates of the achievable energy resolution at the decay Q-value for the nEXO design. Guan, Y. aut Retiere, F. aut Cao, G. aut Bolotnikov, A. aut Kotov, I. aut Rescia, S. aut Soma, A. K. aut Tsang, T. aut Darroch, L. aut Brunner, T. aut Bolster, J. aut Cohen, J. R. aut Franco, T. Pinto aut Gillis, W. C. aut Smalley, H. Peltz aut Thibado, S. aut Pocar, A. aut Bhat, A. aut Jamil, A. aut Moore, D. C. aut Adhikari, G. aut Kharusi, S. Al aut Angelico, E. aut Arnquist, I. J. aut Arsenault, P. aut Badhrees, I. aut Bane, J. aut Belov, V. aut Bernard, E. P. aut Bhatta, T. aut Breur, P. A. aut Brodsky, J. P. aut Brown, E. aut Caden, E. aut Cao, L. aut Chambers, C. aut Chana, B. aut Charlebois, S. A. aut Chernyak, D. aut Chiu, M. aut Cleveland, B. aut Collister, R. aut Cvitan, M. aut Dalmasson, J. aut Daniels, T. aut Deslandes, K. aut DeVoe, R. aut di Vacri, M. L. aut Ding, Y. aut Dolinski, M. J. aut Dragone, A. aut Echevers, J. aut Eckert, B. aut Elbeltagi, M. aut Fabris, L. aut Fairbank, W. aut Farine, J. aut Fu, Y. S. aut Gallacher, D. aut Gautam, P. aut Giacomini, G. aut Gingras, C. aut Goeldi, D. aut Gornea, R. aut Gratta, G. aut Hardy, C. A. aut Hedges, S. aut Heffner, M. aut Hein, E. aut Holt, J. aut Hoppe, E. W. aut Hößl, J. aut House, A. aut Hunt, W. aut Iverson, A. aut Jiang, X. S. aut Karelin, A. aut Kaufman, L. J. aut Krücken, R. aut Kuchenkov, A. aut Kumar, K. S. aut Larson, A. aut Leach, K. G. aut Lenardo, B. G. aut Leonard, D. S. aut Lessard, G. aut Li, G. aut Li, S. aut Li, Z. aut Licciardi, C. aut Lindsay, R. aut MacLellan, R. aut Mahtab, M. aut Majidi, S. aut Malbrunot, C. aut Margetak, P. aut Martel-Dion, P. aut Martin, L. aut Masbou, J. aut Massacret, N. aut McMichael, K. aut Mong, B. aut Murray, K. aut Nattress, J. aut Natzke, C. R. aut Ngwadla, X. E. aut Ondze, J. C. Nzobadila aut Odian, A. aut Orrell, J. L. aut Ortega, G. S. aut Overman, C. T. aut Parent, S. aut Perna, A. aut Piepke, A. aut Pletskova, N. aut Pratte, J. F. aut Radeka, V. aut Raguzin, E. aut Ramonnye, G. J. aut Rao, T. aut Rasiwala, H. aut Raymond, K. aut Rebeiro, B. M. aut Richardson, G. aut Ringuette, J. aut Riot, V. aut Rossignol, T. aut Rowson, P. C. aut Rudolph, L. aut Saldanha, R. aut Sangiorgio, S. aut Shang, X. aut Spadoni, F. aut Stekhanov, V. aut Sun, X. L. aut Tidball, A. aut Totev, T. aut Triambak, S. aut Tsang, R. H. M. aut Tyuka, O. A. aut Vachon, F. aut Vidal, M. aut Viel, S. aut Visser, G. aut Wagenpfeil, M. aut Walent, M. aut Wamba, K. aut Wang, Q. aut Wang, W. aut Wang, Y. aut Watts, M. aut Wei, W. aut Wen, L. J. aut Wichoski, U. aut Wilde, S. aut Worcester, M. aut Wu, W. H. aut Wu, X. aut Xie, L. aut Yan, W. aut Yang, H. aut Yang, L. aut Zeldovich, O. aut Zhao, J. aut Ziegler, T. aut Enthalten in The European physical journal Berlin : Springer, 1998 82(2022), 12 vom: 13. Dez. (DE-627)253722934 (DE-600)1459069-4 1434-6052 nnns volume:82 year:2022 number:12 day:13 month:12 https://dx.doi.org/10.1140/epjc/s10052-022-11072-8 kostenfrei Volltext GBV_USEFLAG_A SYSFLAG_A GBV_SPRINGER GBV_ILN_11 GBV_ILN_20 GBV_ILN_22 GBV_ILN_23 GBV_ILN_24 GBV_ILN_31 GBV_ILN_39 GBV_ILN_40 GBV_ILN_60 GBV_ILN_62 GBV_ILN_63 GBV_ILN_69 GBV_ILN_70 GBV_ILN_73 GBV_ILN_95 GBV_ILN_105 GBV_ILN_110 GBV_ILN_150 GBV_ILN_151 GBV_ILN_161 GBV_ILN_170 GBV_ILN_206 GBV_ILN_213 GBV_ILN_230 GBV_ILN_267 GBV_ILN_285 GBV_ILN_293 GBV_ILN_370 GBV_ILN_602 GBV_ILN_702 GBV_ILN_2001 GBV_ILN_2003 GBV_ILN_2005 GBV_ILN_2006 GBV_ILN_2008 GBV_ILN_2009 GBV_ILN_2010 GBV_ILN_2011 GBV_ILN_2014 GBV_ILN_2015 GBV_ILN_2018 GBV_ILN_2020 GBV_ILN_2021 GBV_ILN_2025 GBV_ILN_2031 GBV_ILN_2038 GBV_ILN_2044 GBV_ILN_2048 GBV_ILN_2050 GBV_ILN_2055 GBV_ILN_2056 GBV_ILN_2057 GBV_ILN_2061 GBV_ILN_2108 GBV_ILN_2111 GBV_ILN_2113 GBV_ILN_2119 GBV_ILN_2190 GBV_ILN_4012 GBV_ILN_4037 GBV_ILN_4112 GBV_ILN_4125 GBV_ILN_4126 GBV_ILN_4246 GBV_ILN_4249 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_4335 GBV_ILN_4338 GBV_ILN_4367 GBV_ILN_4700 AR 82 2022 12 13 12 |
| spelling |
10.1140/epjc/s10052-022-11072-8 doi (DE-627)SPR049502352 (SPR)s10052-022-11072-8-e DE-627 ger DE-627 rakwb eng Gallina, G. verfasserin (orcid)0000-0002-9878-6499 aut Performance of novel VUV-sensitive Silicon Photo-Multipliers for nEXO 2022 Text txt rdacontent Computermedien c rdamedia Online-Ressource cr rdacarrier © The Author(s) 2022 Abstract Liquid xenon time projection chambers are promising detectors to search for neutrinoless double beta decay (0%$\nu \beta \beta %$), due to their response uniformity, monolithic sensitive volume, scalability to large target masses, and suitability for extremely low background operations. The nEXO collaboration has designed a tonne-scale time projection chamber that aims to search for 0%$\nu \beta \beta %$ of %$^{136}%$Xe with projected half-life sensitivity of %$1.35\times 10^{28}%$ yr. To reach this sensitivity, the design goal for nEXO is %$\le %$1% energy resolution at the decay Q-value (%$2458.07\pm 0.31%$ keV). Reaching this resolution requires the efficient collection of both the ionization and scintillation produced in the detector. The nEXO design employs Silicon Photo-Multipliers (SiPMs) to detect the vacuum ultra-violet, 175 nm scintillation light of liquid xenon. This paper reports on the characterization of the newest vacuum ultra-violet sensitive Fondazione Bruno Kessler VUVHD3 SiPMs specifically designed for nEXO, as well as new measurements on new test samples of previously characterised Hamamatsu VUV4 Multi Pixel Photon Counters (MPPCs). Various SiPM and MPPC parameters, such as dark noise, gain, direct crosstalk, correlated avalanches and photon detection efficiency were measured as a function of the applied over voltage and wavelength at liquid xenon temperature (163 K). The results from this study are used to provide updated estimates of the achievable energy resolution at the decay Q-value for the nEXO design. Guan, Y. aut Retiere, F. aut Cao, G. aut Bolotnikov, A. aut Kotov, I. aut Rescia, S. aut Soma, A. K. aut Tsang, T. aut Darroch, L. aut Brunner, T. aut Bolster, J. aut Cohen, J. R. aut Franco, T. Pinto aut Gillis, W. C. aut Smalley, H. Peltz aut Thibado, S. aut Pocar, A. aut Bhat, A. aut Jamil, A. aut Moore, D. C. aut Adhikari, G. aut Kharusi, S. Al aut Angelico, E. aut Arnquist, I. J. aut Arsenault, P. aut Badhrees, I. aut Bane, J. aut Belov, V. aut Bernard, E. P. aut Bhatta, T. aut Breur, P. A. aut Brodsky, J. P. aut Brown, E. aut Caden, E. aut Cao, L. aut Chambers, C. aut Chana, B. aut Charlebois, S. A. aut Chernyak, D. aut Chiu, M. aut Cleveland, B. aut Collister, R. aut Cvitan, M. aut Dalmasson, J. aut Daniels, T. aut Deslandes, K. aut DeVoe, R. aut di Vacri, M. L. aut Ding, Y. aut Dolinski, M. J. aut Dragone, A. aut Echevers, J. aut Eckert, B. aut Elbeltagi, M. aut Fabris, L. aut Fairbank, W. aut Farine, J. aut Fu, Y. S. aut Gallacher, D. aut Gautam, P. aut Giacomini, G. aut Gingras, C. aut Goeldi, D. aut Gornea, R. aut Gratta, G. aut Hardy, C. A. aut Hedges, S. aut Heffner, M. aut Hein, E. aut Holt, J. aut Hoppe, E. W. aut Hößl, J. aut House, A. aut Hunt, W. aut Iverson, A. aut Jiang, X. S. aut Karelin, A. aut Kaufman, L. J. aut Krücken, R. aut Kuchenkov, A. aut Kumar, K. S. aut Larson, A. aut Leach, K. G. aut Lenardo, B. G. aut Leonard, D. S. aut Lessard, G. aut Li, G. aut Li, S. aut Li, Z. aut Licciardi, C. aut Lindsay, R. aut MacLellan, R. aut Mahtab, M. aut Majidi, S. aut Malbrunot, C. aut Margetak, P. aut Martel-Dion, P. aut Martin, L. aut Masbou, J. aut Massacret, N. aut McMichael, K. aut Mong, B. aut Murray, K. aut Nattress, J. aut Natzke, C. R. aut Ngwadla, X. E. aut Ondze, J. C. Nzobadila aut Odian, A. aut Orrell, J. L. aut Ortega, G. S. aut Overman, C. T. aut Parent, S. aut Perna, A. aut Piepke, A. aut Pletskova, N. aut Pratte, J. F. aut Radeka, V. aut Raguzin, E. aut Ramonnye, G. J. aut Rao, T. aut Rasiwala, H. aut Raymond, K. aut Rebeiro, B. M. aut Richardson, G. aut Ringuette, J. aut Riot, V. aut Rossignol, T. aut Rowson, P. C. aut Rudolph, L. aut Saldanha, R. aut Sangiorgio, S. aut Shang, X. aut Spadoni, F. aut Stekhanov, V. aut Sun, X. L. aut Tidball, A. aut Totev, T. aut Triambak, S. aut Tsang, R. H. M. aut Tyuka, O. A. aut Vachon, F. aut Vidal, M. aut Viel, S. aut Visser, G. aut Wagenpfeil, M. aut Walent, M. aut Wamba, K. aut Wang, Q. aut Wang, W. aut Wang, Y. aut Watts, M. aut Wei, W. aut Wen, L. J. aut Wichoski, U. aut Wilde, S. aut Worcester, M. aut Wu, W. H. aut Wu, X. aut Xie, L. aut Yan, W. aut Yang, H. aut Yang, L. aut Zeldovich, O. aut Zhao, J. aut Ziegler, T. aut Enthalten in The European physical journal Berlin : Springer, 1998 82(2022), 12 vom: 13. Dez. (DE-627)253722934 (DE-600)1459069-4 1434-6052 nnns volume:82 year:2022 number:12 day:13 month:12 https://dx.doi.org/10.1140/epjc/s10052-022-11072-8 kostenfrei Volltext GBV_USEFLAG_A SYSFLAG_A GBV_SPRINGER GBV_ILN_11 GBV_ILN_20 GBV_ILN_22 GBV_ILN_23 GBV_ILN_24 GBV_ILN_31 GBV_ILN_39 GBV_ILN_40 GBV_ILN_60 GBV_ILN_62 GBV_ILN_63 GBV_ILN_69 GBV_ILN_70 GBV_ILN_73 GBV_ILN_95 GBV_ILN_105 GBV_ILN_110 GBV_ILN_150 GBV_ILN_151 GBV_ILN_161 GBV_ILN_170 GBV_ILN_206 GBV_ILN_213 GBV_ILN_230 GBV_ILN_267 GBV_ILN_285 GBV_ILN_293 GBV_ILN_370 GBV_ILN_602 GBV_ILN_702 GBV_ILN_2001 GBV_ILN_2003 GBV_ILN_2005 GBV_ILN_2006 GBV_ILN_2008 GBV_ILN_2009 GBV_ILN_2010 GBV_ILN_2011 GBV_ILN_2014 GBV_ILN_2015 GBV_ILN_2018 GBV_ILN_2020 GBV_ILN_2021 GBV_ILN_2025 GBV_ILN_2031 GBV_ILN_2038 GBV_ILN_2044 GBV_ILN_2048 GBV_ILN_2050 GBV_ILN_2055 GBV_ILN_2056 GBV_ILN_2057 GBV_ILN_2061 GBV_ILN_2108 GBV_ILN_2111 GBV_ILN_2113 GBV_ILN_2119 GBV_ILN_2190 GBV_ILN_4012 GBV_ILN_4037 GBV_ILN_4112 GBV_ILN_4125 GBV_ILN_4126 GBV_ILN_4246 GBV_ILN_4249 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_4335 GBV_ILN_4338 GBV_ILN_4367 GBV_ILN_4700 AR 82 2022 12 13 12 |
| allfields_unstemmed |
10.1140/epjc/s10052-022-11072-8 doi (DE-627)SPR049502352 (SPR)s10052-022-11072-8-e DE-627 ger DE-627 rakwb eng Gallina, G. verfasserin (orcid)0000-0002-9878-6499 aut Performance of novel VUV-sensitive Silicon Photo-Multipliers for nEXO 2022 Text txt rdacontent Computermedien c rdamedia Online-Ressource cr rdacarrier © The Author(s) 2022 Abstract Liquid xenon time projection chambers are promising detectors to search for neutrinoless double beta decay (0%$\nu \beta \beta %$), due to their response uniformity, monolithic sensitive volume, scalability to large target masses, and suitability for extremely low background operations. The nEXO collaboration has designed a tonne-scale time projection chamber that aims to search for 0%$\nu \beta \beta %$ of %$^{136}%$Xe with projected half-life sensitivity of %$1.35\times 10^{28}%$ yr. To reach this sensitivity, the design goal for nEXO is %$\le %$1% energy resolution at the decay Q-value (%$2458.07\pm 0.31%$ keV). Reaching this resolution requires the efficient collection of both the ionization and scintillation produced in the detector. The nEXO design employs Silicon Photo-Multipliers (SiPMs) to detect the vacuum ultra-violet, 175 nm scintillation light of liquid xenon. This paper reports on the characterization of the newest vacuum ultra-violet sensitive Fondazione Bruno Kessler VUVHD3 SiPMs specifically designed for nEXO, as well as new measurements on new test samples of previously characterised Hamamatsu VUV4 Multi Pixel Photon Counters (MPPCs). Various SiPM and MPPC parameters, such as dark noise, gain, direct crosstalk, correlated avalanches and photon detection efficiency were measured as a function of the applied over voltage and wavelength at liquid xenon temperature (163 K). The results from this study are used to provide updated estimates of the achievable energy resolution at the decay Q-value for the nEXO design. Guan, Y. aut Retiere, F. aut Cao, G. aut Bolotnikov, A. aut Kotov, I. aut Rescia, S. aut Soma, A. K. aut Tsang, T. aut Darroch, L. aut Brunner, T. aut Bolster, J. aut Cohen, J. R. aut Franco, T. Pinto aut Gillis, W. C. aut Smalley, H. Peltz aut Thibado, S. aut Pocar, A. aut Bhat, A. aut Jamil, A. aut Moore, D. C. aut Adhikari, G. aut Kharusi, S. Al aut Angelico, E. aut Arnquist, I. J. aut Arsenault, P. aut Badhrees, I. aut Bane, J. aut Belov, V. aut Bernard, E. P. aut Bhatta, T. aut Breur, P. A. aut Brodsky, J. P. aut Brown, E. aut Caden, E. aut Cao, L. aut Chambers, C. aut Chana, B. aut Charlebois, S. A. aut Chernyak, D. aut Chiu, M. aut Cleveland, B. aut Collister, R. aut Cvitan, M. aut Dalmasson, J. aut Daniels, T. aut Deslandes, K. aut DeVoe, R. aut di Vacri, M. L. aut Ding, Y. aut Dolinski, M. J. aut Dragone, A. aut Echevers, J. aut Eckert, B. aut Elbeltagi, M. aut Fabris, L. aut Fairbank, W. aut Farine, J. aut Fu, Y. S. aut Gallacher, D. aut Gautam, P. aut Giacomini, G. aut Gingras, C. aut Goeldi, D. aut Gornea, R. aut Gratta, G. aut Hardy, C. A. aut Hedges, S. aut Heffner, M. aut Hein, E. aut Holt, J. aut Hoppe, E. W. aut Hößl, J. aut House, A. aut Hunt, W. aut Iverson, A. aut Jiang, X. S. aut Karelin, A. aut Kaufman, L. J. aut Krücken, R. aut Kuchenkov, A. aut Kumar, K. S. aut Larson, A. aut Leach, K. G. aut Lenardo, B. G. aut Leonard, D. S. aut Lessard, G. aut Li, G. aut Li, S. aut Li, Z. aut Licciardi, C. aut Lindsay, R. aut MacLellan, R. aut Mahtab, M. aut Majidi, S. aut Malbrunot, C. aut Margetak, P. aut Martel-Dion, P. aut Martin, L. aut Masbou, J. aut Massacret, N. aut McMichael, K. aut Mong, B. aut Murray, K. aut Nattress, J. aut Natzke, C. R. aut Ngwadla, X. E. aut Ondze, J. C. Nzobadila aut Odian, A. aut Orrell, J. L. aut Ortega, G. S. aut Overman, C. T. aut Parent, S. aut Perna, A. aut Piepke, A. aut Pletskova, N. aut Pratte, J. F. aut Radeka, V. aut Raguzin, E. aut Ramonnye, G. J. aut Rao, T. aut Rasiwala, H. aut Raymond, K. aut Rebeiro, B. M. aut Richardson, G. aut Ringuette, J. aut Riot, V. aut Rossignol, T. aut Rowson, P. C. aut Rudolph, L. aut Saldanha, R. aut Sangiorgio, S. aut Shang, X. aut Spadoni, F. aut Stekhanov, V. aut Sun, X. L. aut Tidball, A. aut Totev, T. aut Triambak, S. aut Tsang, R. H. M. aut Tyuka, O. A. aut Vachon, F. aut Vidal, M. aut Viel, S. aut Visser, G. aut Wagenpfeil, M. aut Walent, M. aut Wamba, K. aut Wang, Q. aut Wang, W. aut Wang, Y. aut Watts, M. aut Wei, W. aut Wen, L. J. aut Wichoski, U. aut Wilde, S. aut Worcester, M. aut Wu, W. H. aut Wu, X. aut Xie, L. aut Yan, W. aut Yang, H. aut Yang, L. aut Zeldovich, O. aut Zhao, J. aut Ziegler, T. aut Enthalten in The European physical journal Berlin : Springer, 1998 82(2022), 12 vom: 13. Dez. (DE-627)253722934 (DE-600)1459069-4 1434-6052 nnns volume:82 year:2022 number:12 day:13 month:12 https://dx.doi.org/10.1140/epjc/s10052-022-11072-8 kostenfrei Volltext GBV_USEFLAG_A SYSFLAG_A GBV_SPRINGER GBV_ILN_11 GBV_ILN_20 GBV_ILN_22 GBV_ILN_23 GBV_ILN_24 GBV_ILN_31 GBV_ILN_39 GBV_ILN_40 GBV_ILN_60 GBV_ILN_62 GBV_ILN_63 GBV_ILN_69 GBV_ILN_70 GBV_ILN_73 GBV_ILN_95 GBV_ILN_105 GBV_ILN_110 GBV_ILN_150 GBV_ILN_151 GBV_ILN_161 GBV_ILN_170 GBV_ILN_206 GBV_ILN_213 GBV_ILN_230 GBV_ILN_267 GBV_ILN_285 GBV_ILN_293 GBV_ILN_370 GBV_ILN_602 GBV_ILN_702 GBV_ILN_2001 GBV_ILN_2003 GBV_ILN_2005 GBV_ILN_2006 GBV_ILN_2008 GBV_ILN_2009 GBV_ILN_2010 GBV_ILN_2011 GBV_ILN_2014 GBV_ILN_2015 GBV_ILN_2018 GBV_ILN_2020 GBV_ILN_2021 GBV_ILN_2025 GBV_ILN_2031 GBV_ILN_2038 GBV_ILN_2044 GBV_ILN_2048 GBV_ILN_2050 GBV_ILN_2055 GBV_ILN_2056 GBV_ILN_2057 GBV_ILN_2061 GBV_ILN_2108 GBV_ILN_2111 GBV_ILN_2113 GBV_ILN_2119 GBV_ILN_2190 GBV_ILN_4012 GBV_ILN_4037 GBV_ILN_4112 GBV_ILN_4125 GBV_ILN_4126 GBV_ILN_4246 GBV_ILN_4249 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_4335 GBV_ILN_4338 GBV_ILN_4367 GBV_ILN_4700 AR 82 2022 12 13 12 |
| allfieldsGer |
10.1140/epjc/s10052-022-11072-8 doi (DE-627)SPR049502352 (SPR)s10052-022-11072-8-e DE-627 ger DE-627 rakwb eng Gallina, G. verfasserin (orcid)0000-0002-9878-6499 aut Performance of novel VUV-sensitive Silicon Photo-Multipliers for nEXO 2022 Text txt rdacontent Computermedien c rdamedia Online-Ressource cr rdacarrier © The Author(s) 2022 Abstract Liquid xenon time projection chambers are promising detectors to search for neutrinoless double beta decay (0%$\nu \beta \beta %$), due to their response uniformity, monolithic sensitive volume, scalability to large target masses, and suitability for extremely low background operations. The nEXO collaboration has designed a tonne-scale time projection chamber that aims to search for 0%$\nu \beta \beta %$ of %$^{136}%$Xe with projected half-life sensitivity of %$1.35\times 10^{28}%$ yr. To reach this sensitivity, the design goal for nEXO is %$\le %$1% energy resolution at the decay Q-value (%$2458.07\pm 0.31%$ keV). Reaching this resolution requires the efficient collection of both the ionization and scintillation produced in the detector. The nEXO design employs Silicon Photo-Multipliers (SiPMs) to detect the vacuum ultra-violet, 175 nm scintillation light of liquid xenon. This paper reports on the characterization of the newest vacuum ultra-violet sensitive Fondazione Bruno Kessler VUVHD3 SiPMs specifically designed for nEXO, as well as new measurements on new test samples of previously characterised Hamamatsu VUV4 Multi Pixel Photon Counters (MPPCs). Various SiPM and MPPC parameters, such as dark noise, gain, direct crosstalk, correlated avalanches and photon detection efficiency were measured as a function of the applied over voltage and wavelength at liquid xenon temperature (163 K). The results from this study are used to provide updated estimates of the achievable energy resolution at the decay Q-value for the nEXO design. Guan, Y. aut Retiere, F. aut Cao, G. aut Bolotnikov, A. aut Kotov, I. aut Rescia, S. aut Soma, A. K. aut Tsang, T. aut Darroch, L. aut Brunner, T. aut Bolster, J. aut Cohen, J. R. aut Franco, T. Pinto aut Gillis, W. C. aut Smalley, H. Peltz aut Thibado, S. aut Pocar, A. aut Bhat, A. aut Jamil, A. aut Moore, D. C. aut Adhikari, G. aut Kharusi, S. Al aut Angelico, E. aut Arnquist, I. J. aut Arsenault, P. aut Badhrees, I. aut Bane, J. aut Belov, V. aut Bernard, E. P. aut Bhatta, T. aut Breur, P. A. aut Brodsky, J. P. aut Brown, E. aut Caden, E. aut Cao, L. aut Chambers, C. aut Chana, B. aut Charlebois, S. A. aut Chernyak, D. aut Chiu, M. aut Cleveland, B. aut Collister, R. aut Cvitan, M. aut Dalmasson, J. aut Daniels, T. aut Deslandes, K. aut DeVoe, R. aut di Vacri, M. L. aut Ding, Y. aut Dolinski, M. J. aut Dragone, A. aut Echevers, J. aut Eckert, B. aut Elbeltagi, M. aut Fabris, L. aut Fairbank, W. aut Farine, J. aut Fu, Y. S. aut Gallacher, D. aut Gautam, P. aut Giacomini, G. aut Gingras, C. aut Goeldi, D. aut Gornea, R. aut Gratta, G. aut Hardy, C. A. aut Hedges, S. aut Heffner, M. aut Hein, E. aut Holt, J. aut Hoppe, E. W. aut Hößl, J. aut House, A. aut Hunt, W. aut Iverson, A. aut Jiang, X. S. aut Karelin, A. aut Kaufman, L. J. aut Krücken, R. aut Kuchenkov, A. aut Kumar, K. S. aut Larson, A. aut Leach, K. G. aut Lenardo, B. G. aut Leonard, D. S. aut Lessard, G. aut Li, G. aut Li, S. aut Li, Z. aut Licciardi, C. aut Lindsay, R. aut MacLellan, R. aut Mahtab, M. aut Majidi, S. aut Malbrunot, C. aut Margetak, P. aut Martel-Dion, P. aut Martin, L. aut Masbou, J. aut Massacret, N. aut McMichael, K. aut Mong, B. aut Murray, K. aut Nattress, J. aut Natzke, C. R. aut Ngwadla, X. E. aut Ondze, J. C. Nzobadila aut Odian, A. aut Orrell, J. L. aut Ortega, G. S. aut Overman, C. T. aut Parent, S. aut Perna, A. aut Piepke, A. aut Pletskova, N. aut Pratte, J. F. aut Radeka, V. aut Raguzin, E. aut Ramonnye, G. J. aut Rao, T. aut Rasiwala, H. aut Raymond, K. aut Rebeiro, B. M. aut Richardson, G. aut Ringuette, J. aut Riot, V. aut Rossignol, T. aut Rowson, P. C. aut Rudolph, L. aut Saldanha, R. aut Sangiorgio, S. aut Shang, X. aut Spadoni, F. aut Stekhanov, V. aut Sun, X. L. aut Tidball, A. aut Totev, T. aut Triambak, S. aut Tsang, R. H. M. aut Tyuka, O. A. aut Vachon, F. aut Vidal, M. aut Viel, S. aut Visser, G. aut Wagenpfeil, M. aut Walent, M. aut Wamba, K. aut Wang, Q. aut Wang, W. aut Wang, Y. aut Watts, M. aut Wei, W. aut Wen, L. J. aut Wichoski, U. aut Wilde, S. aut Worcester, M. aut Wu, W. H. aut Wu, X. aut Xie, L. aut Yan, W. aut Yang, H. aut Yang, L. aut Zeldovich, O. aut Zhao, J. aut Ziegler, T. aut Enthalten in The European physical journal Berlin : Springer, 1998 82(2022), 12 vom: 13. Dez. 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10.1140/epjc/s10052-022-11072-8 doi (DE-627)SPR049502352 (SPR)s10052-022-11072-8-e DE-627 ger DE-627 rakwb eng Gallina, G. verfasserin (orcid)0000-0002-9878-6499 aut Performance of novel VUV-sensitive Silicon Photo-Multipliers for nEXO 2022 Text txt rdacontent Computermedien c rdamedia Online-Ressource cr rdacarrier © The Author(s) 2022 Abstract Liquid xenon time projection chambers are promising detectors to search for neutrinoless double beta decay (0%$\nu \beta \beta %$), due to their response uniformity, monolithic sensitive volume, scalability to large target masses, and suitability for extremely low background operations. The nEXO collaboration has designed a tonne-scale time projection chamber that aims to search for 0%$\nu \beta \beta %$ of %$^{136}%$Xe with projected half-life sensitivity of %$1.35\times 10^{28}%$ yr. To reach this sensitivity, the design goal for nEXO is %$\le %$1% energy resolution at the decay Q-value (%$2458.07\pm 0.31%$ keV). Reaching this resolution requires the efficient collection of both the ionization and scintillation produced in the detector. The nEXO design employs Silicon Photo-Multipliers (SiPMs) to detect the vacuum ultra-violet, 175 nm scintillation light of liquid xenon. This paper reports on the characterization of the newest vacuum ultra-violet sensitive Fondazione Bruno Kessler VUVHD3 SiPMs specifically designed for nEXO, as well as new measurements on new test samples of previously characterised Hamamatsu VUV4 Multi Pixel Photon Counters (MPPCs). Various SiPM and MPPC parameters, such as dark noise, gain, direct crosstalk, correlated avalanches and photon detection efficiency were measured as a function of the applied over voltage and wavelength at liquid xenon temperature (163 K). The results from this study are used to provide updated estimates of the achievable energy resolution at the decay Q-value for the nEXO design. Guan, Y. aut Retiere, F. aut Cao, G. aut Bolotnikov, A. aut Kotov, I. aut Rescia, S. aut Soma, A. K. aut Tsang, T. aut Darroch, L. aut Brunner, T. aut Bolster, J. aut Cohen, J. R. aut Franco, T. Pinto aut Gillis, W. C. aut Smalley, H. Peltz aut Thibado, S. aut Pocar, A. aut Bhat, A. aut Jamil, A. aut Moore, D. C. aut Adhikari, G. aut Kharusi, S. Al aut Angelico, E. aut Arnquist, I. J. aut Arsenault, P. aut Badhrees, I. aut Bane, J. aut Belov, V. aut Bernard, E. P. aut Bhatta, T. aut Breur, P. A. aut Brodsky, J. P. aut Brown, E. aut Caden, E. aut Cao, L. aut Chambers, C. aut Chana, B. aut Charlebois, S. A. aut Chernyak, D. aut Chiu, M. aut Cleveland, B. aut Collister, R. aut Cvitan, M. aut Dalmasson, J. aut Daniels, T. aut Deslandes, K. aut DeVoe, R. aut di Vacri, M. L. aut Ding, Y. aut Dolinski, M. J. aut Dragone, A. aut Echevers, J. aut Eckert, B. aut Elbeltagi, M. aut Fabris, L. aut Fairbank, W. aut Farine, J. aut Fu, Y. S. aut Gallacher, D. aut Gautam, P. aut Giacomini, G. aut Gingras, C. aut Goeldi, D. aut Gornea, R. aut Gratta, G. aut Hardy, C. A. aut Hedges, S. aut Heffner, M. aut Hein, E. aut Holt, J. aut Hoppe, E. W. aut Hößl, J. aut House, A. aut Hunt, W. aut Iverson, A. aut Jiang, X. S. aut Karelin, A. aut Kaufman, L. J. aut Krücken, R. aut Kuchenkov, A. aut Kumar, K. S. aut Larson, A. aut Leach, K. G. aut Lenardo, B. G. aut Leonard, D. S. aut Lessard, G. aut Li, G. aut Li, S. aut Li, Z. aut Licciardi, C. aut Lindsay, R. aut MacLellan, R. aut Mahtab, M. aut Majidi, S. aut Malbrunot, C. aut Margetak, P. aut Martel-Dion, P. aut Martin, L. aut Masbou, J. aut Massacret, N. aut McMichael, K. aut Mong, B. aut Murray, K. aut Nattress, J. aut Natzke, C. R. aut Ngwadla, X. E. aut Ondze, J. C. Nzobadila aut Odian, A. aut Orrell, J. L. aut Ortega, G. S. aut Overman, C. T. aut Parent, S. aut Perna, A. aut Piepke, A. aut Pletskova, N. aut Pratte, J. F. aut Radeka, V. aut Raguzin, E. aut Ramonnye, G. J. aut Rao, T. aut Rasiwala, H. aut Raymond, K. aut Rebeiro, B. M. aut Richardson, G. aut Ringuette, J. aut Riot, V. aut Rossignol, T. aut Rowson, P. C. aut Rudolph, L. aut Saldanha, R. aut Sangiorgio, S. aut Shang, X. aut Spadoni, F. aut Stekhanov, V. aut Sun, X. L. aut Tidball, A. aut Totev, T. aut Triambak, S. aut Tsang, R. H. M. aut Tyuka, O. A. aut Vachon, F. aut Vidal, M. aut Viel, S. aut Visser, G. aut Wagenpfeil, M. aut Walent, M. aut Wamba, K. aut Wang, Q. aut Wang, W. aut Wang, Y. aut Watts, M. aut Wei, W. aut Wen, L. J. aut Wichoski, U. aut Wilde, S. aut Worcester, M. aut Wu, W. H. aut Wu, X. aut Xie, L. aut Yan, W. aut Yang, H. aut Yang, L. aut Zeldovich, O. aut Zhao, J. aut Ziegler, T. aut Enthalten in The European physical journal Berlin : Springer, 1998 82(2022), 12 vom: 13. Dez. (DE-627)253722934 (DE-600)1459069-4 1434-6052 nnns volume:82 year:2022 number:12 day:13 month:12 https://dx.doi.org/10.1140/epjc/s10052-022-11072-8 kostenfrei Volltext GBV_USEFLAG_A SYSFLAG_A GBV_SPRINGER GBV_ILN_11 GBV_ILN_20 GBV_ILN_22 GBV_ILN_23 GBV_ILN_24 GBV_ILN_31 GBV_ILN_39 GBV_ILN_40 GBV_ILN_60 GBV_ILN_62 GBV_ILN_63 GBV_ILN_69 GBV_ILN_70 GBV_ILN_73 GBV_ILN_95 GBV_ILN_105 GBV_ILN_110 GBV_ILN_150 GBV_ILN_151 GBV_ILN_161 GBV_ILN_170 GBV_ILN_206 GBV_ILN_213 GBV_ILN_230 GBV_ILN_267 GBV_ILN_285 GBV_ILN_293 GBV_ILN_370 GBV_ILN_602 GBV_ILN_702 GBV_ILN_2001 GBV_ILN_2003 GBV_ILN_2005 GBV_ILN_2006 GBV_ILN_2008 GBV_ILN_2009 GBV_ILN_2010 GBV_ILN_2011 GBV_ILN_2014 GBV_ILN_2015 GBV_ILN_2018 GBV_ILN_2020 GBV_ILN_2021 GBV_ILN_2025 GBV_ILN_2031 GBV_ILN_2038 GBV_ILN_2044 GBV_ILN_2048 GBV_ILN_2050 GBV_ILN_2055 GBV_ILN_2056 GBV_ILN_2057 GBV_ILN_2061 GBV_ILN_2108 GBV_ILN_2111 GBV_ILN_2113 GBV_ILN_2119 GBV_ILN_2190 GBV_ILN_4012 GBV_ILN_4037 GBV_ILN_4112 GBV_ILN_4125 GBV_ILN_4126 GBV_ILN_4246 GBV_ILN_4249 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_4335 GBV_ILN_4338 GBV_ILN_4367 GBV_ILN_4700 AR 82 2022 12 13 12 |
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Gallina, G. @@aut@@ Guan, Y. @@aut@@ Retiere, F. @@aut@@ Cao, G. @@aut@@ Bolotnikov, A. @@aut@@ Kotov, I. @@aut@@ Rescia, S. @@aut@@ Soma, A. K. @@aut@@ Tsang, T. @@aut@@ Darroch, L. @@aut@@ Brunner, T. @@aut@@ Bolster, J. @@aut@@ Cohen, J. R. @@aut@@ Franco, T. Pinto @@aut@@ Gillis, W. C. @@aut@@ Smalley, H. Peltz @@aut@@ Thibado, S. @@aut@@ Pocar, A. @@aut@@ Bhat, A. @@aut@@ Jamil, A. @@aut@@ Moore, D. C. @@aut@@ Adhikari, G. @@aut@@ Kharusi, S. Al @@aut@@ Angelico, E. @@aut@@ Arnquist, I. J. @@aut@@ Arsenault, P. @@aut@@ Badhrees, I. @@aut@@ Bane, J. @@aut@@ Belov, V. @@aut@@ Bernard, E. P. @@aut@@ Bhatta, T. @@aut@@ Breur, P. A. @@aut@@ Brodsky, J. P. @@aut@@ Brown, E. @@aut@@ Caden, E. @@aut@@ Cao, L. @@aut@@ Chambers, C. @@aut@@ Chana, B. @@aut@@ Charlebois, S. A. @@aut@@ Chernyak, D. @@aut@@ Chiu, M. @@aut@@ Cleveland, B. @@aut@@ Collister, R. @@aut@@ Cvitan, M. @@aut@@ Dalmasson, J. @@aut@@ Daniels, T. @@aut@@ Deslandes, K. @@aut@@ DeVoe, R. @@aut@@ di Vacri, M. L. @@aut@@ Ding, Y. @@aut@@ Dolinski, M. J. @@aut@@ Dragone, A. @@aut@@ Echevers, J. @@aut@@ Eckert, B. @@aut@@ Elbeltagi, M. @@aut@@ Fabris, L. @@aut@@ Fairbank, W. @@aut@@ Farine, J. @@aut@@ Fu, Y. S. @@aut@@ Gallacher, D. @@aut@@ Gautam, P. @@aut@@ Giacomini, G. @@aut@@ Gingras, C. @@aut@@ Goeldi, D. @@aut@@ Gornea, R. @@aut@@ Gratta, G. @@aut@@ Hardy, C. A. @@aut@@ Hedges, S. @@aut@@ Heffner, M. @@aut@@ Hein, E. @@aut@@ Holt, J. @@aut@@ Hoppe, E. W. @@aut@@ Hößl, J. @@aut@@ House, A. @@aut@@ Hunt, W. @@aut@@ Iverson, A. @@aut@@ Jiang, X. S. @@aut@@ Karelin, A. @@aut@@ Kaufman, L. J. @@aut@@ Krücken, R. @@aut@@ Kuchenkov, A. @@aut@@ Kumar, K. S. @@aut@@ Larson, A. @@aut@@ Leach, K. G. @@aut@@ Lenardo, B. G. @@aut@@ Leonard, D. S. @@aut@@ Lessard, G. @@aut@@ Li, G. @@aut@@ Li, S. @@aut@@ Li, Z. @@aut@@ Licciardi, C. @@aut@@ Lindsay, R. @@aut@@ MacLellan, R. @@aut@@ Mahtab, M. @@aut@@ Majidi, S. @@aut@@ Malbrunot, C. @@aut@@ Margetak, P. @@aut@@ Martel-Dion, P. @@aut@@ Martin, L. @@aut@@ Masbou, J. @@aut@@ Massacret, N. @@aut@@ McMichael, K. @@aut@@ Mong, B. @@aut@@ Murray, K. @@aut@@ Nattress, J. @@aut@@ Natzke, C. R. @@aut@@ Ngwadla, X. E. @@aut@@ Ondze, J. C. Nzobadila @@aut@@ Odian, A. @@aut@@ Orrell, J. L. @@aut@@ Ortega, G. S. @@aut@@ Overman, C. T. @@aut@@ Parent, S. @@aut@@ Perna, A. @@aut@@ Piepke, A. @@aut@@ Pletskova, N. @@aut@@ Pratte, J. F. @@aut@@ Radeka, V. @@aut@@ Raguzin, E. @@aut@@ Ramonnye, G. J. @@aut@@ Rao, T. @@aut@@ Rasiwala, H. @@aut@@ Raymond, K. @@aut@@ Rebeiro, B. M. @@aut@@ Richardson, G. @@aut@@ Ringuette, J. @@aut@@ Riot, V. @@aut@@ Rossignol, T. @@aut@@ Rowson, P. C. @@aut@@ Rudolph, L. @@aut@@ Saldanha, R. @@aut@@ Sangiorgio, S. @@aut@@ Shang, X. @@aut@@ Spadoni, F. @@aut@@ Stekhanov, V. @@aut@@ Sun, X. L. @@aut@@ Tidball, A. @@aut@@ Totev, T. @@aut@@ Triambak, S. @@aut@@ Tsang, R. H. M. @@aut@@ Tyuka, O. A. @@aut@@ Vachon, F. @@aut@@ Vidal, M. @@aut@@ Viel, S. @@aut@@ Visser, G. @@aut@@ Wagenpfeil, M. @@aut@@ Walent, M. @@aut@@ Wamba, K. @@aut@@ Wang, Q. @@aut@@ Wang, W. @@aut@@ Wang, Y. @@aut@@ Watts, M. @@aut@@ Wei, W. @@aut@@ Wen, L. J. @@aut@@ Wichoski, U. @@aut@@ Wilde, S. @@aut@@ Worcester, M. @@aut@@ Wu, W. H. @@aut@@ Wu, X. @@aut@@ Xie, L. @@aut@@ Yan, W. @@aut@@ Yang, H. @@aut@@ Yang, L. @@aut@@ Zeldovich, O. @@aut@@ Zhao, J. @@aut@@ Ziegler, T. @@aut@@ |
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Gallina, G. Performance of novel VUV-sensitive Silicon Photo-Multipliers for nEXO |
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Performance of novel VUV-sensitive Silicon Photo-Multipliers for nEXO |
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Gallina, G. Guan, Y. Retiere, F. Cao, G. Bolotnikov, A. Kotov, I. Rescia, S. Soma, A. K. Tsang, T. Darroch, L. Brunner, T. Bolster, J. Cohen, J. R. Franco, T. Pinto Gillis, W. C. Smalley, H. Peltz Thibado, S. Pocar, A. Bhat, A. Jamil, A. Moore, D. C. Adhikari, G. Kharusi, S. Al Angelico, E. Arnquist, I. J. Arsenault, P. Badhrees, I. Bane, J. Belov, V. Bernard, E. P. Bhatta, T. Breur, P. A. Brodsky, J. P. Brown, E. Caden, E. Cao, L. Chambers, C. Chana, B. Charlebois, S. A. Chernyak, D. Chiu, M. Cleveland, B. Collister, R. Cvitan, M. Dalmasson, J. Daniels, T. Deslandes, K. DeVoe, R. di Vacri, M. L. Ding, Y. Dolinski, M. J. Dragone, A. Echevers, J. Eckert, B. Elbeltagi, M. Fabris, L. Fairbank, W. Farine, J. Fu, Y. S. Gallacher, D. Gautam, P. Giacomini, G. Gingras, C. Goeldi, D. Gornea, R. Gratta, G. Hardy, C. A. Hedges, S. Heffner, M. Hein, E. Holt, J. Hoppe, E. W. Hößl, J. House, A. Hunt, W. Iverson, A. Jiang, X. S. Karelin, A. Kaufman, L. J. Krücken, R. Kuchenkov, A. Kumar, K. S. Larson, A. Leach, K. G. Lenardo, B. G. Leonard, D. S. Lessard, G. Li, G. Li, S. Li, Z. Licciardi, C. Lindsay, R. MacLellan, R. Mahtab, M. Majidi, S. Malbrunot, C. Margetak, P. Martel-Dion, P. Martin, L. Masbou, J. Massacret, N. McMichael, K. Mong, B. Murray, K. Nattress, J. Natzke, C. R. Ngwadla, X. E. Ondze, J. C. Nzobadila Odian, A. Orrell, J. L. Ortega, G. S. Overman, C. T. Parent, S. Perna, A. Piepke, A. Pletskova, N. Pratte, J. F. Radeka, V. Raguzin, E. Ramonnye, G. J. Rao, T. Rasiwala, H. Raymond, K. Rebeiro, B. M. Richardson, G. Ringuette, J. Riot, V. Rossignol, T. Rowson, P. C. Rudolph, L. Saldanha, R. Sangiorgio, S. Shang, X. Spadoni, F. Stekhanov, V. Sun, X. L. Tidball, A. Totev, T. Triambak, S. Tsang, R. H. M. Tyuka, O. A. Vachon, F. Vidal, M. Viel, S. Visser, G. Wagenpfeil, M. Walent, M. Wamba, K. Wang, Q. Wang, W. Wang, Y. Watts, M. Wei, W. Wen, L. J. Wichoski, U. Wilde, S. Worcester, M. Wu, W. H. Wu, X. Xie, L. Yan, W. Yang, H. Yang, L. Zeldovich, O. Zhao, J. Ziegler, T. |
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performance of novel vuv-sensitive silicon photo-multipliers for nexo |
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Performance of novel VUV-sensitive Silicon Photo-Multipliers for nEXO |
| abstract |
Abstract Liquid xenon time projection chambers are promising detectors to search for neutrinoless double beta decay (0%$\nu \beta \beta %$), due to their response uniformity, monolithic sensitive volume, scalability to large target masses, and suitability for extremely low background operations. The nEXO collaboration has designed a tonne-scale time projection chamber that aims to search for 0%$\nu \beta \beta %$ of %$^{136}%$Xe with projected half-life sensitivity of %$1.35\times 10^{28}%$ yr. To reach this sensitivity, the design goal for nEXO is %$\le %$1% energy resolution at the decay Q-value (%$2458.07\pm 0.31%$ keV). Reaching this resolution requires the efficient collection of both the ionization and scintillation produced in the detector. The nEXO design employs Silicon Photo-Multipliers (SiPMs) to detect the vacuum ultra-violet, 175 nm scintillation light of liquid xenon. This paper reports on the characterization of the newest vacuum ultra-violet sensitive Fondazione Bruno Kessler VUVHD3 SiPMs specifically designed for nEXO, as well as new measurements on new test samples of previously characterised Hamamatsu VUV4 Multi Pixel Photon Counters (MPPCs). Various SiPM and MPPC parameters, such as dark noise, gain, direct crosstalk, correlated avalanches and photon detection efficiency were measured as a function of the applied over voltage and wavelength at liquid xenon temperature (163 K). The results from this study are used to provide updated estimates of the achievable energy resolution at the decay Q-value for the nEXO design. © The Author(s) 2022 |
| abstractGer |
Abstract Liquid xenon time projection chambers are promising detectors to search for neutrinoless double beta decay (0%$\nu \beta \beta %$), due to their response uniformity, monolithic sensitive volume, scalability to large target masses, and suitability for extremely low background operations. The nEXO collaboration has designed a tonne-scale time projection chamber that aims to search for 0%$\nu \beta \beta %$ of %$^{136}%$Xe with projected half-life sensitivity of %$1.35\times 10^{28}%$ yr. To reach this sensitivity, the design goal for nEXO is %$\le %$1% energy resolution at the decay Q-value (%$2458.07\pm 0.31%$ keV). Reaching this resolution requires the efficient collection of both the ionization and scintillation produced in the detector. The nEXO design employs Silicon Photo-Multipliers (SiPMs) to detect the vacuum ultra-violet, 175 nm scintillation light of liquid xenon. This paper reports on the characterization of the newest vacuum ultra-violet sensitive Fondazione Bruno Kessler VUVHD3 SiPMs specifically designed for nEXO, as well as new measurements on new test samples of previously characterised Hamamatsu VUV4 Multi Pixel Photon Counters (MPPCs). Various SiPM and MPPC parameters, such as dark noise, gain, direct crosstalk, correlated avalanches and photon detection efficiency were measured as a function of the applied over voltage and wavelength at liquid xenon temperature (163 K). The results from this study are used to provide updated estimates of the achievable energy resolution at the decay Q-value for the nEXO design. © The Author(s) 2022 |
| abstract_unstemmed |
Abstract Liquid xenon time projection chambers are promising detectors to search for neutrinoless double beta decay (0%$\nu \beta \beta %$), due to their response uniformity, monolithic sensitive volume, scalability to large target masses, and suitability for extremely low background operations. The nEXO collaboration has designed a tonne-scale time projection chamber that aims to search for 0%$\nu \beta \beta %$ of %$^{136}%$Xe with projected half-life sensitivity of %$1.35\times 10^{28}%$ yr. To reach this sensitivity, the design goal for nEXO is %$\le %$1% energy resolution at the decay Q-value (%$2458.07\pm 0.31%$ keV). Reaching this resolution requires the efficient collection of both the ionization and scintillation produced in the detector. The nEXO design employs Silicon Photo-Multipliers (SiPMs) to detect the vacuum ultra-violet, 175 nm scintillation light of liquid xenon. This paper reports on the characterization of the newest vacuum ultra-violet sensitive Fondazione Bruno Kessler VUVHD3 SiPMs specifically designed for nEXO, as well as new measurements on new test samples of previously characterised Hamamatsu VUV4 Multi Pixel Photon Counters (MPPCs). Various SiPM and MPPC parameters, such as dark noise, gain, direct crosstalk, correlated avalanches and photon detection efficiency were measured as a function of the applied over voltage and wavelength at liquid xenon temperature (163 K). The results from this study are used to provide updated estimates of the achievable energy resolution at the decay Q-value for the nEXO design. © The Author(s) 2022 |
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<?xml version="1.0" encoding="UTF-8"?><collection xmlns="http://www.loc.gov/MARC21/slim"><record><leader>01000naa a22002652 4500</leader><controlfield tag="001">SPR049502352</controlfield><controlfield tag="003">DE-627</controlfield><controlfield tag="005">20230301064728.0</controlfield><controlfield tag="007">cr uuu---uuuuu</controlfield><controlfield tag="008">230301s2022 xx |||||o 00| ||eng c</controlfield><datafield tag="024" ind1="7" ind2=" "><subfield code="a">10.1140/epjc/s10052-022-11072-8</subfield><subfield code="2">doi</subfield></datafield><datafield tag="035" ind1=" " ind2=" "><subfield code="a">(DE-627)SPR049502352</subfield></datafield><datafield tag="035" ind1=" " ind2=" "><subfield code="a">(SPR)s10052-022-11072-8-e</subfield></datafield><datafield tag="040" ind1=" " ind2=" "><subfield code="a">DE-627</subfield><subfield code="b">ger</subfield><subfield code="c">DE-627</subfield><subfield code="e">rakwb</subfield></datafield><datafield tag="041" ind1=" " ind2=" "><subfield code="a">eng</subfield></datafield><datafield tag="100" ind1="1" ind2=" "><subfield code="a">Gallina, G.</subfield><subfield code="e">verfasserin</subfield><subfield code="0">(orcid)0000-0002-9878-6499</subfield><subfield code="4">aut</subfield></datafield><datafield tag="245" ind1="1" ind2="0"><subfield code="a">Performance of novel VUV-sensitive Silicon Photo-Multipliers for nEXO</subfield></datafield><datafield tag="264" ind1=" " ind2="1"><subfield code="c">2022</subfield></datafield><datafield tag="336" ind1=" " ind2=" "><subfield code="a">Text</subfield><subfield code="b">txt</subfield><subfield code="2">rdacontent</subfield></datafield><datafield tag="337" ind1=" " ind2=" "><subfield code="a">Computermedien</subfield><subfield code="b">c</subfield><subfield code="2">rdamedia</subfield></datafield><datafield tag="338" ind1=" " ind2=" "><subfield code="a">Online-Ressource</subfield><subfield code="b">cr</subfield><subfield code="2">rdacarrier</subfield></datafield><datafield tag="500" ind1=" " ind2=" "><subfield code="a">© The Author(s) 2022</subfield></datafield><datafield tag="520" ind1=" " ind2=" "><subfield code="a">Abstract Liquid xenon time projection chambers are promising detectors to search for neutrinoless double beta decay (0%$\nu \beta \beta %$), due to their response uniformity, monolithic sensitive volume, scalability to large target masses, and suitability for extremely low background operations. The nEXO collaboration has designed a tonne-scale time projection chamber that aims to search for 0%$\nu \beta \beta %$ of %$^{136}%$Xe with projected half-life sensitivity of %$1.35\times 10^{28}%$ yr. To reach this sensitivity, the design goal for nEXO is %$\le %$1% energy resolution at the decay Q-value (%$2458.07\pm 0.31%$ keV). Reaching this resolution requires the efficient collection of both the ionization and scintillation produced in the detector. The nEXO design employs Silicon Photo-Multipliers (SiPMs) to detect the vacuum ultra-violet, 175 nm scintillation light of liquid xenon. This paper reports on the characterization of the newest vacuum ultra-violet sensitive Fondazione Bruno Kessler VUVHD3 SiPMs specifically designed for nEXO, as well as new measurements on new test samples of previously characterised Hamamatsu VUV4 Multi Pixel Photon Counters (MPPCs). Various SiPM and MPPC parameters, such as dark noise, gain, direct crosstalk, correlated avalanches and photon detection efficiency were measured as a function of the applied over voltage and wavelength at liquid xenon temperature (163 K). The results from this study are used to provide updated estimates of the achievable energy resolution at the decay Q-value for the nEXO design.</subfield></datafield><datafield tag="700" ind1="1" ind2=" "><subfield code="a">Guan, Y.</subfield><subfield code="4">aut</subfield></datafield><datafield tag="700" ind1="1" ind2=" "><subfield code="a">Retiere, F.</subfield><subfield code="4">aut</subfield></datafield><datafield tag="700" ind1="1" ind2=" "><subfield code="a">Cao, G.</subfield><subfield code="4">aut</subfield></datafield><datafield tag="700" ind1="1" ind2=" "><subfield code="a">Bolotnikov, A.</subfield><subfield code="4">aut</subfield></datafield><datafield tag="700" ind1="1" ind2=" "><subfield code="a">Kotov, I.</subfield><subfield code="4">aut</subfield></datafield><datafield tag="700" ind1="1" ind2=" "><subfield code="a">Rescia, S.</subfield><subfield code="4">aut</subfield></datafield><datafield tag="700" ind1="1" ind2=" "><subfield code="a">Soma, A. 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| score |
7.400667 |