SuperFGD prototype time resolution studies
The SuperFGD will be a part of the ND280 near detector of the T2K and Hyper Kamiokande projects, that will help to reduce systematic uncertainties related with neutrino flux and cross-section modeling. The upgraded ND280 will be able to perform a full exclusive reconstruction of the final state from...
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creator | Alekseev, I Arihara, T Baranov, V Bartoszek, L Bernardi, L Blondel, A Boikov, A V Buizza-Avanzini, M Cadoux, F Capó, J Cayo, J Chakrani, J Chong, P S Chvirova, A Danilov, M Davydov, Yu I Dergacheva, A Dokania, N Douqa, D Drapier, O Eguchi, A Favre, Y Fedorova, D Fedotov, S Fujii, Y Gastaldi, F Gendotti, A Glagolev, V Guillaumat, R Iwamoto, K Jakkapu, M Jesús-Valls, C Jung, C K Kakuno, H Kasetti, S P Khabibullin, M Khotjantsev, A Kikutani, H Kobayashi, T Kodama, S Korzenev, A Kose, U Kudenko, Y Kutter, T Last, D B Li Z Li Lin, L S Lin, S Louzir, M Lux, T Maret, L Martynenko, S Matsubara, T Mauger, C McGrew, C Mefodiev, A Mineev, O Nakadaira, T Nakagiri, K Nanni, J Nicola, L Noah, E Paolone, V Parsa, S Pellegrino, R Ramirez, M A Reh, M Ricco, C Rubbia, A Sakashita, K Sanchez, F Sgalaberna, D Shvartsman, A Skrobova, N Suslov, I A Suvorov, S Svirida, D Teklu, A Tereshchenko, V V Tzanov, M Vasilyev, I I Wood, K Yang, G Yershov, N Yokoyama, M Yoshimoto, Y Zhao, X Zilberman, P Zimmerman, E D |
description | The SuperFGD will be a part of the ND280 near detector of the T2K and Hyper Kamiokande projects, that will help to reduce systematic uncertainties related with neutrino flux and cross-section modeling. The upgraded ND280 will be able to perform a full exclusive reconstruction of the final state from neutrino-nucleus interactions, including measurements of low momentum protons, pions and, for the first time, event-by event measurements of neutron kinematics. The time resolution defines the neutron energy resolution. We present the results of time resolution measurements made with the SuperFGD prototype that consists of 9216 plastic scintillator cubes (cube size is 1 cm\(^3\)) readout with 1728 wavelength-shifting fibers going along three orthogonal directions. We use data from the muon beam exposure at CERN. The time resolution of 0.97 ns was obtained for one readout channel after implementing the time calibration with a correction for the time-walk effect. The time resolution improves with energy deposited in a scintillator cube. Averaging two readout channels for one scintillator cube improves the time resolution to 0.68 ns which means that signals in different channels are not synchronous. Therefore the contribution from the time recording step of 2.5 ns is averaged as well. Averaging time values from N channels improves the time resolution by \(\sim 1/\sqrt{N}\). Therefore a very good time resolution should be achievable for neutrons since neutron recoils hit typically several scintillator cubes and in addition produce larger amplitudes than muons. Measurements performed with a laser and a wide-bandwidth oscilloscope demonstrated that the time resolution obtained with the muon beam is not far from its expected limit. The intrinsic time resolution of one channel is 0.67 ns for signals of 56 photo-electron typical for minimum ionizing particles. |
doi_str_mv | 10.48550/arxiv.2206.10507 |
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The upgraded ND280 will be able to perform a full exclusive reconstruction of the final state from neutrino-nucleus interactions, including measurements of low momentum protons, pions and, for the first time, event-by event measurements of neutron kinematics. The time resolution defines the neutron energy resolution. We present the results of time resolution measurements made with the SuperFGD prototype that consists of 9216 plastic scintillator cubes (cube size is 1 cm\(^3\)) readout with 1728 wavelength-shifting fibers going along three orthogonal directions. We use data from the muon beam exposure at CERN. The time resolution of 0.97 ns was obtained for one readout channel after implementing the time calibration with a correction for the time-walk effect. The time resolution improves with energy deposited in a scintillator cube. Averaging two readout channels for one scintillator cube improves the time resolution to 0.68 ns which means that signals in different channels are not synchronous. Therefore the contribution from the time recording step of 2.5 ns is averaged as well. Averaging time values from N channels improves the time resolution by \(\sim 1/\sqrt{N}\). Therefore a very good time resolution should be achievable for neutrons since neutron recoils hit typically several scintillator cubes and in addition produce larger amplitudes than muons. Measurements performed with a laser and a wide-bandwidth oscilloscope demonstrated that the time resolution obtained with the muon beam is not far from its expected limit. The intrinsic time resolution of one channel is 0.67 ns for signals of 56 photo-electron typical for minimum ionizing particles.</description><identifier>EISSN: 2331-8422</identifier><identifier>DOI: 10.48550/arxiv.2206.10507</identifier><language>eng</language><publisher>Ithaca: Cornell University Library, arXiv.org</publisher><subject>Channels ; Cubes ; Energy resolution ; Kinematics ; Muons ; Neutrinos ; Particle beams ; Particle physics ; Physics - Instrumentation and Detectors ; Pions ; Prototypes ; Scintillation counters ; Time measurement</subject><ispartof>arXiv.org, 2023-01</ispartof><rights>2023. This work is published under http://arxiv.org/licenses/nonexclusive-distrib/1.0/ (the “License”). Notwithstanding the ProQuest Terms and Conditions, you may use this content in accordance with the terms of the License.</rights><rights>http://arxiv.org/licenses/nonexclusive-distrib/1.0</rights><oa>free_for_read</oa><woscitedreferencessubscribed>false</woscitedreferencessubscribed></display><links><openurl>$$Topenurl_article</openurl><openurlfulltext>$$Topenurlfull_article</openurlfulltext><thumbnail>$$Tsyndetics_thumb_exl</thumbnail><link.rule.ids>228,230,776,780,881,27902</link.rule.ids><backlink>$$Uhttps://doi.org/10.48550/arXiv.2206.10507$$DView paper in arXiv$$Hfree_for_read</backlink><backlink>$$Uhttps://doi.org/10.1088/1748-0221/18/01/P01012$$DView published paper (Access to full text may be restricted)$$Hfree_for_read</backlink></links><search><creatorcontrib>Alekseev, I</creatorcontrib><creatorcontrib>Arihara, T</creatorcontrib><creatorcontrib>Baranov, V</creatorcontrib><creatorcontrib>Bartoszek, L</creatorcontrib><creatorcontrib>Bernardi, L</creatorcontrib><creatorcontrib>Blondel, A</creatorcontrib><creatorcontrib>Boikov, A V</creatorcontrib><creatorcontrib>Buizza-Avanzini, M</creatorcontrib><creatorcontrib>Cadoux, F</creatorcontrib><creatorcontrib>Capó, J</creatorcontrib><creatorcontrib>Cayo, J</creatorcontrib><creatorcontrib>Chakrani, J</creatorcontrib><creatorcontrib>Chong, P S</creatorcontrib><creatorcontrib>Chvirova, A</creatorcontrib><creatorcontrib>Danilov, M</creatorcontrib><creatorcontrib>Davydov, Yu I</creatorcontrib><creatorcontrib>Dergacheva, A</creatorcontrib><creatorcontrib>Dokania, N</creatorcontrib><creatorcontrib>Douqa, D</creatorcontrib><creatorcontrib>Drapier, O</creatorcontrib><creatorcontrib>Eguchi, A</creatorcontrib><creatorcontrib>Favre, Y</creatorcontrib><creatorcontrib>Fedorova, D</creatorcontrib><creatorcontrib>Fedotov, S</creatorcontrib><creatorcontrib>Fujii, Y</creatorcontrib><creatorcontrib>Gastaldi, F</creatorcontrib><creatorcontrib>Gendotti, A</creatorcontrib><creatorcontrib>Glagolev, V</creatorcontrib><creatorcontrib>Guillaumat, R</creatorcontrib><creatorcontrib>Iwamoto, K</creatorcontrib><creatorcontrib>Jakkapu, M</creatorcontrib><creatorcontrib>Jesús-Valls, C</creatorcontrib><creatorcontrib>Jung, C K</creatorcontrib><creatorcontrib>Kakuno, H</creatorcontrib><creatorcontrib>Kasetti, S P</creatorcontrib><creatorcontrib>Khabibullin, M</creatorcontrib><creatorcontrib>Khotjantsev, A</creatorcontrib><creatorcontrib>Kikutani, H</creatorcontrib><creatorcontrib>Kobayashi, T</creatorcontrib><creatorcontrib>Kodama, S</creatorcontrib><creatorcontrib>Korzenev, A</creatorcontrib><creatorcontrib>Kose, U</creatorcontrib><creatorcontrib>Kudenko, Y</creatorcontrib><creatorcontrib>Kutter, T</creatorcontrib><creatorcontrib>Last, D</creatorcontrib><creatorcontrib>B Li</creatorcontrib><creatorcontrib>Z Li</creatorcontrib><creatorcontrib>Lin, L S</creatorcontrib><creatorcontrib>Lin, S</creatorcontrib><creatorcontrib>Louzir, M</creatorcontrib><creatorcontrib>Lux, T</creatorcontrib><creatorcontrib>Maret, L</creatorcontrib><creatorcontrib>Martynenko, S</creatorcontrib><creatorcontrib>Matsubara, T</creatorcontrib><creatorcontrib>Mauger, C</creatorcontrib><creatorcontrib>McGrew, C</creatorcontrib><creatorcontrib>Mefodiev, A</creatorcontrib><creatorcontrib>Mineev, O</creatorcontrib><creatorcontrib>Nakadaira, T</creatorcontrib><creatorcontrib>Nakagiri, K</creatorcontrib><creatorcontrib>Nanni, J</creatorcontrib><creatorcontrib>Nicola, L</creatorcontrib><creatorcontrib>Noah, E</creatorcontrib><creatorcontrib>Paolone, V</creatorcontrib><creatorcontrib>Parsa, S</creatorcontrib><creatorcontrib>Pellegrino, R</creatorcontrib><creatorcontrib>Ramirez, M A</creatorcontrib><creatorcontrib>Reh, M</creatorcontrib><creatorcontrib>Ricco, C</creatorcontrib><creatorcontrib>Rubbia, A</creatorcontrib><creatorcontrib>Sakashita, K</creatorcontrib><creatorcontrib>Sanchez, F</creatorcontrib><creatorcontrib>Sgalaberna, D</creatorcontrib><creatorcontrib>Shvartsman, A</creatorcontrib><creatorcontrib>Skrobova, N</creatorcontrib><creatorcontrib>Suslov, I A</creatorcontrib><creatorcontrib>Suvorov, S</creatorcontrib><creatorcontrib>Svirida, D</creatorcontrib><creatorcontrib>Teklu, A</creatorcontrib><creatorcontrib>Tereshchenko, V V</creatorcontrib><creatorcontrib>Tzanov, M</creatorcontrib><creatorcontrib>Vasilyev, I I</creatorcontrib><creatorcontrib>Wood, K</creatorcontrib><creatorcontrib>Yang, G</creatorcontrib><creatorcontrib>Yershov, N</creatorcontrib><creatorcontrib>Yokoyama, M</creatorcontrib><creatorcontrib>Yoshimoto, Y</creatorcontrib><creatorcontrib>Zhao, X</creatorcontrib><creatorcontrib>Zilberman, P</creatorcontrib><creatorcontrib>Zimmerman, E D</creatorcontrib><title>SuperFGD prototype time resolution studies</title><title>arXiv.org</title><description>The SuperFGD will be a part of the ND280 near detector of the T2K and Hyper Kamiokande projects, that will help to reduce systematic uncertainties related with neutrino flux and cross-section modeling. The upgraded ND280 will be able to perform a full exclusive reconstruction of the final state from neutrino-nucleus interactions, including measurements of low momentum protons, pions and, for the first time, event-by event measurements of neutron kinematics. The time resolution defines the neutron energy resolution. We present the results of time resolution measurements made with the SuperFGD prototype that consists of 9216 plastic scintillator cubes (cube size is 1 cm\(^3\)) readout with 1728 wavelength-shifting fibers going along three orthogonal directions. We use data from the muon beam exposure at CERN. The time resolution of 0.97 ns was obtained for one readout channel after implementing the time calibration with a correction for the time-walk effect. The time resolution improves with energy deposited in a scintillator cube. Averaging two readout channels for one scintillator cube improves the time resolution to 0.68 ns which means that signals in different channels are not synchronous. Therefore the contribution from the time recording step of 2.5 ns is averaged as well. Averaging time values from N channels improves the time resolution by \(\sim 1/\sqrt{N}\). Therefore a very good time resolution should be achievable for neutrons since neutron recoils hit typically several scintillator cubes and in addition produce larger amplitudes than muons. Measurements performed with a laser and a wide-bandwidth oscilloscope demonstrated that the time resolution obtained with the muon beam is not far from its expected limit. The intrinsic time resolution of one channel is 0.67 ns for signals of 56 photo-electron typical for minimum ionizing particles.</description><subject>Channels</subject><subject>Cubes</subject><subject>Energy resolution</subject><subject>Kinematics</subject><subject>Muons</subject><subject>Neutrinos</subject><subject>Particle beams</subject><subject>Particle physics</subject><subject>Physics - Instrumentation and Detectors</subject><subject>Pions</subject><subject>Prototypes</subject><subject>Scintillation counters</subject><subject>Time 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M</creator><creator>Vasilyev, I I</creator><creator>Wood, K</creator><creator>Yang, G</creator><creator>Yershov, N</creator><creator>Yokoyama, M</creator><creator>Yoshimoto, Y</creator><creator>Zhao, X</creator><creator>Zilberman, P</creator><creator>Zimmerman, E D</creator><general>Cornell University Library, arXiv.org</general><scope>8FE</scope><scope>8FG</scope><scope>ABJCF</scope><scope>ABUWG</scope><scope>AFKRA</scope><scope>AZQEC</scope><scope>BENPR</scope><scope>BGLVJ</scope><scope>CCPQU</scope><scope>DWQXO</scope><scope>HCIFZ</scope><scope>L6V</scope><scope>M7S</scope><scope>PIMPY</scope><scope>PQEST</scope><scope>PQQKQ</scope><scope>PQUKI</scope><scope>PRINS</scope><scope>PTHSS</scope><scope>GOX</scope></search><sort><creationdate>20230118</creationdate><title>SuperFGD prototype time resolution studies</title><author>Alekseev, I ; Arihara, T ; Baranov, V ; Bartoszek, L ; Bernardi, L ; Blondel, A ; Boikov, A V ; Buizza-Avanzini, M ; Cadoux, F ; Capó, J ; Cayo, J ; Chakrani, J ; Chong, P S ; Chvirova, A ; Danilov, M ; Davydov, Yu I ; Dergacheva, A ; Dokania, N ; Douqa, D ; Drapier, O ; Eguchi, A ; Favre, Y ; Fedorova, D ; Fedotov, S ; Fujii, Y ; Gastaldi, F ; Gendotti, A ; Glagolev, V ; Guillaumat, R ; Iwamoto, K ; Jakkapu, M ; Jesús-Valls, C ; Jung, C K ; Kakuno, H ; Kasetti, S P ; Khabibullin, M ; Khotjantsev, A ; Kikutani, H ; Kobayashi, T ; Kodama, S ; Korzenev, A ; Kose, U ; Kudenko, Y ; Kutter, T ; Last, D ; B Li ; Z Li ; Lin, L S ; Lin, S ; Louzir, M ; Lux, T ; Maret, L ; Martynenko, S ; Matsubara, T ; Mauger, C ; McGrew, C ; Mefodiev, A ; Mineev, O ; Nakadaira, T ; Nakagiri, K ; Nanni, J ; Nicola, L ; Noah, E ; Paolone, V ; Parsa, S ; Pellegrino, R ; Ramirez, M A ; Reh, M ; Ricco, C ; Rubbia, A ; Sakashita, K ; Sanchez, F ; Sgalaberna, D ; Shvartsman, A ; Skrobova, N ; Suslov, I A ; Suvorov, S ; Svirida, D ; Teklu, A ; Tereshchenko, V V ; Tzanov, M ; Vasilyev, I I ; Wood, K ; Yang, G ; Yershov, N ; Yokoyama, M ; Yoshimoto, Y ; Zhao, X ; Zilberman, P ; Zimmerman, E D</author></sort><facets><frbrtype>5</frbrtype><frbrgroupid>cdi_FETCH-LOGICAL-a524-38265ff0e29827bfc65e4a4a8a655d7f1945f3388f236e41344dce603ae1b8a73</frbrgroupid><rsrctype>articles</rsrctype><prefilter>articles</prefilter><language>eng</language><creationdate>2023</creationdate><topic>Channels</topic><topic>Cubes</topic><topic>Energy resolution</topic><topic>Kinematics</topic><topic>Muons</topic><topic>Neutrinos</topic><topic>Particle beams</topic><topic>Particle physics</topic><topic>Physics - Instrumentation and Detectors</topic><topic>Pions</topic><topic>Prototypes</topic><topic>Scintillation counters</topic><topic>Time measurement</topic><toplevel>online_resources</toplevel><creatorcontrib>Alekseev, I</creatorcontrib><creatorcontrib>Arihara, T</creatorcontrib><creatorcontrib>Baranov, V</creatorcontrib><creatorcontrib>Bartoszek, L</creatorcontrib><creatorcontrib>Bernardi, L</creatorcontrib><creatorcontrib>Blondel, A</creatorcontrib><creatorcontrib>Boikov, A V</creatorcontrib><creatorcontrib>Buizza-Avanzini, M</creatorcontrib><creatorcontrib>Cadoux, F</creatorcontrib><creatorcontrib>Capó, J</creatorcontrib><creatorcontrib>Cayo, J</creatorcontrib><creatorcontrib>Chakrani, J</creatorcontrib><creatorcontrib>Chong, P S</creatorcontrib><creatorcontrib>Chvirova, A</creatorcontrib><creatorcontrib>Danilov, M</creatorcontrib><creatorcontrib>Davydov, Yu I</creatorcontrib><creatorcontrib>Dergacheva, A</creatorcontrib><creatorcontrib>Dokania, N</creatorcontrib><creatorcontrib>Douqa, D</creatorcontrib><creatorcontrib>Drapier, O</creatorcontrib><creatorcontrib>Eguchi, A</creatorcontrib><creatorcontrib>Favre, Y</creatorcontrib><creatorcontrib>Fedorova, D</creatorcontrib><creatorcontrib>Fedotov, S</creatorcontrib><creatorcontrib>Fujii, Y</creatorcontrib><creatorcontrib>Gastaldi, F</creatorcontrib><creatorcontrib>Gendotti, A</creatorcontrib><creatorcontrib>Glagolev, V</creatorcontrib><creatorcontrib>Guillaumat, R</creatorcontrib><creatorcontrib>Iwamoto, K</creatorcontrib><creatorcontrib>Jakkapu, M</creatorcontrib><creatorcontrib>Jesús-Valls, C</creatorcontrib><creatorcontrib>Jung, C K</creatorcontrib><creatorcontrib>Kakuno, H</creatorcontrib><creatorcontrib>Kasetti, S P</creatorcontrib><creatorcontrib>Khabibullin, M</creatorcontrib><creatorcontrib>Khotjantsev, A</creatorcontrib><creatorcontrib>Kikutani, H</creatorcontrib><creatorcontrib>Kobayashi, T</creatorcontrib><creatorcontrib>Kodama, S</creatorcontrib><creatorcontrib>Korzenev, A</creatorcontrib><creatorcontrib>Kose, U</creatorcontrib><creatorcontrib>Kudenko, Y</creatorcontrib><creatorcontrib>Kutter, T</creatorcontrib><creatorcontrib>Last, D</creatorcontrib><creatorcontrib>B Li</creatorcontrib><creatorcontrib>Z Li</creatorcontrib><creatorcontrib>Lin, L S</creatorcontrib><creatorcontrib>Lin, S</creatorcontrib><creatorcontrib>Louzir, M</creatorcontrib><creatorcontrib>Lux, T</creatorcontrib><creatorcontrib>Maret, L</creatorcontrib><creatorcontrib>Martynenko, S</creatorcontrib><creatorcontrib>Matsubara, T</creatorcontrib><creatorcontrib>Mauger, C</creatorcontrib><creatorcontrib>McGrew, C</creatorcontrib><creatorcontrib>Mefodiev, A</creatorcontrib><creatorcontrib>Mineev, O</creatorcontrib><creatorcontrib>Nakadaira, T</creatorcontrib><creatorcontrib>Nakagiri, K</creatorcontrib><creatorcontrib>Nanni, J</creatorcontrib><creatorcontrib>Nicola, L</creatorcontrib><creatorcontrib>Noah, E</creatorcontrib><creatorcontrib>Paolone, V</creatorcontrib><creatorcontrib>Parsa, S</creatorcontrib><creatorcontrib>Pellegrino, R</creatorcontrib><creatorcontrib>Ramirez, M A</creatorcontrib><creatorcontrib>Reh, M</creatorcontrib><creatorcontrib>Ricco, C</creatorcontrib><creatorcontrib>Rubbia, A</creatorcontrib><creatorcontrib>Sakashita, K</creatorcontrib><creatorcontrib>Sanchez, F</creatorcontrib><creatorcontrib>Sgalaberna, D</creatorcontrib><creatorcontrib>Shvartsman, A</creatorcontrib><creatorcontrib>Skrobova, N</creatorcontrib><creatorcontrib>Suslov, I A</creatorcontrib><creatorcontrib>Suvorov, S</creatorcontrib><creatorcontrib>Svirida, D</creatorcontrib><creatorcontrib>Teklu, A</creatorcontrib><creatorcontrib>Tereshchenko, V V</creatorcontrib><creatorcontrib>Tzanov, M</creatorcontrib><creatorcontrib>Vasilyev, I I</creatorcontrib><creatorcontrib>Wood, K</creatorcontrib><creatorcontrib>Yang, G</creatorcontrib><creatorcontrib>Yershov, N</creatorcontrib><creatorcontrib>Yokoyama, M</creatorcontrib><creatorcontrib>Yoshimoto, Y</creatorcontrib><creatorcontrib>Zhao, X</creatorcontrib><creatorcontrib>Zilberman, P</creatorcontrib><creatorcontrib>Zimmerman, E D</creatorcontrib><collection>ProQuest SciTech Collection</collection><collection>ProQuest Technology Collection</collection><collection>Materials Science & Engineering Collection</collection><collection>ProQuest Central (Alumni Edition)</collection><collection>ProQuest Central UK/Ireland</collection><collection>ProQuest Central Essentials</collection><collection>ProQuest Central</collection><collection>Technology Collection</collection><collection>ProQuest One Community College</collection><collection>ProQuest Central Korea</collection><collection>SciTech Premium Collection</collection><collection>ProQuest Engineering Collection</collection><collection>Engineering Database</collection><collection>Publicly Available Content Database</collection><collection>ProQuest One Academic Eastern Edition (DO NOT USE)</collection><collection>ProQuest One Academic</collection><collection>ProQuest One Academic UKI Edition</collection><collection>ProQuest Central China</collection><collection>Engineering Collection</collection><collection>arXiv.org</collection><jtitle>arXiv.org</jtitle></facets><delivery><delcategory>Remote Search Resource</delcategory><fulltext>fulltext</fulltext></delivery><addata><au>Alekseev, I</au><au>Arihara, T</au><au>Baranov, V</au><au>Bartoszek, L</au><au>Bernardi, L</au><au>Blondel, A</au><au>Boikov, A V</au><au>Buizza-Avanzini, M</au><au>Cadoux, F</au><au>Capó, J</au><au>Cayo, J</au><au>Chakrani, J</au><au>Chong, P S</au><au>Chvirova, A</au><au>Danilov, M</au><au>Davydov, Yu I</au><au>Dergacheva, A</au><au>Dokania, N</au><au>Douqa, D</au><au>Drapier, O</au><au>Eguchi, A</au><au>Favre, Y</au><au>Fedorova, D</au><au>Fedotov, S</au><au>Fujii, Y</au><au>Gastaldi, F</au><au>Gendotti, A</au><au>Glagolev, V</au><au>Guillaumat, R</au><au>Iwamoto, K</au><au>Jakkapu, M</au><au>Jesús-Valls, C</au><au>Jung, C K</au><au>Kakuno, H</au><au>Kasetti, S P</au><au>Khabibullin, M</au><au>Khotjantsev, A</au><au>Kikutani, H</au><au>Kobayashi, T</au><au>Kodama, S</au><au>Korzenev, A</au><au>Kose, U</au><au>Kudenko, Y</au><au>Kutter, T</au><au>Last, D</au><au>B Li</au><au>Z Li</au><au>Lin, L S</au><au>Lin, S</au><au>Louzir, M</au><au>Lux, T</au><au>Maret, L</au><au>Martynenko, S</au><au>Matsubara, T</au><au>Mauger, C</au><au>McGrew, C</au><au>Mefodiev, A</au><au>Mineev, O</au><au>Nakadaira, T</au><au>Nakagiri, K</au><au>Nanni, J</au><au>Nicola, L</au><au>Noah, E</au><au>Paolone, V</au><au>Parsa, S</au><au>Pellegrino, R</au><au>Ramirez, M A</au><au>Reh, M</au><au>Ricco, C</au><au>Rubbia, A</au><au>Sakashita, K</au><au>Sanchez, F</au><au>Sgalaberna, D</au><au>Shvartsman, A</au><au>Skrobova, N</au><au>Suslov, I A</au><au>Suvorov, S</au><au>Svirida, D</au><au>Teklu, A</au><au>Tereshchenko, V V</au><au>Tzanov, M</au><au>Vasilyev, I I</au><au>Wood, K</au><au>Yang, G</au><au>Yershov, N</au><au>Yokoyama, M</au><au>Yoshimoto, Y</au><au>Zhao, X</au><au>Zilberman, P</au><au>Zimmerman, E D</au><format>journal</format><genre>article</genre><ristype>JOUR</ristype><atitle>SuperFGD prototype time resolution studies</atitle><jtitle>arXiv.org</jtitle><date>2023-01-18</date><risdate>2023</risdate><eissn>2331-8422</eissn><abstract>The SuperFGD will be a part of the ND280 near detector of the T2K and Hyper Kamiokande projects, that will help to reduce systematic uncertainties related with neutrino flux and cross-section modeling. The upgraded ND280 will be able to perform a full exclusive reconstruction of the final state from neutrino-nucleus interactions, including measurements of low momentum protons, pions and, for the first time, event-by event measurements of neutron kinematics. The time resolution defines the neutron energy resolution. We present the results of time resolution measurements made with the SuperFGD prototype that consists of 9216 plastic scintillator cubes (cube size is 1 cm\(^3\)) readout with 1728 wavelength-shifting fibers going along three orthogonal directions. We use data from the muon beam exposure at CERN. The time resolution of 0.97 ns was obtained for one readout channel after implementing the time calibration with a correction for the time-walk effect. The time resolution improves with energy deposited in a scintillator cube. Averaging two readout channels for one scintillator cube improves the time resolution to 0.68 ns which means that signals in different channels are not synchronous. Therefore the contribution from the time recording step of 2.5 ns is averaged as well. Averaging time values from N channels improves the time resolution by \(\sim 1/\sqrt{N}\). Therefore a very good time resolution should be achievable for neutrons since neutron recoils hit typically several scintillator cubes and in addition produce larger amplitudes than muons. Measurements performed with a laser and a wide-bandwidth oscilloscope demonstrated that the time resolution obtained with the muon beam is not far from its expected limit. The intrinsic time resolution of one channel is 0.67 ns for signals of 56 photo-electron typical for minimum ionizing particles.</abstract><cop>Ithaca</cop><pub>Cornell University Library, arXiv.org</pub><doi>10.48550/arxiv.2206.10507</doi><oa>free_for_read</oa></addata></record> |
fulltext | fulltext |
identifier | EISSN: 2331-8422 |
ispartof | arXiv.org, 2023-01 |
issn | 2331-8422 |
language | eng |
recordid | cdi_arxiv_primary_2206_10507 |
source | arXiv.org; Free E- Journals |
subjects | Channels Cubes Energy resolution Kinematics Muons Neutrinos Particle beams Particle physics Physics - Instrumentation and Detectors Pions Prototypes Scintillation counters Time measurement |
title | SuperFGD prototype time resolution studies |
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