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Properties of a New Group of Cosmic Nuclei: Results from the Alpha Magnetic Spectrometer on Sodium, Aluminum, and Nitrogen

We report the properties of sodium (Na) and aluminum (Al) cosmic rays in the rigidity range 2.15 GV to 3.0 TV based on 0.46 million sodium and 0.51 million aluminum nuclei collected by the Alpha Magnetic Spectrometer experiment on the International Space Station. We found that Na and Al, together wi...

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Detalles Bibliográficos
Autores principales: Aguilar, M, Cavasonza, L Ali, Alpat, B, Ambrosi, G, Arruda, L, Attig, N, Barao, F, Barrin, L, Bartoloni, A, Başeğmez-du Pree, S, Battiston, R, Behlmann, M, Beranek, B, Berdugo, J, Bertucci, B, Bindi, V, Bollweg, K, Borgia, B, Boschini, M J, Bourquin, M, Bueno, E F, Burger, J, Burger, W J, Burmeister, S, Cai, X D, Capell, M, Casaus, J, Castellini, G, Cervelli, F, Chang, Y H, Chen, G M, Chen, G R, Chen, H S, Chen, Y, Cheng, L, Chou, H Y, Chouridou, S, Choutko, V, Chung, C H, Clark, C, Coignet, G, Consolandi, C, Contin, A, Corti, C, Cui, Z, Dadzie, K, Delgado, C, Della Torre, S, Demirköz, M B, Derome, L, Di Falco, S, Di Felice, V, Díaz, C, Dimiccoli, F, von Doetinchem, P, Dong, F, Donnini, F, Duranti, M, Egorov, A, Eline, A, Feng, J, Fiandrini, E, Fisher, P, Formato, V, Freeman, C, Gámez, C, García-López, R J, Gargiulo, C, Gast, H, Gervasi, M, Giovacchini, F, Gómez-Coral, D M, Gong, J, Goy, C, Grabski, V, Grandi, D, Graziani, M, Haino, S, Han, K C, Hashmani, R K, He, Z H, Heber, B, Hsieh, T H, Hu, J Y, Incagli, M, Jang, W Y, Jia, Yi, Jinchi, H, Khiali, B, Kim, G N, Kirn, Th, Konyushikhin, M, Kounina, O, Kounine, A, Koutsenko, V, Krasnopevtsev, D, Kuhlman, A, Kulemzin, A, La Vacca, G, Laudi, E, Laurenti, G, Lazzizzera, I, Lebedev, A, Lee, H T, Lee, S C, Li, J Q, Li, M, Li, Q, Li, S, Li, J H, Li, Z H, Liang, J, Light, C, Lin, C H, Lippert, T, Liu, J H, Liu, Z, Lu, S Q, Lu, Y S, Luebelsmeyer, K, Luo, J Z, Luo, Xi, Machate, F, Mañá, C, Marín, J, Marquardt, J, Martin, T, Martínez, G, Masi, N, Maurin, D, Medvedeva, T, Menchaca-Rocha, A, Meng, Q, Mikhailov, V V, Molero, M, Mott, P, Mussolin, L, Negrete, J, Nikonov, N, Nozzoli, F, Oliva, A, Orcinha, M, Palermo, M, Palmonari, F, Paniccia, M, Pashnin, A, Pauluzzi, M, Pensotti, S, Phan, H D, Plyaskin, V, Pohl, M, Poluianov, S, Qin, X, Qu, Z Y, Quadrani, L, Rancoita, P G, Rapin, D, Conde, A Reina, Robyn, E, Rosier-Lees, S, Rozhkov, A, Rozza, D, Sagdeev, R, Schael, S, von Dratzig, A Schulz, Schwering, G, Seo, E S, Shakfa, Z, Shan, B S, Siedenburg, T, Solano, C, Song, J W, Song, X J, Sonnabend, R, Strigari, L, Su, T, Sun, Q, Sun, Z T, Tacconi, M, Tang, X W, Tang, Z C, Tian, J, Ting, Samuel C C, Ting, S M, Tomassetti, N, Torsti, J, Tüysüz, C, Urban, T, Usoskin, I, Vagelli, V, Vainio, R, Valencia-Otero, M, Valente, E, Valtonen, E, Vázquez Acosta, M, Vecchi, M, Velasco, M, Vialle, J P, Wang, C X, Wang, L, Wang, L Q, Wang, N H, Wang, Q L, Wang, S, Wang, X, Wang, Yu, Wang, Z M, Wei, J, Weng, Z L, Wu, H, Xiong, R Q, Xu, W, Yan, Q, Yang, Y, Yashin, I I, Yi, H, Yu, Y M, Yu, Z Q, Zannoni, M, Zhang, C, Zhang, F, Zhang, F Z, Zhang, J H, Zhang, Z, Zhao, F, Zheng, C, Zheng, Z M, Zhuang, H L, Zhukov, V, Zichichi, A, Zuccon, P
Lenguaje:eng
Publicado: 2021
Materias:
Acceso en línea:https://dx.doi.org/10.1103/PhysRevLett.127.021101
http://cds.cern.ch/record/2776602
_version_ 1780971638235332608
author Aguilar, M
Cavasonza, L Ali
Alpat, B
Ambrosi, G
Arruda, L
Attig, N
Barao, F
Barrin, L
Bartoloni, A
Başeğmez-du Pree, S
Battiston, R
Behlmann, M
Beranek, B
Berdugo, J
Bertucci, B
Bindi, V
Bollweg, K
Borgia, B
Boschini, M J
Bourquin, M
Bueno, E F
Burger, J
Burger, W J
Burmeister, S
Cai, X D
Capell, M
Casaus, J
Castellini, G
Cervelli, F
Chang, Y H
Chen, G M
Chen, G R
Chen, H S
Chen, Y
Cheng, L
Chou, H Y
Chouridou, S
Choutko, V
Chung, C H
Clark, C
Coignet, G
Consolandi, C
Contin, A
Corti, C
Cui, Z
Dadzie, K
Delgado, C
Della Torre, S
Demirköz, M B
Derome, L
Di Falco, S
Di Felice, V
Díaz, C
Dimiccoli, F
von Doetinchem, P
Dong, F
Donnini, F
Duranti, M
Egorov, A
Eline, A
Feng, J
Fiandrini, E
Fisher, P
Formato, V
Freeman, C
Gámez, C
García-López, R J
Gargiulo, C
Gast, H
Gervasi, M
Giovacchini, F
Gómez-Coral, D M
Gong, J
Goy, C
Grabski, V
Grandi, D
Graziani, M
Haino, S
Han, K C
Hashmani, R K
He, Z H
Heber, B
Hsieh, T H
Hu, J Y
Incagli, M
Jang, W Y
Jia, Yi
Jinchi, H
Khiali, B
Kim, G N
Kirn, Th
Konyushikhin, M
Kounina, O
Kounine, A
Koutsenko, V
Krasnopevtsev, D
Kuhlman, A
Kulemzin, A
La Vacca, G
Laudi, E
Laurenti, G
Lazzizzera, I
Lebedev, A
Lee, H T
Lee, S C
Li, J Q
Li, M
Li, Q
Li, S
Li, J H
Li, Z H
Liang, J
Light, C
Lin, C H
Lippert, T
Liu, J H
Liu, Z
Lu, S Q
Lu, Y S
Luebelsmeyer, K
Luo, J Z
Luo, Xi
Machate, F
Mañá, C
Marín, J
Marquardt, J
Martin, T
Martínez, G
Masi, N
Maurin, D
Medvedeva, T
Menchaca-Rocha, A
Meng, Q
Mikhailov, V V
Molero, M
Mott, P
Mussolin, L
Negrete, J
Nikonov, N
Nozzoli, F
Oliva, A
Orcinha, M
Palermo, M
Palmonari, F
Paniccia, M
Pashnin, A
Pauluzzi, M
Pensotti, S
Phan, H D
Plyaskin, V
Pohl, M
Poluianov, S
Qin, X
Qu, Z Y
Quadrani, L
Rancoita, P G
Rapin, D
Conde, A Reina
Robyn, E
Rosier-Lees, S
Rozhkov, A
Rozza, D
Sagdeev, R
Schael, S
von Dratzig, A Schulz
Schwering, G
Seo, E S
Shakfa, Z
Shan, B S
Siedenburg, T
Solano, C
Song, J W
Song, X J
Sonnabend, R
Strigari, L
Su, T
Sun, Q
Sun, Z T
Tacconi, M
Tang, X W
Tang, Z C
Tian, J
Ting, Samuel C C
Ting, S M
Tomassetti, N
Torsti, J
Tüysüz, C
Urban, T
Usoskin, I
Vagelli, V
Vainio, R
Valencia-Otero, M
Valente, E
Valtonen, E
Vázquez Acosta, M
Vecchi, M
Velasco, M
Vialle, J P
Wang, C X
Wang, L
Wang, L Q
Wang, N H
Wang, Q L
Wang, S
Wang, X
Wang, Yu
Wang, Z M
Wei, J
Weng, Z L
Wu, H
Xiong, R Q
Xu, W
Yan, Q
Yang, Y
Yashin, I I
Yi, H
Yu, Y M
Yu, Z Q
Zannoni, M
Zhang, C
Zhang, F
Zhang, F Z
Zhang, J H
Zhang, Z
Zhao, F
Zheng, C
Zheng, Z M
Zhuang, H L
Zhukov, V
Zichichi, A
Zuccon, P
author_facet Aguilar, M
Cavasonza, L Ali
Alpat, B
Ambrosi, G
Arruda, L
Attig, N
Barao, F
Barrin, L
Bartoloni, A
Başeğmez-du Pree, S
Battiston, R
Behlmann, M
Beranek, B
Berdugo, J
Bertucci, B
Bindi, V
Bollweg, K
Borgia, B
Boschini, M J
Bourquin, M
Bueno, E F
Burger, J
Burger, W J
Burmeister, S
Cai, X D
Capell, M
Casaus, J
Castellini, G
Cervelli, F
Chang, Y H
Chen, G M
Chen, G R
Chen, H S
Chen, Y
Cheng, L
Chou, H Y
Chouridou, S
Choutko, V
Chung, C H
Clark, C
Coignet, G
Consolandi, C
Contin, A
Corti, C
Cui, Z
Dadzie, K
Delgado, C
Della Torre, S
Demirköz, M B
Derome, L
Di Falco, S
Di Felice, V
Díaz, C
Dimiccoli, F
von Doetinchem, P
Dong, F
Donnini, F
Duranti, M
Egorov, A
Eline, A
Feng, J
Fiandrini, E
Fisher, P
Formato, V
Freeman, C
Gámez, C
García-López, R J
Gargiulo, C
Gast, H
Gervasi, M
Giovacchini, F
Gómez-Coral, D M
Gong, J
Goy, C
Grabski, V
Grandi, D
Graziani, M
Haino, S
Han, K C
Hashmani, R K
He, Z H
Heber, B
Hsieh, T H
Hu, J Y
Incagli, M
Jang, W Y
Jia, Yi
Jinchi, H
Khiali, B
Kim, G N
Kirn, Th
Konyushikhin, M
Kounina, O
Kounine, A
Koutsenko, V
Krasnopevtsev, D
Kuhlman, A
Kulemzin, A
La Vacca, G
Laudi, E
Laurenti, G
Lazzizzera, I
Lebedev, A
Lee, H T
Lee, S C
Li, J Q
Li, M
Li, Q
Li, S
Li, J H
Li, Z H
Liang, J
Light, C
Lin, C H
Lippert, T
Liu, J H
Liu, Z
Lu, S Q
Lu, Y S
Luebelsmeyer, K
Luo, J Z
Luo, Xi
Machate, F
Mañá, C
Marín, J
Marquardt, J
Martin, T
Martínez, G
Masi, N
Maurin, D
Medvedeva, T
Menchaca-Rocha, A
Meng, Q
Mikhailov, V V
Molero, M
Mott, P
Mussolin, L
Negrete, J
Nikonov, N
Nozzoli, F
Oliva, A
Orcinha, M
Palermo, M
Palmonari, F
Paniccia, M
Pashnin, A
Pauluzzi, M
Pensotti, S
Phan, H D
Plyaskin, V
Pohl, M
Poluianov, S
Qin, X
Qu, Z Y
Quadrani, L
Rancoita, P G
Rapin, D
Conde, A Reina
Robyn, E
Rosier-Lees, S
Rozhkov, A
Rozza, D
Sagdeev, R
Schael, S
von Dratzig, A Schulz
Schwering, G
Seo, E S
Shakfa, Z
Shan, B S
Siedenburg, T
Solano, C
Song, J W
Song, X J
Sonnabend, R
Strigari, L
Su, T
Sun, Q
Sun, Z T
Tacconi, M
Tang, X W
Tang, Z C
Tian, J
Ting, Samuel C C
Ting, S M
Tomassetti, N
Torsti, J
Tüysüz, C
Urban, T
Usoskin, I
Vagelli, V
Vainio, R
Valencia-Otero, M
Valente, E
Valtonen, E
Vázquez Acosta, M
Vecchi, M
Velasco, M
Vialle, J P
Wang, C X
Wang, L
Wang, L Q
Wang, N H
Wang, Q L
Wang, S
Wang, X
Wang, Yu
Wang, Z M
Wei, J
Weng, Z L
Wu, H
Xiong, R Q
Xu, W
Yan, Q
Yang, Y
Yashin, I I
Yi, H
Yu, Y M
Yu, Z Q
Zannoni, M
Zhang, C
Zhang, F
Zhang, F Z
Zhang, J H
Zhang, Z
Zhao, F
Zheng, C
Zheng, Z M
Zhuang, H L
Zhukov, V
Zichichi, A
Zuccon, P
author_sort Aguilar, M
collection CERN
description We report the properties of sodium (Na) and aluminum (Al) cosmic rays in the rigidity range 2.15 GV to 3.0 TV based on 0.46 million sodium and 0.51 million aluminum nuclei collected by the Alpha Magnetic Spectrometer experiment on the International Space Station. We found that Na and Al, together with nitrogen (N), belong to a distinct cosmic ray group. In this group, we observe that, similar to the N flux, both the Na flux and Al flux are well described by the sums of a primary cosmic ray component (proportional to the silicon flux) and a secondary cosmic ray component (proportional to the fluorine flux). The fraction of the primary component increases with rigidity for the N, Na, and Al fluxes and becomes dominant at the highest rigidities. The Na=Si and Al=Si abundance ratios at the source, $0.036 \pm 0.003$ for Na/Si and $0.103 \pm 0.004$ for Al/Si, are determined independent of cosmic ray propagation.
id cern-2776602
institution Organización Europea para la Investigación Nuclear
language eng
publishDate 2021
record_format invenio
spelling cern-27766022022-06-30T12:03:40Zdoi:10.1103/PhysRevLett.127.021101http://cds.cern.ch/record/2776602engAguilar, MCavasonza, L AliAlpat, BAmbrosi, GArruda, LAttig, NBarao, FBarrin, LBartoloni, ABaşeğmez-du Pree, SBattiston, RBehlmann, MBeranek, BBerdugo, JBertucci, BBindi, VBollweg, KBorgia, BBoschini, M JBourquin, MBueno, E FBurger, JBurger, W JBurmeister, SCai, X DCapell, MCasaus, JCastellini, GCervelli, FChang, Y HChen, G MChen, G RChen, H SChen, YCheng, LChou, H YChouridou, SChoutko, VChung, C HClark, CCoignet, GConsolandi, CContin, ACorti, CCui, ZDadzie, KDelgado, CDella Torre, SDemirköz, M BDerome, LDi Falco, SDi Felice, VDíaz, CDimiccoli, Fvon Doetinchem, PDong, FDonnini, FDuranti, MEgorov, AEline, AFeng, JFiandrini, EFisher, PFormato, VFreeman, CGámez, CGarcía-López, R JGargiulo, CGast, HGervasi, MGiovacchini, FGómez-Coral, D MGong, JGoy, CGrabski, VGrandi, DGraziani, MHaino, SHan, K CHashmani, R KHe, Z HHeber, BHsieh, T HHu, J YIncagli, MJang, W YJia, YiJinchi, HKhiali, BKim, G NKirn, ThKonyushikhin, MKounina, OKounine, AKoutsenko, VKrasnopevtsev, DKuhlman, AKulemzin, ALa Vacca, GLaudi, ELaurenti, GLazzizzera, ILebedev, ALee, H TLee, S CLi, J QLi, MLi, QLi, SLi, J HLi, Z HLiang, JLight, CLin, C HLippert, TLiu, J HLiu, ZLu, S QLu, Y SLuebelsmeyer, KLuo, J ZLuo, XiMachate, FMañá, CMarín, JMarquardt, JMartin, TMartínez, GMasi, NMaurin, DMedvedeva, TMenchaca-Rocha, AMeng, QMikhailov, V VMolero, MMott, PMussolin, LNegrete, JNikonov, NNozzoli, FOliva, AOrcinha, MPalermo, MPalmonari, FPaniccia, MPashnin, APauluzzi, MPensotti, SPhan, H DPlyaskin, VPohl, MPoluianov, SQin, XQu, Z YQuadrani, LRancoita, P GRapin, DConde, A ReinaRobyn, ERosier-Lees, SRozhkov, ARozza, DSagdeev, RSchael, Svon Dratzig, A SchulzSchwering, GSeo, E SShakfa, ZShan, B SSiedenburg, TSolano, CSong, J WSong, X JSonnabend, RStrigari, LSu, TSun, QSun, Z TTacconi, MTang, X WTang, Z CTian, JTing, Samuel C CTing, S MTomassetti, NTorsti, JTüysüz, CUrban, TUsoskin, IVagelli, VVainio, RValencia-Otero, MValente, EValtonen, EVázquez Acosta, MVecchi, MVelasco, MVialle, J PWang, C XWang, LWang, L QWang, N HWang, Q LWang, SWang, XWang, YuWang, Z MWei, JWeng, Z LWu, HXiong, R QXu, WYan, QYang, YYashin, I IYi, HYu, Y MYu, Z QZannoni, MZhang, CZhang, FZhang, F ZZhang, J HZhang, ZZhao, FZheng, CZheng, Z MZhuang, H LZhukov, VZichichi, AZuccon, PProperties of a New Group of Cosmic Nuclei: Results from the Alpha Magnetic Spectrometer on Sodium, Aluminum, and NitrogenNuclear Physics - ExperimentWe report the properties of sodium (Na) and aluminum (Al) cosmic rays in the rigidity range 2.15 GV to 3.0 TV based on 0.46 million sodium and 0.51 million aluminum nuclei collected by the Alpha Magnetic Spectrometer experiment on the International Space Station. We found that Na and Al, together with nitrogen (N), belong to a distinct cosmic ray group. In this group, we observe that, similar to the N flux, both the Na flux and Al flux are well described by the sums of a primary cosmic ray component (proportional to the silicon flux) and a secondary cosmic ray component (proportional to the fluorine flux). The fraction of the primary component increases with rigidity for the N, Na, and Al fluxes and becomes dominant at the highest rigidities. The Na=Si and Al=Si abundance ratios at the source, $0.036 \pm 0.003$ for Na/Si and $0.103 \pm 0.004$ for Al/Si, are determined independent of cosmic ray propagation.oai:cds.cern.ch:27766022021
spellingShingle Nuclear Physics - Experiment
Aguilar, M
Cavasonza, L Ali
Alpat, B
Ambrosi, G
Arruda, L
Attig, N
Barao, F
Barrin, L
Bartoloni, A
Başeğmez-du Pree, S
Battiston, R
Behlmann, M
Beranek, B
Berdugo, J
Bertucci, B
Bindi, V
Bollweg, K
Borgia, B
Boschini, M J
Bourquin, M
Bueno, E F
Burger, J
Burger, W J
Burmeister, S
Cai, X D
Capell, M
Casaus, J
Castellini, G
Cervelli, F
Chang, Y H
Chen, G M
Chen, G R
Chen, H S
Chen, Y
Cheng, L
Chou, H Y
Chouridou, S
Choutko, V
Chung, C H
Clark, C
Coignet, G
Consolandi, C
Contin, A
Corti, C
Cui, Z
Dadzie, K
Delgado, C
Della Torre, S
Demirköz, M B
Derome, L
Di Falco, S
Di Felice, V
Díaz, C
Dimiccoli, F
von Doetinchem, P
Dong, F
Donnini, F
Duranti, M
Egorov, A
Eline, A
Feng, J
Fiandrini, E
Fisher, P
Formato, V
Freeman, C
Gámez, C
García-López, R J
Gargiulo, C
Gast, H
Gervasi, M
Giovacchini, F
Gómez-Coral, D M
Gong, J
Goy, C
Grabski, V
Grandi, D
Graziani, M
Haino, S
Han, K C
Hashmani, R K
He, Z H
Heber, B
Hsieh, T H
Hu, J Y
Incagli, M
Jang, W Y
Jia, Yi
Jinchi, H
Khiali, B
Kim, G N
Kirn, Th
Konyushikhin, M
Kounina, O
Kounine, A
Koutsenko, V
Krasnopevtsev, D
Kuhlman, A
Kulemzin, A
La Vacca, G
Laudi, E
Laurenti, G
Lazzizzera, I
Lebedev, A
Lee, H T
Lee, S C
Li, J Q
Li, M
Li, Q
Li, S
Li, J H
Li, Z H
Liang, J
Light, C
Lin, C H
Lippert, T
Liu, J H
Liu, Z
Lu, S Q
Lu, Y S
Luebelsmeyer, K
Luo, J Z
Luo, Xi
Machate, F
Mañá, C
Marín, J
Marquardt, J
Martin, T
Martínez, G
Masi, N
Maurin, D
Medvedeva, T
Menchaca-Rocha, A
Meng, Q
Mikhailov, V V
Molero, M
Mott, P
Mussolin, L
Negrete, J
Nikonov, N
Nozzoli, F
Oliva, A
Orcinha, M
Palermo, M
Palmonari, F
Paniccia, M
Pashnin, A
Pauluzzi, M
Pensotti, S
Phan, H D
Plyaskin, V
Pohl, M
Poluianov, S
Qin, X
Qu, Z Y
Quadrani, L
Rancoita, P G
Rapin, D
Conde, A Reina
Robyn, E
Rosier-Lees, S
Rozhkov, A
Rozza, D
Sagdeev, R
Schael, S
von Dratzig, A Schulz
Schwering, G
Seo, E S
Shakfa, Z
Shan, B S
Siedenburg, T
Solano, C
Song, J W
Song, X J
Sonnabend, R
Strigari, L
Su, T
Sun, Q
Sun, Z T
Tacconi, M
Tang, X W
Tang, Z C
Tian, J
Ting, Samuel C C
Ting, S M
Tomassetti, N
Torsti, J
Tüysüz, C
Urban, T
Usoskin, I
Vagelli, V
Vainio, R
Valencia-Otero, M
Valente, E
Valtonen, E
Vázquez Acosta, M
Vecchi, M
Velasco, M
Vialle, J P
Wang, C X
Wang, L
Wang, L Q
Wang, N H
Wang, Q L
Wang, S
Wang, X
Wang, Yu
Wang, Z M
Wei, J
Weng, Z L
Wu, H
Xiong, R Q
Xu, W
Yan, Q
Yang, Y
Yashin, I I
Yi, H
Yu, Y M
Yu, Z Q
Zannoni, M
Zhang, C
Zhang, F
Zhang, F Z
Zhang, J H
Zhang, Z
Zhao, F
Zheng, C
Zheng, Z M
Zhuang, H L
Zhukov, V
Zichichi, A
Zuccon, P
Properties of a New Group of Cosmic Nuclei: Results from the Alpha Magnetic Spectrometer on Sodium, Aluminum, and Nitrogen
title Properties of a New Group of Cosmic Nuclei: Results from the Alpha Magnetic Spectrometer on Sodium, Aluminum, and Nitrogen
title_full Properties of a New Group of Cosmic Nuclei: Results from the Alpha Magnetic Spectrometer on Sodium, Aluminum, and Nitrogen
title_fullStr Properties of a New Group of Cosmic Nuclei: Results from the Alpha Magnetic Spectrometer on Sodium, Aluminum, and Nitrogen
title_full_unstemmed Properties of a New Group of Cosmic Nuclei: Results from the Alpha Magnetic Spectrometer on Sodium, Aluminum, and Nitrogen
title_short Properties of a New Group of Cosmic Nuclei: Results from the Alpha Magnetic Spectrometer on Sodium, Aluminum, and Nitrogen
title_sort properties of a new group of cosmic nuclei: results from the alpha magnetic spectrometer on sodium, aluminum, and nitrogen
topic Nuclear Physics - Experiment
url https://dx.doi.org/10.1103/PhysRevLett.127.021101
http://cds.cern.ch/record/2776602
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