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Towards Understanding the Origin of Cosmic-Ray Positrons

Precision measurements of cosmic ray positrons by the Alpha Magnetic Spectrometer on the International Space Station are presented up to 1 TeV based on 1.9 million positrons.The positron flux exhibits a significant excess starting from $25.2 \pm 1.8$ GeV followed by a sharp drop-off above $284^{+91}...

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Detalles Bibliográficos
Autores principales:	Aguilar, M, Ali Cavasonza, L, Ambrosi, G, Arruda, L, Attig, N, Azzarello, P, Bachlechner, A, Barao, F, Barrau, A, Barrin, L, Bartoloni, A, Basara, L, Başeğmez-du Pree, S, Battiston, R, Becker, U, Behlmann, M, Beischer, B, Berdugo, J, Bertucci, B, Bindi, V, de Boer, W, Bollweg, K, Borgia, B, Boschini, M J, Bourquin, M, Bueno, E F, Burger, J, Burger, W J, Cai, X D, Capell, M, Caroff, S, Casaus, J, Castellini, G, Cervelli, F, Chang, Y H, Chen, G M, Chen, H S, Chen, Y, Cheng, L, Chou, H Y, Choutko, V, Chung, C H, Clark, C, Coignet, G, Consolandi, C, Contin, A, Corti, C, Crispoltoni, M, Cui, Z, Dadzie, K, Dai, Y M, Datta, A, Delgado, C, Della Torre, S, Demirköz, M B, Derome, L, Di Falco, S, Dimiccoli, F, Díaz, C, von Doetinchem, P, Dong, F, Donnini, F, Duranti, M, Egorov, A, Eline, A, Eronen, T, Feng, J, Fiandrini, E, Fisher, P, Formato, V, Galaktionov, Y, García-López, R J, Gargiulo, C, Gast, H, Gebauer, I, Gervasi, M, Giovacchini, F, Gómez-Coral, D M, Gong, J, Goy, C, Grabski, V, Grandi, D, Graziani, M, Guo, K H, Haino, S, Han, K C, He, Z H, Heil, M, Hsieh, T H, Huang, H, Huang, Z C, Incagli, M, Jia, Yi, Jinchi, H, Kanishev, K, Khiali, B, Kirn, Th, Konak, C, Kounina, O, Kounine, A, Koutsenko, V, Kulemzin, A, La Vacca, G, Laudi, E, Laurenti, G, Lazzizzera, I, Lebedev, A, Lee, H T, Lee, S C, Leluc, C, Li, J Q, Li, Q, Li, T X, Li, Z H, Light, C, Lin, C H, Lippert, T, Liu, F Z, Liu, Hu, Liu, Z, Lu, S Q, Lu, Y S, Luebelsmeyer, K, Luo, F, Luo, J Z, Luo, Xi, Lyu, S S, Machate, F, Mañá, C, Marín, J, Martin, T, Martínez, G, Masi, N, Maurin, D, Menchaca-Rocha, A, Meng, Q, Mo, D C, Molero, M, Mott, P, Mussolin, L, Nelson, T, Ni, J Q, Nikonov, N, Nozzoli, F, Oliva, A, Orcinha, M, Palermo, M, Palmonari, F, Paniccia, M, Pashnin, A, Pauluzzi, M, Pensotti, S, Perrina, C, Phan, H D, Picot-Clemente, N, Plyaskin, V, Pohl, M, Poireau, V, Popkow, A, Quadrani, L, Qi, X M, Qin, X, Qu, Z Y, Rancoita, P G, Rapin, D, Conde, A Reina, Rosier-Lees, S, Rozhkov, A, Rozza, D, Sagdeev, R, Solano, C, Schael, S, Schmidt, S M, Schulz von Dratzig, A, Schwering, G, Seo, E S, Shan, B S, Shi, J Y, Siedenburg, T, Song, J W, Sun, Z T, Tacconi, M, Tang, X W, Tang, Z C, Tian, J, Ting, Samuel C C, Ting, S M, Tomassetti, N, Torsti, J, Urban, T, Vagelli, V, Valente, E, Valtonen, E, Vázquez Acosta, M, Vecchi, M, Velasco, M, Vialle, J P, Vizán, J, Wang, L Q, Wang, N H, Wang, Q L, Wang, X, Wang, X Q, Wang, Z X, Wei, J, Weng, Z L, Wu, H, Xiong, R Q, Xu, W, Yan, Q, Yang, Y, Yi, H, Yu, Y J, Yu, Z Q, Zannoni, M, Zeissler, S, Zhang, C, Zhang, F, Zhang, J H, Zhang, Z, Zhao, F, Zheng, Z M, Zhuang, H L, Zhukov, V, Zichichi, A, Zimmermann, N, Zuccon, P
Lenguaje:	eng
Publicado:	2019
Materias:	Astrophysics and Astronomy
Acceso en línea:	https://dx.doi.org/10.1103/PhysRevLett.122.041102 http://cds.cern.ch/record/2683834

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author	Aguilar, M Ali Cavasonza, L Ambrosi, G Arruda, L Attig, N Azzarello, P Bachlechner, A Barao, F Barrau, A Barrin, L Bartoloni, A Basara, L Başeğmez-du Pree, S Battiston, R Becker, U Behlmann, M Beischer, B Berdugo, J Bertucci, B Bindi, V de Boer, W Bollweg, K Borgia, B Boschini, M J Bourquin, M Bueno, E F Burger, J Burger, W J Cai, X D Capell, M Caroff, S Casaus, J Castellini, G Cervelli, F Chang, Y H Chen, G M Chen, H S Chen, Y Cheng, L Chou, H Y Choutko, V Chung, C H Clark, C Coignet, G Consolandi, C Contin, A Corti, C Crispoltoni, M Cui, Z Dadzie, K Dai, Y M Datta, A Delgado, C Della Torre, S Demirköz, M B Derome, L Di Falco, S Dimiccoli, F Díaz, C von Doetinchem, P Dong, F Donnini, F Duranti, M Egorov, A Eline, A Eronen, T Feng, J Fiandrini, E Fisher, P Formato, V Galaktionov, Y García-López, R J Gargiulo, C Gast, H Gebauer, I Gervasi, M Giovacchini, F Gómez-Coral, D M Gong, J Goy, C Grabski, V Grandi, D Graziani, M Guo, K H Haino, S Han, K C He, Z H Heil, M Hsieh, T H Huang, H Huang, Z C Incagli, M Jia, Yi Jinchi, H Kanishev, K Khiali, B Kirn, Th Konak, C Kounina, O Kounine, A Koutsenko, V Kulemzin, A La Vacca, G Laudi, E Laurenti, G Lazzizzera, I Lebedev, A Lee, H T Lee, S C Leluc, C Li, J Q Li, Q Li, T X Li, Z H Light, C Lin, C H Lippert, T Liu, F Z Liu, Hu Liu, Z Lu, S Q Lu, Y S Luebelsmeyer, K Luo, F Luo, J Z Luo, Xi Lyu, S S Machate, F Mañá, C Marín, J Martin, T Martínez, G Masi, N Maurin, D Menchaca-Rocha, A Meng, Q Mo, D C Molero, M Mott, P Mussolin, L Nelson, T Ni, J Q Nikonov, N Nozzoli, F Oliva, A Orcinha, M Palermo, M Palmonari, F Paniccia, M Pashnin, A Pauluzzi, M Pensotti, S Perrina, C Phan, H D Picot-Clemente, N Plyaskin, V Pohl, M Poireau, V Popkow, A Quadrani, L Qi, X M Qin, X Qu, Z Y Rancoita, P G Rapin, D Conde, A Reina Rosier-Lees, S Rozhkov, A Rozza, D Sagdeev, R Solano, C Schael, S Schmidt, S M Schulz von Dratzig, A Schwering, G Seo, E S Shan, B S Shi, J Y Siedenburg, T Song, J W Sun, Z T Tacconi, M Tang, X W Tang, Z C Tian, J Ting, Samuel C C Ting, S M Tomassetti, N Torsti, J Urban, T Vagelli, V Valente, E Valtonen, E Vázquez Acosta, M Vecchi, M Velasco, M Vialle, J P Vizán, J Wang, L Q Wang, N H Wang, Q L Wang, X Wang, X Q Wang, Z X Wei, J Weng, Z L Wu, H Xiong, R Q Xu, W Yan, Q Yang, Y Yi, H Yu, Y J Yu, Z Q Zannoni, M Zeissler, S Zhang, C Zhang, F Zhang, J H Zhang, Z Zhao, F Zheng, Z M Zhuang, H L Zhukov, V Zichichi, A Zimmermann, N Zuccon, P
author_facet	Aguilar, M Ali Cavasonza, L Ambrosi, G Arruda, L Attig, N Azzarello, P Bachlechner, A Barao, F Barrau, A Barrin, L Bartoloni, A Basara, L Başeğmez-du Pree, S Battiston, R Becker, U Behlmann, M Beischer, B Berdugo, J Bertucci, B Bindi, V de Boer, W Bollweg, K Borgia, B Boschini, M J Bourquin, M Bueno, E F Burger, J Burger, W J Cai, X D Capell, M Caroff, S Casaus, J Castellini, G Cervelli, F Chang, Y H Chen, G M Chen, H S Chen, Y Cheng, L Chou, H Y Choutko, V Chung, C H Clark, C Coignet, G Consolandi, C Contin, A Corti, C Crispoltoni, M Cui, Z Dadzie, K Dai, Y M Datta, A Delgado, C Della Torre, S Demirköz, M B Derome, L Di Falco, S Dimiccoli, F Díaz, C von Doetinchem, P Dong, F Donnini, F Duranti, M Egorov, A Eline, A Eronen, T Feng, J Fiandrini, E Fisher, P Formato, V Galaktionov, Y García-López, R J Gargiulo, C Gast, H Gebauer, I Gervasi, M Giovacchini, F Gómez-Coral, D M Gong, J Goy, C Grabski, V Grandi, D Graziani, M Guo, K H Haino, S Han, K C He, Z H Heil, M Hsieh, T H Huang, H Huang, Z C Incagli, M Jia, Yi Jinchi, H Kanishev, K Khiali, B Kirn, Th Konak, C Kounina, O Kounine, A Koutsenko, V Kulemzin, A La Vacca, G Laudi, E Laurenti, G Lazzizzera, I Lebedev, A Lee, H T Lee, S C Leluc, C Li, J Q Li, Q Li, T X Li, Z H Light, C Lin, C H Lippert, T Liu, F Z Liu, Hu Liu, Z Lu, S Q Lu, Y S Luebelsmeyer, K Luo, F Luo, J Z Luo, Xi Lyu, S S Machate, F Mañá, C Marín, J Martin, T Martínez, G Masi, N Maurin, D Menchaca-Rocha, A Meng, Q Mo, D C Molero, M Mott, P Mussolin, L Nelson, T Ni, J Q Nikonov, N Nozzoli, F Oliva, A Orcinha, M Palermo, M Palmonari, F Paniccia, M Pashnin, A Pauluzzi, M Pensotti, S Perrina, C Phan, H D Picot-Clemente, N Plyaskin, V Pohl, M Poireau, V Popkow, A Quadrani, L Qi, X M Qin, X Qu, Z Y Rancoita, P G Rapin, D Conde, A Reina Rosier-Lees, S Rozhkov, A Rozza, D Sagdeev, R Solano, C Schael, S Schmidt, S M Schulz von Dratzig, A Schwering, G Seo, E S Shan, B S Shi, J Y Siedenburg, T Song, J W Sun, Z T Tacconi, M Tang, X W Tang, Z C Tian, J Ting, Samuel C C Ting, S M Tomassetti, N Torsti, J Urban, T Vagelli, V Valente, E Valtonen, E Vázquez Acosta, M Vecchi, M Velasco, M Vialle, J P Vizán, J Wang, L Q Wang, N H Wang, Q L Wang, X Wang, X Q Wang, Z X Wei, J Weng, Z L Wu, H Xiong, R Q Xu, W Yan, Q Yang, Y Yi, H Yu, Y J Yu, Z Q Zannoni, M Zeissler, S Zhang, C Zhang, F Zhang, J H Zhang, Z Zhao, F Zheng, Z M Zhuang, H L Zhukov, V Zichichi, A Zimmermann, N Zuccon, P
author_sort	Aguilar, M
collection	CERN
description	Precision measurements of cosmic ray positrons by the Alpha Magnetic Spectrometer on the International Space Station are presented up to 1 TeV based on 1.9 million positrons.The positron flux exhibits a significant excess starting from $25.2 \pm 1.8$ GeV followed by a sharp drop-off above $284^{+91}_{-64}$ GeV.In the entire energy range the positron flux is well described by the sum of a diffuse termassociated with low energy secondary positrons produced in the collision of cosmic rays, and a new source term of high energy positrons with a finite energy cutoff. The finite cutoff energy of the source term, $E_s$, is established with a significance of more than $4 \sigma$, and it's value is determined to be $E_s = 810^{+310}_{-180}$ GeV.These experimental data on cosmic ray positrons show that, at high energies, they predominantly originate either from dark matter collisions or from new astrophysical sources.
id	oai-inspirehep.net-1718083
institution	Organización Europea para la Investigación Nuclear
language	eng
publishDate	2019
record_format	invenio
spelling	oai-inspirehep.net-17180832022-08-10T12:26:09Zdoi:10.1103/PhysRevLett.122.041102http://cds.cern.ch/record/2683834engAguilar, MAli Cavasonza, LAmbrosi, GArruda, LAttig, NAzzarello, PBachlechner, ABarao, FBarrau, ABarrin, LBartoloni, ABasara, LBaşeğmez-du Pree, SBattiston, RBecker, UBehlmann, MBeischer, BBerdugo, JBertucci, BBindi, Vde Boer, WBollweg, KBorgia, BBoschini, M JBourquin, MBueno, E FBurger, JBurger, W JCai, X DCapell, MCaroff, SCasaus, JCastellini, GCervelli, FChang, Y HChen, G MChen, H SChen, YCheng, LChou, H YChoutko, VChung, C HClark, CCoignet, GConsolandi, CContin, ACorti, CCrispoltoni, MCui, ZDadzie, KDai, Y MDatta, ADelgado, CDella Torre, SDemirköz, M BDerome, LDi Falco, SDimiccoli, FDíaz, Cvon Doetinchem, PDong, FDonnini, FDuranti, MEgorov, AEline, AEronen, TFeng, JFiandrini, EFisher, PFormato, VGalaktionov, YGarcía-López, R JGargiulo, CGast, HGebauer, IGervasi, MGiovacchini, FGómez-Coral, D MGong, JGoy, CGrabski, VGrandi, DGraziani, MGuo, K HHaino, SHan, K CHe, Z HHeil, MHsieh, T HHuang, HHuang, Z CIncagli, MJia, YiJinchi, HKanishev, KKhiali, BKirn, ThKonak, CKounina, OKounine, AKoutsenko, VKulemzin, ALa Vacca, GLaudi, ELaurenti, GLazzizzera, ILebedev, ALee, H TLee, S CLeluc, CLi, J QLi, QLi, T XLi, Z HLight, CLin, C HLippert, TLiu, F ZLiu, HuLiu, ZLu, S QLu, Y SLuebelsmeyer, KLuo, FLuo, J ZLuo, XiLyu, S SMachate, FMañá, CMarín, JMartin, TMartínez, GMasi, NMaurin, DMenchaca-Rocha, AMeng, QMo, D CMolero, MMott, PMussolin, LNelson, TNi, J QNikonov, NNozzoli, FOliva, AOrcinha, MPalermo, MPalmonari, FPaniccia, MPashnin, APauluzzi, MPensotti, SPerrina, CPhan, H DPicot-Clemente, NPlyaskin, VPohl, MPoireau, VPopkow, AQuadrani, LQi, X MQin, XQu, Z YRancoita, P GRapin, DConde, A ReinaRosier-Lees, SRozhkov, ARozza, DSagdeev, RSolano, CSchael, SSchmidt, S MSchulz von Dratzig, ASchwering, GSeo, E SShan, B SShi, J YSiedenburg, TSong, J WSun, Z TTacconi, MTang, X WTang, Z CTian, JTing, Samuel C CTing, S MTomassetti, NTorsti, JUrban, TVagelli, VValente, EValtonen, EVázquez Acosta, MVecchi, MVelasco, MVialle, J PVizán, JWang, L QWang, N HWang, Q LWang, XWang, X QWang, Z XWei, JWeng, Z LWu, HXiong, R QXu, WYan, QYang, YYi, HYu, Y JYu, Z QZannoni, MZeissler, SZhang, CZhang, FZhang, J HZhang, ZZhao, FZheng, Z MZhuang, H LZhukov, VZichichi, AZimmermann, NZuccon, PTowards Understanding the Origin of Cosmic-Ray PositronsAstrophysics and AstronomyPrecision measurements of cosmic ray positrons by the Alpha Magnetic Spectrometer on the International Space Station are presented up to 1 TeV based on 1.9 million positrons.The positron flux exhibits a significant excess starting from $25.2 \pm 1.8$ GeV followed by a sharp drop-off above $284^{+91}_{-64}$ GeV.In the entire energy range the positron flux is well described by the sum of a diffuse termassociated with low energy secondary positrons produced in the collision of cosmic rays, and a new source term of high energy positrons with a finite energy cutoff. The finite cutoff energy of the source term, $E_s$, is established with a significance of more than $4 \sigma$, and it's value is determined to be $E_s = 810^{+310}_{-180}$ GeV.These experimental data on cosmic ray positrons show that, at high energies, they predominantly originate either from dark matter collisions or from new astrophysical sources.oai:inspirehep.net:17180832019
spellingShingle	Astrophysics and Astronomy Aguilar, M Ali Cavasonza, L Ambrosi, G Arruda, L Attig, N Azzarello, P Bachlechner, A Barao, F Barrau, A Barrin, L Bartoloni, A Basara, L Başeğmez-du Pree, S Battiston, R Becker, U Behlmann, M Beischer, B Berdugo, J Bertucci, B Bindi, V de Boer, W Bollweg, K Borgia, B Boschini, M J Bourquin, M Bueno, E F Burger, J Burger, W J Cai, X D Capell, M Caroff, S Casaus, J Castellini, G Cervelli, F Chang, Y H Chen, G M Chen, H S Chen, Y Cheng, L Chou, H Y Choutko, V Chung, C H Clark, C Coignet, G Consolandi, C Contin, A Corti, C Crispoltoni, M Cui, Z Dadzie, K Dai, Y M Datta, A Delgado, C Della Torre, S Demirköz, M B Derome, L Di Falco, S Dimiccoli, F Díaz, C von Doetinchem, P Dong, F Donnini, F Duranti, M Egorov, A Eline, A Eronen, T Feng, J Fiandrini, E Fisher, P Formato, V Galaktionov, Y García-López, R J Gargiulo, C Gast, H Gebauer, I Gervasi, M Giovacchini, F Gómez-Coral, D M Gong, J Goy, C Grabski, V Grandi, D Graziani, M Guo, K H Haino, S Han, K C He, Z H Heil, M Hsieh, T H Huang, H Huang, Z C Incagli, M Jia, Yi Jinchi, H Kanishev, K Khiali, B Kirn, Th Konak, C Kounina, O Kounine, A Koutsenko, V Kulemzin, A La Vacca, G Laudi, E Laurenti, G Lazzizzera, I Lebedev, A Lee, H T Lee, S C Leluc, C Li, J Q Li, Q Li, T X Li, Z H Light, C Lin, C H Lippert, T Liu, F Z Liu, Hu Liu, Z Lu, S Q Lu, Y S Luebelsmeyer, K Luo, F Luo, J Z Luo, Xi Lyu, S S Machate, F Mañá, C Marín, J Martin, T Martínez, G Masi, N Maurin, D Menchaca-Rocha, A Meng, Q Mo, D C Molero, M Mott, P Mussolin, L Nelson, T Ni, J Q Nikonov, N Nozzoli, F Oliva, A Orcinha, M Palermo, M Palmonari, F Paniccia, M Pashnin, A Pauluzzi, M Pensotti, S Perrina, C Phan, H D Picot-Clemente, N Plyaskin, V Pohl, M Poireau, V Popkow, A Quadrani, L Qi, X M Qin, X Qu, Z Y Rancoita, P G Rapin, D Conde, A Reina Rosier-Lees, S Rozhkov, A Rozza, D Sagdeev, R Solano, C Schael, S Schmidt, S M Schulz von Dratzig, A Schwering, G Seo, E S Shan, B S Shi, J Y Siedenburg, T Song, J W Sun, Z T Tacconi, M Tang, X W Tang, Z C Tian, J Ting, Samuel C C Ting, S M Tomassetti, N Torsti, J Urban, T Vagelli, V Valente, E Valtonen, E Vázquez Acosta, M Vecchi, M Velasco, M Vialle, J P Vizán, J Wang, L Q Wang, N H Wang, Q L Wang, X Wang, X Q Wang, Z X Wei, J Weng, Z L Wu, H Xiong, R Q Xu, W Yan, Q Yang, Y Yi, H Yu, Y J Yu, Z Q Zannoni, M Zeissler, S Zhang, C Zhang, F Zhang, J H Zhang, Z Zhao, F Zheng, Z M Zhuang, H L Zhukov, V Zichichi, A Zimmermann, N Zuccon, P Towards Understanding the Origin of Cosmic-Ray Positrons
title	Towards Understanding the Origin of Cosmic-Ray Positrons
title_full	Towards Understanding the Origin of Cosmic-Ray Positrons
title_fullStr	Towards Understanding the Origin of Cosmic-Ray Positrons
title_full_unstemmed	Towards Understanding the Origin of Cosmic-Ray Positrons
title_short	Towards Understanding the Origin of Cosmic-Ray Positrons
title_sort	towards understanding the origin of cosmic-ray positrons
topic	Astrophysics and Astronomy
url	https://dx.doi.org/10.1103/PhysRevLett.122.041102 http://cds.cern.ch/record/2683834
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Towards Understanding the Origin of Cosmic-Ray Positrons

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