Antiprotons and Elementary Particles over a Solar Cycle: Results from the Alpha Magnetic Spectrometer

We present results over an 11-year Solar cycle of cosmic antiprotons based on 1.1×10^{6} events in the rigidity range from 1.00 to 41.9 GV. The p[over ¯] fluxes exhibit distinct properties. The magnitude of the p[over ¯] flux temporal variation is significantly smaller than those of p, e^{-}, and e^{+}. A hysteresis between the p[over ¯] fluxes and the p fluxes is observed, whereas the p[over ¯] and e^{-} fluxes show a linear correlation. With a model-independent analysis, we found a universal relation between the shape of the rigidity spectrum and the magnitude of flux temporal variation over an 11-year Solar cycle for both positively and negatively charged particles. The simultaneous results on p[over ¯] and p, e^{-}, and e^{+} provide unique information for understanding particle transport in the Solar System as a function of mass, charge, and spectral shape.

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Journal
Physical Review Letters
Published
2025-02-03
DOI
https://doi.org/10.1103/physrevlett.134.051002
Citations
14
Primary Topic
Dark Matter and Cosmic Phenomena
Type
article
Field-Weighted Citation Impact
26.18

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article

Antiprotons and Elementary Particles over a Solar Cycle: Results from the Alpha Magnetic Spectrometer

G. R. Chen, P. von Doetinchem, M. Duranti, R. K. Hashmani et al.
14 citations
Physical Review Letters
Dark Matter and Cosmic Phenomena
26.18
article

Antiprotons and Elementary Particles over a Solar Cycle: Results from the Alpha Magnetic Spectrometer

G. R. Chen, P. von Doetinchem, M. Duranti, R. K. Hashmani, Y. Najafi Jozani, M. Incagli, Nicola Tomassetti, M. Graziani, V. V. Mikhailov, G. Ambrosi, Alessio Ubaldi, D. Maurin, Timothy H. Hsieh, Ilya Usoskin, Samuel C.C. Ting, D. Pridöhl, R. Z. Sagdeev, G. Silvestre, D. M. Gómez-Coral, R. Battiston, A. Eline, M. Zuberi, A. Oliva, S. C. Lee, A. Shukla, Dario Pelosi, B. W. Huang, M. Vecchi, D. Rozza, C. Delgado Mendez, M. Li, Z. T. Sun, Z. H. Qu, J. H. Zhang, B. Demirköz, J. Ocampo-Peleteiro, H.L. Zhuang, Zhibin Wu, G. Laurenti, P. Väisänen, G. La Vacca, B. Heber, Fulvio D’Angelo, E. Robyn, O. Kounina, M. Paniccia, F. Dimiccoli, A. I. Egorov, A. Contin, C. Consolandi, F. Nozzoli, S. Pensotti, I. Lazzizzera, E. S. Seo, E. Fiandrini, Jie Tian, L. Wang, A. Zichichi, F. Palmonari, V. Plyaskin, M. Orcinha, E. Laudi, Thomas K. Lippert, M. Borchiellini, Chuncheng Wei, Amala Dass, Johanna Bürger, J. Bolster, S. Haino, J. Marquardt, C. Zhang, L. Quadrani, H. R. Anderson, G. Karagöz, X. Wang, V. Vagelli, Z. H. Li, Lisa Romaneehsen, F. Barão, Z. Cui, J. Casaus, S. Li, G. LaVecchia, V. Bindi, J. Zhang, V. Formato, N. Attig, Ammar Bayyari, H. S. Chen, A. Kuhlman, I. Rodríguez-García, H. Y. Chou, N. H. Wang, S. Di Falco, L. Mussolin, C. X. Wang, Stepan Poluianov, Miguel Molero Gonzalez, M. Tacconi, N. L. Belyaev, J. Gong, H. L. Li, S. Della Torre, C. H. Chung, J. H. Li, Chao‐Hung Lin, M. Valencia-Otero, Xiaojian Song, L. Q. Wang, L. Barrin, A. Kounine, L. Derome, G. Castellini, Y. H. You, Z. Zhang, Q. Li, A. P. Klipfel, M. Velasco, Riccardo Nicolaidis, W. Xu, F. Cervelli, Q. Luo, P.G. Rancoita, F. Z. Zhang, C. Zheng, N. Masi, F. Faldi, C. Corti, F. Giovacchini, M. Aguilar, D. Grandi, B. S. Shan, H. Chen, C. Díaz, S. Q. Lu, M. Gervasi, J. H. Feng, P. Zuccon, A. Menchaca-Rocha, Q. L. Wang, V. Choutko, Jiwei Song, R. Sonnabend, Yi Jia, Z. M. Zheng, T. Su, Rami Vainio, S. Kokou Dadzie, D. Krasnopevtsev, N. Nikonov, Xi Luo, Z. M. Wang, H. T. Lee, M. Boschini, Y. Chen, L. Arruda, Shiliang Li, B. Bertucci, Lidia Strigari, A. Pashnin, V. Di Felice, C. Bagwell, A. Kulemzin, D. Fehr, P. Pietzcker, L. Tabarroni, C. Brugnoni, Qiang Li, Qie Sun, Y. Yang, Shan Luo, Young Moon Yu, A. Reina Conde, Qi Yan, H. Yang, Lin Cheng, Xianze Xiong, Yao Lu, Pu Liao, B. Borgia, Q. Meng, Pei Zhao, Y. Tian, F. Rossi, Jiangyong Hu, Z. H. He, A. Bartoloni, R. J. Garcı́a López, J. Marín, M. Capell, Th. Kirn, M. Pauluzzi, M. Barbanera, G. M. Chen, W. J. Burger, E. Valente, M. Bourquin, C. Mañá, T. Siedenburg, S. Schael, P.H. Fisher, Z. Q. Yu, H. Wu, T. Medvedeva, R. Q. Xiong, C. Gargiulo, G. Martı́nez, P. Mott, E. Valtonen, X.D. Cai, G. Coignet, A. Rozhkov, Y. Wu, K. C. Han, Z. Weng, Fang Dong, T. Urban, P. C. Liu, J. Torsti, Zichao Tang, A. Schultz von Dratzig, S. Chouridou, Han Yi, H. Gast, V. Koutsenko, D. Rapin, C. Clark, J. Luo, K. Bollweg, G. Schwering, Jincheng Wang, S.M. Ting, M. Ionica, V. Zhukov, H. Jinchi, J. N. Xiao, M. J. Liang, S. Wang, M. Vázquez Acosta, Y. H. Chang, Q. Y. Li, Haibo Liu, F. Hernández-Nicolás
article en
14 citations

Abstract

We present results over an 11-year Solar cycle of cosmic antiprotons based on 1.1×10^{6} events in the rigidity range from 1.00 to 41.9 GV. The p[over ¯] fluxes exhibit distinct properties. The magnitude of the p[over ¯] flux temporal variation is significantly smaller than those of p, e^{-}, and e^{+}. A hysteresis between the p[over ¯] fluxes and the p fluxes is observed, whereas the p[over ¯] and e^{-} fluxes show a linear correlation. With a model-independent analysis, we found a universal relation between the shape of the rigidity spectrum and the magnitude of flux temporal variation over an 11-year Solar cycle for both positively and negatively charged particles. The simultaneous results on p[over ¯] and p, e^{-}, and e^{+} provide unique information for understanding particle transport in the Solar System as a function of mass, charge, and spectral shape.

Physical Review LettersVol. 134(5)
University of Geneva (CH), University of Hawaii System (US), Shandong University (CN), University of Turku (FI), Sun Yat-sen University (CN), Universidad de La Laguna (ES), University of Groningen (NL), National Chung Shan Institute of Science and Technology (TW), University of Trento (IT), Chinese Academy of Sciences (CN), Middle East Technical University (TR), National Central University (TW), University of Perugia (IT), LIP - Laboratory of Instrumentation and Experimental Particle Physics (PT), Agenzia Spaziale Italiana (IT), Ernst Ruska Centre (DE), Christian-Albrechts-Universität zu Kiel (DE), Genomics Research Center, Academia Sinica (TW), East–West Center (US), Southeast University (BD), Istituto Nazionale di Fisica Nucleare, Trento Institute for Fundamental Physics And Applications (IT), Institute of Physics, Academia Sinica (TW), Istituto Nazionale di Fisica Nucleare, Roma Tor Vergata (IT), National Aeronautics and Space Administration (US), Institute of Electrical Engineering (CN), Instituto de Astrofísica de Canarias (ES), Institute of High Energy Physics (CN), Istituto Nazionale di Fisica Nucleare, Sezione di Milano Bicocca (IT), Istituto Nazionale di Fisica Nucleare, Sezione di Bologna (IT), Johnson Space Center (US), Istituto Nazionale di Fisica Nucleare, Sezione di Roma I (IT), Zhejiang University-University of Edinburgh Institute (CN), Istituto Nazionale di Fisica Nucleare, Sezione di Pisa (IT), Istituto Nazionale di Fisica Nucleare, Sezione di Perugia (IT), University of Chinese Academy of Sciences (CN), Centro de Investigaciones Energéticas, Medioambientales y Tecnológicas (ES), Shandong Institute of Advanced Technology, Institut des langues et cultures d'Europe, Amérique, Afrique, Asie et Australie (FR), Massachusetts Institute of Technology (US), University of Milano-Bicocca (IT), University of Maryland, College Park (US), European Organization for Nuclear Research (CH), Université Savoie Mont Blanc (FR), Zhejiang University (CN), Southeast University (CN), Beihang University (CN), Academia Sinica (TW), Sapienza University of Rome (IT), RWTH Aachen University (DE), Universidad Nacional Autónoma de México (MX), Université Grenoble Alpes (FR), National Cheng Kung University (TW), University of Bologna (IT), University of Oulu (FI)
National Science Foundation, U.S. Department of Energy, National Aeronautics and Space Administration, Massachusetts Institute of Technology, Shandong University, CERN, National Energy Research Scientific Computing Center, Türkiye Enerji, Nükleer ve Maden Araştırma Kurumu, National Natural Science Foundation of China, Academia Sinica, Centro para el Desarrollo Tecnológico Industrial, Academy of Finland, Suomalainen Tiedeakatemia, Chinese Academy of Sciences, Centre National d’Etudes Spatiales, Ministry of Science and Technology of the People's Republic of China, Government of Guangdong Province, Deutsches Zentrum für Luft- und Raumfahrt, Government of Jiangsu Province, Consejo Nacional de Ciencia y Tecnología, Nederlandse Organisatie voor Wetenschappelijk Onderzoek, Agenzia Spaziale Italiana, China Scholarship Council, Ministry of Science and Technology, Taiwan, Centre National de la Recherche Scientifique, Ministerio de Ciencia e Innovación, Universidad Nacional Autónoma de México, RWTH Aachen University, National Cheng Kung University, Università degli Studi di Perugia, Ministero dell'Università e della Ricerca, Instituto de Astrofísica de Canarias, Marshall Space Flight Center, Johnson Space Center, Fundação para a Ciência e a Tecnologia, Instituto Nazionale di Fisica Nucleare, European Regional Development Fund, Centro de Investigaciones Energéticas, Medioambientales y Tecnológicas, Agencia Estatal de Investigación, Institute of High Energy Physics, National Key Research and Development Program of China, Institut National de Physique Nucléaire et de Physique des Particules, Government of Shandong Province
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Dark Matter and Cosmic Phenomena
26.18
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