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Physical review letters · 2025

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

СтатьяНазвание и аннотация: Перевод пока не подготовлен
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Aguilar M, Ambrosi G, Anderson H, Arruda L, Attig N, Bagwell C, Barao F, Barbanera M, Barrin L, Bartoloni A, Battiston R, Bayyari A, Belyaev N, Bertucci B, Bindi V, Bollweg K, Bolster J, Borchiellini M, Borgia B, Boschini M J, Bourquin M, Brugnoni C, Burger J, Burger W J, Cai X D, Capell M, Casaus J, Castellini G, Cervelli F, Chang Y H, Chen G M, Chen G R, Chen H, 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, D'Angelo F, Dass A, 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, Duranti M, Egorov A, Eline A, Faldi F, Fehr D, Feng J, Fiandrini E, Fisher P, Formato V, García-López R J, Gargiulo C, Gast H, Gervasi M, Giovacchini F, Gómez-Coral D M, Gong J, Grandi D, Graziani M, Haino S, Han K C, Hashmani R K, He Z H, Heber B, Hernández-Nicolás F, Hsieh T H, Hu J Y, Huang B W, Ionica M, Incagli M, Jia Yi, Jinchi H, Karagöz G, Kirn Th, Klipfel A P, Kounina O, Kounine A, Koutsenko V, Krasnopevtsev D, Kuhlman A, Kulemzin A, La Vacca G, Laudi E, Laurenti G, LaVecchia G, Lazzizzera I, Lee H T, Lee S C, Li H L, Li J H, Li J Q, Li M, Li M, Li Q, Li Q, Li Q Y, Li S, Li S L, Li Z H, Liang M J, Liao P, Lin C H, Lippert T, Liu J H, Liu P C, Lu S Q, Lu Y S, Luo J Z, Luo Q, Luo S D, Luo Xi, Mañá C, Marín J, Marquardt J, Martínez G, Masi N, Maurin D, Medvedeva T, Menchaca-Rocha A, Meng Q, Mikhailov V V, Molero M, Mott P, Mussolin L, Jozani Y Najafi, Nicolaidis R, Nikonov N, Nozzoli F, Ocampo-Peleteiro J, Oliva A, Orcinha M, Palmonari F, Paniccia M, Pashnin A, Pauluzzi M, Pelosi D, Pensotti S, Pietzcker P, Plyaskin V, Poluianov S, Pridöhl D, Qu Z Y, Quadrani L, Rancoita P G, Rapin D, Conde A Reina, Robyn E, Rodríguez-García I, Romaneehsen L, Rossi F, Rozhkov A, Rozza D, Sagdeev R, Schael S, von Dratzig A Schultz, Schwering G, Seo E S, Shan B S, Shukla A, Siedenburg T, Silvestre G, Song J W, Song X J, Sonnabend R, Strigari L, Su T, Sun Q, Sun Z T, Tabarroni L, Tacconi M, Tang Z C, Tian J, Tian Y, Ting Samuel C C, Ting S M, Tomassetti N, Torsti J, Ubaldi A, Urban T, Usoskin I, Vagelli V, Vainio R, Väisänen P, Valencia-Otero M, Valente E, Valtonen E, Acosta M Vázquez, Vecchi M, Velasco M, Wang C X, Wang J C, Wang L, Wang L Q, Wang N H, Wang Q L, Wang S, Wang X, Wang Z M, Wei J, Weng Z L, Wu H, Wu Y, Wu Z B, Xiao J N, Xiong R Q, Xiong X Z, Xu W, Yan Q, Yang H T, Yang Y, Yi H, You Y H, Yu Y M, Yu Z Q, Zhang C, Zhang F Z, Zhang J, Zhang J H, Zhang Z, Zhao P W, Zheng C, Zheng Z M, Zhuang H L, Zhukov V, Zichichi A, Zuberi M, Zuccon P, AMS Collaboration

Аннотация

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.

ИП Урсолов Владлен Сергеевич

ИНН 500118482352 · ОГРНИП 314500117700049

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