Results 1 to 10 of about 4,448,337 (335)
Cosmic-ray antinuclei as messengers of new physics: status and outlook for the new decade. [PDF]
J Cosmol Astropart Phys, 2020 The precise measurement of cosmic-ray antinuclei serves as an important means for identifying the nature of dark matter and other new astrophysical phenomena, and could be used with other cosmic-ray species to understand cosmic-ray production and ...von Doetinchem P, Perez K, Aramaki T, Baker S, Barwick S, Bird R, Boezio M, Boggs SE, Cui M, Datta A, Donato F, Evoli C, Fabris L, Fabbietti L, Ferronato Bueno E, Fornengo N, Fuke H, Gerrity C, Gomez Coral D, Hailey C, Hooper D, Kachelriess M, Korsmeier M, Kozai M, Lea R, Li N, Lowell A, Manghisoni M, Moskalenko IV, Munini R, Naskret M, Nelson T, Ng KCY, Nozzoli F, Oliva A, Ong RA, Osteria G, Pierog T, Poulin V, Profumo S, Pöschl T, Quinn S, Re V, Rogers F, Ryan J, Saffold N, Sakai K, Salati P, Schael S, Serksnyte L, Shukla A, Stoessl A, Tjemsland J, Vannuccini E, Vecchi M, Winkler MW, Wright D, Xiao M, Xu W, Yoshida T, Zampa G, Zuccon P. +61 moreeuropepmc +3 more sourcesMeasurement of the cosmic ray proton spectrum from 40 GeV to 100 TeV with the DAMPE satellite. [PDF]
Sci Adv, 2019 DAMPE satellite has directly measured the cosmic ray proton spectrum from 40 GeV to 100 TeV and revealed a new feature at about 13.6 TeV. The precise measurement of the spectrum of protons, the most abundant component of the cosmic radiation, is ...DAMPE Collaboration, An Q, Asfandiyarov R, Azzarello P, Bernardini P, Bi XJ, Bi XJ, Cai MS, Chang J, Chen DY, Chen HF, Chen JL, Chen W, Cui MY, Cui TS, Dai HT, D'Amone A, De Benedittis A, De Mitri I, Di Santo M, Ding M, Dong TK, Dong YF, Dong ZX, Donvito G, Droz D, Duan JL, Duan KK, D'Urso D, Fan RR, Fan YZ, Fang F, Feng CQ, Feng L, Fusco P, Gallo V, Gan FJ, Gao M, Gargano F, Gong K, Gong YZ, Guo DY, Guo JH, Guo XL, Han SX, Hu YM, Huang GS, Huang XY, Huang YY, Ionica M, Jiang W, Jin X, Kong J, Lei SJ, Li S, Li WL, Li X, Li XQ, Li Y, Liang YF, Liang YM, Liao NH, Liu CM, Liu H, Liu J, Liu SB, Liu WQ, Liu Y, Loparco F, Luo CN, Ma M, Ma PX, Ma SY, Ma T, Ma XY, Marsella G, Mazziotta MN, Mo D, Niu XY, Pan X, Peng WX, Peng XY, Qiao R, Rao JN, Salinas MM, Shang GZ, Shen WH, Shen ZQ, Shen ZT, Song JX, Su H, Su M, Sun ZY, Surdo A, Teng XJ, Tykhonov A, Vitillo S, Wang C, Wang H, Wang HY, Wang JZ, Wang LG, Wang Q, Wang S, Wang XH, Wang XL, Wang YF, Wang YP, Wang YZ, Wang ZM, Wei DM, Wei JJ, Wei YF, Wen SC, Wu D, Wu J, Wu LB, Wu SS, Wu X, Xi K, Xia ZQ, Xu HT, Xu ZH, Xu ZL, Xu ZZ, Xue GF, Yang HB, Yang P, Yang YQ, Yang ZL, Yao HJ, Yu YH, Yuan Q, Yue C, Zang JJ, Zhang F, Zhang JY, Zhang JZ, Zhang PF, Zhang SX, Zhang WZ, Zhang Y, Zhang YJ, Zhang YL, Zhang YP, Zhang YQ, Zhang Z, Zhang ZY, Zhao H, Zhao HY, Zhao XF, Zhou CY, Zhou Y, Zhu X, Zhu Y, Zimmer S. +155 moreeuropepmc +3 more sourcesCosmic-Ray Extremely Distributed Observatory [PDF]
Symmetry, 2020 The Cosmic-Ray Extremely Distributed Observatory (CREDO) is a newly formed, global collaboration dedicated to observing and studying cosmic rays (CR) and cosmic-ray ensembles (CRE): groups of at least two CR with a common primary interaction vertex or ...P. Homola, D. Beznosko, G. Bhatta, Lukasz Bibrzycki, Michalina Borczyńska, L. Bratek, N. Budnev, Dariusz Burakowski, D. Alvarez-Castillo, K. A. Cheminant, A. Ćwikła, Punsiri Dam-O, N. Dhital, A. Duffy, Piotr Głownia, K. Gorzkiewicz, D. Góra, Alok C. Gupta, Z. Hlávková, Martin Homola, J. Jałocha, R. Kaminski, M. Karbowiak, M. Kasztelan, R. Kierepko, M. Knap, P. Kovács, S. Kuliński, B. Lozowski, M. Magrys, M. Medvedev, J. Mędrala, J. Mietelski, J. Miszczyk, A. Mozgova, A. Napolitano, V. Nazari, Y. Ng, M. Niedźwiecki, C. Oancea, B. Ogan, G. Opila, K. Oziomek, M. Pawlik, M. Piekarczyk, Bozena Poncyliusz, Jerzy Pryga, Matías Rosas, K. Rzecki, J. Zamora-Saá, K. Smelcerz, K. Smolek, Weronika K Stanek, J. Stasielak, S. Stuglik, J. Sulma, O. Sushchov, M. Svanidze, Kyle Tam, A. Tursunov, J. Vaquero, T. Wibig, K. Wozniak +62 moresemanticscholar +1 more sourceTowards Understanding the Origin of Cosmic-Ray Positrons and Electrons
Proceedings of 40th International Conference on High Energy physics — PoS(ICHEP2020), 2021 Precision measurements of cosmic-ray positron flux by the Alpha Magnetic Spectrometer on the International Space Station are presented based on 1.9 million positrons up to 1 TeV. The positron flux exhibits distinct and complex energy dependence.M. Aguilar, L. Ali Cavasonza, G. Ambrosi, L. Arruda, N. Attig, P. Azzarello, A. Bachlechner, F. Barão, A. Barrau, L. Barrin, A. Bartoloni, L. Basara, S. Başeğmez-du Pree, R. Battiston, U. Becker, M. Behlmann, B. Beischer, J. Berdugo, B. Bertucci, V. Bindi, W. de Boer, K. Bollweg, B. Borgia, M. Boschini, M. Bourquin, E. Bueno, J. Burger, W. Burger, X. Cai, M. Capell, S. Caroff, J. Casaus, G. Castellini, F. Cervelli, Y. H. Chang, G. Chen, H. Chen, Y. Chen, L. Cheng, H. Chou, V. Choutko, C. Chung, C. Clark, Nicolas Produit, C. Consolandi, A. Contin, C. Corti, M. Crispoltoni, Z. Cui, K. Dadzie, Y. Dai, A. Datta, C. Delgado, S. Della Torre, M. Demirköz, L. Derome, S. Di Falco, F. Dimiccoli, C. Díaz, P. von Doetinchem, F. Dong, F. Donnini, M. Duranti, A. Egorov, A. Eline, T. Eronen, J. Feng, E. Fiandrini, P. Fisher, V. Formato, Y. Galaktionov, R. García-López, C. Gargiulo, H. Gast, I. Gebauer, M. Gervasi, F. Giovacchini, D. Gómez-Coral, J. Gong, C. Goy, V. Grabski, D. Grandi, M. Graziani, K. Guo, S. Haino, K. Han, Z. H. He, M. Heil, T. Hsieh, H. Huang, Z. Huang, M. Incagli, Yi Jia, H. Jinchi, K. Kanishev, B. Khiali, T. Kirn, C. Konak, O. Kounina, A. Kounine, V. Koutsenko, A. Kulemzin, G. La Vacca, E. Laudi, G. Laurenti, I. Lazzizzera, A. Lebedev, H. T. Lee, S. Lee, C. Leluc, J. Li, Q. Li, T. X. Li, Z. Li, C. Light, C. H. Lin, T. Lippert, F. Liu, Hu Liu, Z. Liu, S. Lu, Y. Lu, K. Luebelsmeyer, F. Luo, J. Luo, Xi Luo, S. Lyu, F. Machate, C. Mañá, J. Marin, T. Martin, G. Martinez, N. Masi, D. Maurin, A. Menchaca-Rocha, Q. Meng, D. Mo, M. Molero, P. Mott, L. Mussolin, T. Nelson, J. Ni, N. Nikonov, F. Nozzoli, A. Oliva, M. Orcinha, M. Palermo, Federico Palmonari, M. Paniccia, A. Pashnin, M. Pauluzzi, S. Pensotti, C. Perrina, H D Phan, N. Picot-Clemente, V. Plyaskin, M. Pohl, V. Poireau, A. Popkow, L. Quadrani, X. Qi, X. Qin, Z. Qu, P. Rancoita, D. Rapin, A. R. Conde, S. Rosier-Lees, A. Rozhkov, D. Rozza, R. Sagdeev, C. Solano, S. Schael, S. M. Schmidt, A. Schulz von Dratzig, G. Schwering, E. Seo, B. Shan, J. Shi, T. Siedenburg, J. Song, Z. Sun, M. Tacconi, X. Tang, Z. Tang, J. Tian, S. Ting, S. Ting, N. Tomassetti, J. Torsti, T. Urban, V. Vagelli, E. Valente, E. Valtonen, M. Vazquez Acosta, M. Vecchi, M. Velasco, J. Vialle, J. Vizán, L. Wang, N. Wang, Q. Wang, X. Wang, X. Wang, Z. Wang, J. Wei, Z. Weng, H. Wu, R. Xiong, W. Xu, Qi Yan, Y. Yang, H. Yi, Y. Yu, Z. Yu, M. Zannoni, S. Zeissler, C. Zhang, F. Zhang, J. Zhang, Z. Zhang, F. Zhao, Z. Zheng, H. Zhuang, V. Zhukov, A. Zichichi, N. Zimmermann, P. Zuccon +226 moresemanticscholar +1 more sourceThe Updated Version of the A.Ne.Mo.S. GLE Alert System: The Case of the Ground-Level Enhancement GLE73 on 28 October 2021
Universe, 2022 A ground-level enhancement (GLE) event is a sudden increase in cosmic ray intensity originated by solar sources and recorded by ground-based detectors. GLEs are invariably associated with large solar flares that can release and accelerate solar particles Helen Mavromichalaki, Pavlos Paschalis, Maria Gerontidou, Maria-Christina Papailiou, Evangelos Paouris, Anastasia Tezari, Dimitra Lingri, Maria Livada, Argyris N. Stassinakis, Norma Crosby, Mark Dierckxsens +10 moredoaj +1 more sourceLeading cluster approach to simulations of hadron collisions with GHOST generator [PDF]
EPJ Web of Conferences, 2019 The model HDPM of CORSIKA has been updated and developed on the base of the recent measurements by ALICE, CMS, TOTEM, LHCb, LHCf... The new model, GHOST, involving a four-source production reproduces correctly the pseudo-rapidity distributions of charged Capdevielle Jean-Noël, Plebaniak Zbigniew, Szabelska Barbara, Szabelski Jacek +3 moredoaj +1 more sourceTAx4 surface detectors data analysis [PDF]
EPJ Web of Conferences, 2023 The TAx4 experiment aims to understand UHECR by expanding the observation area of the TA experiment by a factor of 4 and increasing the statistics of UHECR events with energy greater than 1019 eV.Fujisue Kozodoaj +1 more source
