Results 41 to 50 of about 3,781,710 (350)
Protostars: Forges of cosmic rays? [PDF]
, 2016 Galactic cosmic rays (CR) are particles presumably accelerated in supernova remnant shocks that propagate in the interstellar medium up to the densest parts of molecular clouds, losing energy and their ionisation efficiency because of the presence of ...M. Padovani, A. Marcowith, P. Hennebelle, K. F. L. U. E. P. D. Montpellier, U. Montpellier, France., Inaf - Arcetri, Firenze, Italy., Cea, Irfu, Sap, C. Saclay, Gif-sur-Yvette, Irap, U. Toulouse +15 moresemanticscholar +1 more sourcePrecision Measurement of the Proton Flux in Primary Cosmic Rays from Rigidity 1 GV to 1.8 TV with the Alpha Magnetic Spectrometer on the International Space Station. [PDF]
Physical Review Letters, 2014 A precise measurement of the proton flux in primary cosmic rays with rigidity (momentum/charge) from 1 GV to 1.8 TV is presented based on 300 million events. Knowledge of the rigidity dependence of the proton flux is important in understanding the origin,M. Aguilar, D. Aisa, B. Alpat, A. Alvino, G. Ambrosi, K. Andeen, L. Arruda, N. Attig, P. Azzarello, A. Bachlechner, F. Barão, A. Barrau, L. Barrin, A. Bartoloni, L. Basara, M. Battarbee, R. Battiston, J. Bazo, U. Becker, M. Behlmann, B. Beischer, J. Berdugo, B. Bertucci, G. Bigongiari, V. Bindi, S. Bizzaglia, M. Bizzarri, G. Boella, W. de Boer, K. Bollweg, V. Bonnivard, B. Borgia, S. Borsini, M. Boschini, M. Bourquin, J. Burger, F. Cadoux, X. Cai, M. Capell, S. Caroff, J. Casaus, V. Cascioli, G. Castellini, I. Cernuda, D. Cerreta, F. Cervelli, M. Chae, Y. H. Chang, A. Chen, H. Chen, G. Cheng, H. Chen, L. Cheng, H. Chou, E. Choumilov, V. Choutko, C. Chung, C. Clark, R. Clavero, Nicolas Produit, C. Consolandi, A. Contin, C. Corti, E. Cortina Gil, B. Coste, W. Creus, M. Crispoltoni, Z. Cui, Y. Dai, C. Delgado, S. Della Torre, M. Demirköz, L. Derome, S. Di Falco, L. Di Masso, F. Dimiccoli, C. Díaz, P. von Doetinchem, F. Donnini, W. Du, M. Duranti, D. D’Urso, A. Eline, F. J. Eppling, T. Eronen, Y. Y. Fan, L. Farnesini, J. Feng, E. Fiandrini, A. Fiasson, E. Finch, P. Fisher, Y. Galaktionov, G. Gallucci, B. Garcia, R. García-López, C. Gargiulo, H. Gast, I. Gebauer, M. Gervasi, A. Ghelfi, W. Gillard, F. Giovacchini, P. Goglov, J. Gong, C. Goy, V. Grabski, D. Grandi, M. Graziani, C. Guandalini, I. Guerri, K. Guo, D. Haas, M. Habiby, S. Haino, K. Han, Z. H. He, M. Heil, J. Hoffman, T. Hsieh, Z. Huang, C. Huh, M. Incagli, M. Ionica, W. Jang, H. Jinchi, K. Kanishev, G. Kim, K. Kim, T. Kirn, R. Kossakowski, O. Kounina, A. Kounine, V. Koutsenko, Matthew Scott Krafczyk, G. La Vacca, E. Laudi, G. Laurenti, I. Lazzizzera, A. Lebedev, H. T. Lee, S. Lee, C. Leluc, G. Levi, H. L. Li, J. Li, Q. Li, Q. Li, T. X. Li, W. Li, Y. Li, Z. Li, Z. Li, S. Lim, C. H. Lin, P. Lipari, T. Lippert, D. Liu, H. Liu, M. Lolli, T. Lomtadze, M. Lu, S. Lu, Y. Lu, K. Luebelsmeyer, J. Luo, S. Lv, R. Majka, C. Mañá, J. Marin, T. Martin, G. Martinez, N. Masi, D. Maurin, A. Menchaca-Rocha, Q. Meng, D. Mo, L. Morescalchi, P. Mott, M. Müller, J. Ni, N. Nikonov, F. Nozzoli, P. Nunes, A. Obermeier, A. Oliva, M. Orcinha, Federico Palmonari, C. Palomares, M. Paniccia, A. Papi, M. Pauluzzi, E. Pedreschi, S. Pensotti, R. Pereira, N. Picot-Clemente, F. Pilo, A. Piluso, C. Pizzolotto, V. Plyaskin, M. Pohl, V. Poireau, E. Postaci, A. Putze, L. Quadrani, X. Qi, X. Qin, Z. Qu, T. Räihä, P. Rancoita, D. Rapin, J. Ricol, I. Rodríguez, S. Rosier-Lees, A. Rozhkov, D. Rozza, R. Sagdeev, J. Sandweiss, P. Saouter, C. Sbarra, S. Schael, S. M. Schmidt, A. Schulz von Dratzig, G. Schwering, G. Scolieri, E. Seo, B. Shan, Y. Shan, J. Shi, X. Shi, Y. Shi, T. Siedenburg, D. Son, F. Spada, F. Spinella, W. Sun, W. Sun, M. Tacconi, C. P. Tang, X. Tang, Z. Tang, L. Tao, D. Tescaro, S. Ting, S. Ting, N. Tomassetti, J. Torsti, C. Türkoğlu, T. Urban, V. Vagelli, E. Valente, C. Vannini, E. Valtonen, S. Vaurynovich, M. Vecchi, M. Velasco, J. Vialle, V. Vitale, S. Vitillo, L. Wang, N. Wang, Q. Wang, R. Wang, X. Wang, Z. Wang, Z. Weng, K. Whitman, J. Wienkenhöver, H. Wu, X. Wu, X. Xia, M. Xie, S. Xie, R. Xiong, G. Xin, N. Xu, W. Xu, Qi Yan, J. Yang, M. Yang, Q. Ye, H. Yi, Y. Yu, Z. Yu, S. Zeissler, J. Zhang, M. Zhang, X. B. Zhang, Z. Zhang, Z. Zheng, H. Zhuang, V. Zhukov, A. Zichichi, N. Zimmermann, P. Zuccon, C. Zurbach +295 moresemanticscholar +1 more sourceAntiproton Flux, Antiproton-to-Proton Flux Ratio, and Properties of Elementary Particle Fluxes in Primary Cosmic Rays Measured with the Alpha Magnetic Spectrometer on the International Space Station.
Physical Review Letters, 2016 A precision measurement by AMS of the antiproton flux and the antiproton-to-proton flux ratio in primary cosmic rays in the absolute rigidity range from 1 to 450 GV is presented based on 3.49×10^{5} antiproton events and 2.42×10^{9} proton events.M. Aguilar, L. Ali Cavasonza, B. Alpat, G. Ambrosi, L. Arruda, N. Attig, S. Aupetit, P. Azzarello, A. Bachlechner, F. Barão, A. Barrau, L. Barrin, A. Bartoloni, L. Basara, S. Başeğmez-du Pree, M. Battarbee, R. Battiston, J. Bazo, U. Becker, M. Behlmann, B. Beischer, J. Berdugo, B. Bertucci, V. Bindi, G. Boella, W. de Boer, K. Bollweg, V. Bonnivard, B. Borgia, M. Boschini, M. Bourquin, E. Bueno, J. Burger, F. Cadoux, X. Cai, M. Capell, S. Caroff, J. Casaus, G. Castellini, I. Cernuda, F. Cervelli, M. Chae, Y. H. Chang, A. Chen, G. Chen, H. Chen, L. Cheng, H. Chou, E. Choumilov, V. Choutko, C. Chung, C. Clark, R. Clavero, Nicolas Produit, C. Consolandi, A. Contin, C. Corti, B. Coste, W. Creus, M. Crispoltoni, Z. Cui, Y. Dai, 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, D. D’Urso, A. Egorov, A. Eline, T. Eronen, J. Feng, E. Fiandrini, E. Finch, P. Fisher, V. Formato, Y. Galaktionov, G. Gallucci, B. Garcia, R. García-López, C. Gargiulo, H. Gast, I. Gebauer, M. Gervasi, A. Ghelfi, F. Giovacchini, P. Goglov, D. Gómez-Coral, J. Gong, C. Goy, V. Grabski, D. Grandi, M. Graziani, I. Guerri, K. Guo, M. Habiby, S. Haino, K. Han, Z. H. He, M. Heil, J. Hoffman, T. Hsieh, H. Huang, Z. Huang, C. Huh, M. Incagli, M. Ionica, W. Jang, H. Jinchi, S. Kang, K. Kanishev, G. Kim, K. Kim, T. Kirn, C. Konak, O. Kounina, A. Kounine, V. Koutsenko, Matthew Scott Krafczyk, G. La Vacca, E. Laudi, G. Laurenti, I. Lazzizzera, A. Lebedev, H. T. Lee, S. Lee, C. Leluc, H. S. Li, J. Li, J. Li, Q. Li, T. X. Li, W. Li, Z. Li, Z. Li, S. Lim, C. H. Lin, P. Lipari, T. Lippert, D. Liu, Hu Liu, S. Lu, Y. Lu, K. Luebelsmeyer, F. Luo, J. Luo, S. Lv, R. Majka, C. Mañá, J. Marin, T. Martin, G. Martinez, N. Masi, D. Maurin, A. Menchaca-Rocha, Q. Meng, D. Mo, L. Morescalchi, P. Mott, T. Nelson, J. Ni, N. Nikonov, F. Nozzoli, P. Nunes, A. Oliva, M. Orcinha, Federico Palmonari, C. Palomares, M. Paniccia, M. Pauluzzi, S. Pensotti, R. Pereira, N. Picot-Clemente, F. Pilo, C. Pizzolotto, V. Plyaskin, M. Pohl, V. Poireau, A. Putze, L. Quadrani, X. Qi, X. Qin, Z. Qu, T. Räihä, P. Rancoita, D. Rapin, J. Ricol, I. Rodríguez, S. Rosier-Lees, A. Rozhkov, D. Rozza, R. Sagdeev, J. Sandweiss, P. Saouter, S. Schael, S. M. Schmidt, A. Schulz von Dratzig, G. Schwering, E. Seo, B. Shan, J. Shi, T. Siedenburg, D. Son, J. Song, W. Sun, M. Tacconi, X. Tang, Z. Tang, L. Tao, D. Tescaro, S. Ting, S. Ting, N. Tomassetti, J. Torsti, C. Türkoğlu, T. Urban, V. Vagelli, E. Valente, C. Vannini, E. Valtonen, M. Vazquez Acosta, M. Vecchi, M. Velasco, J. Vialle, V. Vitale, S. Vitillo, L. Wang, N. Wang, Q. Wang, X. Wang, X. Wang, Z. Wang, C. Wei, Z. Weng, K. Whitman, J. Wienkenhöver, M. Willenbrock, H. Wu, X. Wu, X. Xia, R. Xiong, W. Xu, Qi Yan, J. Yang, M. Yang, Y. Yang, H. Yi, Y. Yu, Z. Yu, S. Zeissler, C. Zhang, J. Zhang, J. Zhang, S. Zhang, S. Zhang, Z. Zhang, Z. Zheng, Z. Q. Zhu, H. Zhuang, V. Zhukov, A. Zichichi, N. Zimmermann, P. Zuccon +268 moresemanticscholar +1 more sourceGalactic cosmic rays
EPJ Web of Conferences, 2015 The multi-facet nature of the origin of cosmic rays is such that some of the problems currently met in our path to describing available data are due to oversimplified models of CR acceleration and transport, and others to lack of knowledge of the ...Blasi Pasqualedoaj +1 more sourceNew generation Cherenkov telescope array: HADAR and its performance introduction
Nuclear Physics BAstrophysical very high energy (VHE) gamma-rays are believed to result almost exclusively from the interactions of populations of highly relativistic particles with ambient matter or photon fields.Qingyuan Hou, Qingqian Zhou, Tianlu Chen, Youliang Feng, Hengjiao Liu, Yiqing Guo, Cheng Liu, Zihao Zhang, Xinlong Li, Qi Gao, Maoyuan Liu, Xiangli Qian, Yuanqi Liu, Jiadan Xie, Shanjie Shu, Weiqi Han, Qijiao Fang, Yanan Wang, Shaohua Zhang +18 moredoaj +1 more sourceOne century of cosmic rays – A particle physicist's view
EPJ Web of Conferences, 2015 Experiments on cosmic rays and the elementary particles share a common history that dates back to the 19th century. Following the discovery of radioactivity in the 1890s, the paths of the two fields intertwined, especially during the decades after the ...Sutton Christinedoaj +1 more source
