Results 31 to 40 of about 3,781,710 (350)
COSMIC RAY ANTIPROTONS [PDF]
Particles, Strings and Cosmology (PASCOS 99), 2000 Cosmic ray antiprotons have been detected for over 20 years and are now measured reliably. Standard particle and astrophysics predict a conventional spectrum and abundance of secondary antiprotons consistent with all current measurements. These measurements place limits on exotic Galactic antiproton sources and non-standard antiproton properties ...openaire +2 more sourcesObservation of New Properties of Secondary Cosmic Rays Lithium, Beryllium, and Boron by the Alpha Magnetic Spectrometer on the International Space Station.
Physical Review Letters, 2018 We report on the observation of new properties of secondary cosmic rays Li, Be, and B measured in the rigidity (momentum per unit charge) range 1.9 GV to 3.3 TV with a total of 5.4×10^{6} nuclei collected by AMS during the first five years of operation ...M. Aguilar, L. Ali Cavasonza, 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, U. Becker, M. Behlmann, B. Beischer, J. Berdugo, B. Bertucci, K. F. Bindel, V. Bindi, W. de Boer, K. Bollweg, V. Bonnivard, B. Borgia, M. Boschini, M. Bourquin, E. Bueno, J. Burger, W. Burger, F. Cadoux, X. Cai, M. Capell, S. Caroff, J. Casaus, G. Castellini, 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, W. Creus, 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, D. D’Urso, A. Egorov, A. Eline, T. Eronen, J. Feng, E. Fiandrini, P. Fisher, V. Formato, Y. Galaktionov, G. Gallucci, R. García-López, C. Gargiulo, H. Gast, I. Gebauer, M. Gervasi, A. Ghelfi, 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, C. Huh, M. Incagli, M. Ionica, W. Jang, Yi Jia, H. Jinchi, S. Kang, K. Kanishev, B. Khiali, G. Kim, K. Kim, 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, H. S. Li, J. Li, Q. Li, T. X. Li, Y. Li, Z. Li, Z. Li, S. Lim, C. H. Lin, P. Lipari, T. Lippert, D. Liu, Hu Liu, V. D. Lordello, S. Lu, Y. Lu, K. Luebelsmeyer, F. Luo, J. Luo, S. Lyu, F. Machate, C. Mañá, J. Marin, T. Martin, G. Martinez, N. Masi, D. Maurin, A. Menchaca-Rocha, Q. Meng, V. Mikuni, D. Mo, P. Mott, T. Nelson, J. Ni, N. Nikonov, F. Nozzoli, A. Oliva, M. Orcinha, M. Palermo, Federico Palmonari, C. Palomares, M. Paniccia, M. Pauluzzi, S. Pensotti, C. Perrina, H. Phan, N. Picot-Clemente, F. Pilo, C. Pizzolotto, V. Plyaskin, M. Pohl, V. Poireau, L. Quadrani, X. Qi, X. Qin, Z. Qu, T. Räihä, P. Rancoita, D. Rapin, J. Ricol, S. Rosier-Lees, A. Rozhkov, D. Rozza, R. Sagdeev, S. Schael, S. M. Schmidt, A. Schulz von Dratzig, G. Schwering, E. Seo, B. Shan, J. Shi, T. Siedenburg, D. Son, J. Song, M. Tacconi, X. Tang, Z. Tang, D. Tescaro, S. Ting, S. Ting, N. Tomassetti, J. Torsti, C. Türkoğlu, T. Urban, V. Vagelli, E. Valente, E. Valtonen, M. Vazquez Acosta, M. Vecchi, M. Velasco, J. Vialle, V. Vitale, L. Wang, N. Wang, Q. Wang, X. Wang, X. Wang, Z. Wang, C. Wei, Z. Weng, K. Whitman, H. Wu, X. Wu, R. Xiong, W. Xu, Qi Yan, J. Yang, M. Yang, Y. Yang, H. Yi, Y. Yu, Z. Yu, M. Zannoni, S. Zeissler, C. Zhang, F. Zhang, J. Zhang, J. Zhang, S. Zhang, Z. Zhang, Z. Zheng, H. Zhuang, V. Zhukov, A. Zichichi, N. Zimmermann, P. Zuccon +253 moresemanticscholar +1 more sourceA large light-mass component of cosmic rays at 1017–1017.5 electronvolts from radio observations [PDF]
Nature, 2016 Cosmic rays are the highest-energy particles found in nature. Measurements of the mass composition of cosmic rays with energies of 1017–1018 electronvolts are essential to understanding whether they have galactic or extragalactic sources.S. Buitink, A. Corstanje, H. Falcke, J. Horandel, T. Huege, A. Nelles, J. Rachen, L. Rossetto, P. Schellart, O. Scholten, S. Veen, S. Thoudam, T. Trinh, J. Anderson, A. Asgekar, I. Avruch, M. Bell, M. Bentum, G. Bernardi, P. Best, A. Bonafede, F. Breitling, J. Broderick, W. Brouw, M. Bruggen, H. Butcher, D. Carbone, B. Ciardi, J. Conway, F. Gasperin, E. D. Geus, A. Deller, R. Dettmar, G. V. Diepen, S. Duscha, J. Eisloffel, D. Engels, J. Enriquez, R. Fallows, R. Fender, C. Ferrari, W. Frieswijk, M. Garrett, J. Grießmeier, A. Gunst, M. V. Haarlem, T. Hassall, G. Heald, J. Hessels, M. Hoeft, A. Horneffer, M. Iacobelli, H. Intema, E. Juette, A. Karastergiou, V. Kondratiev, M. Kramer, M. Kuniyoshi, G. Kuper, J. V. Leeuwen, G. Loose, P. Maat, G. Mann, S. Markoff, R. McFadden, D. McKay-Bukowski, J. McKean, M. Mevius, D. Mulcahy, H. Munk, M. Norden, E. Orrú, H. Paas, M. Pandey-Pommier, V. Pandey, M. Piętka, R. Pizzo, A. Polatidis, W. Reich, H. Rottgering, A. Scaife, D. Schwarz, M. Serylak, J. Sluman, O. Smirnov, B. Stappers, M. Steinmetz, A. Stewart, J. Swinbank, M. Tagger, Y. Tang, C. Tasse, M. C. Toribio, R. Vermeulen, C. Vocks, C. Vogt, R. V. Weeren, R. Wijers, S. Wijnholds, M. Wise, O. Wucknitz, S. Yatawatta, P. Zarka, J. A. Z. A. Institute, V. U. Brussel, Department of AstrophysicsIMAPP, R. Nijmegen, Astron, N. F. F. R. Astronomy, Nikhef, Science Park Amsterdam, M. F. Radioastronomie, Ikp, Karlsruhe Institute of Technology, D. Physics, Astronomy, U. C. Irvine, Kvi Cart, U. Groningen, D. 1. Potsdam, D. Gfz, Shell Technology Center, S. I. F. S. Research, K. Institute, Csiro Australia Telescope National Facility, University of Twente, H. C. F. Astrophysics, Ska South Africa, Institute for Astronomy, U. Edinburgh, U. Hamburg, Leibniz-Institut, S. O. Physics, U. Southampton, Research School for Astronomy, Astrophysics, Australian National University, A. S. M. F. Astronomy, U. Amsterdam, Max Planck Institute for Astrophysics, O. Observatory, Dept. of Earth, S. Sciences, C. U. Technology, BV SmarterVision, Astronomisches Institut der Ruhr-Universitat Bochum, Thuringer Landessternwarte, H. Sternwarte, Laboratoire Lagrange, Universit'e Cote d'Azur, L. Observatory, Leiden University, LPC2E - Universite d'OrleansCNRS, S. Nancay, O. D. P. -. Cnrsinsu, National Radio Astronomy Observatory, U. Oxford, A. Institute, N. A. O. O. Japan, Japan Sodankyla Geophysical Observatory, U. Oulu, Stfc Rutherford Appleton Laboratory, Harwell Science, Innovation Campus, Center for Relativistic Astrophysics - Georgia Institute Technology, C. Lyon, Observatoire de Lyon, F. Physik, U. Bielefeld, Electronics, R. University, J. B. C. F. Astrophysics, The University of Manchester, D. Sciences, P. University, Gepi, Observatoire de Paris, Cnrs, U. Diderot, Lesia +179 moresemanticscholar +1 more sourceThe Dipole Anisotropy of Galactic Cosmic Rays [PDF]
, 2018 The arrival directions of Galactic cosmic rays exhibit anisotropies up to the
level of one per-mille over various angular scales. Recent observations of
TeV-PeV cosmic rays show that the dipole anisotropy has a strong energy
dependence with a phase-flip ...Ahlers, Markuscore +2 more sourcesThe origin of galactic cosmic rays [PDF]
, 2007 The origin of galactic cosmic rays is one of the most interesting unsolved
problems in astroparticle physics. Experimentally, the problem is attacked by a
multi-disciplinary effort, namely by direct measurements of cosmic rays above
the atmosphere, by ...Aharonian, Aharonian, Aharonian, Allan, Amenomori, Antoni, Antoni, Antoni, Antoni, Antoni, Apel, Ardouin, Baade, Bell, Berezhko, Berezhko, Blanford, Candia, Doll, Engel, Engler, Falcke, Ferenc, Fermi, Gahbauer, Gaisser, Garcia-Munoz, Garzia-Munoz, Guzik, Hess, Hinton, Huege, Hörandel, Hörandel, Hörandel, Hörandel, Hörandel, Hörandel, Hörandel, Hörandel, Hörandel, Jörg R. Hörandel, Kestel, Krymsky, Maier, Matthews, Milke, Navarra, Ptuskin, Seo, Simpson, Strong, Völk, Weekes, Yanasak +54 morecore +3 more sources
