Results 11 to 20 of about 4,292,570 (358)
Impact of Cosmic Ray Transport on Galactic Winds [PDF]
, 2017 The role of cosmic rays generated by supernovae and young stars has very
recently begun to receive significant attention in studies of galaxy formation
and evolution due to the realization that cosmic rays can efficiently
accelerate galactic winds. Microscopic cosmic ray transport processes are
fundamental for determining the efficiency of cosmic ray ...R. Farber, M. Ruszkowski, Karen Yang, E. Zweibel +3 morearxiv +3 more sourcesCosmic-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 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, L. 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 sourceMeasurement 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 sourcesOpen Questions in Cosmic-Ray Research at Ultrahigh Energies [PDF]
Frontiers in Astronomy and Space Sciences, 2019 We review open questions and prospects for progress in ultrahigh-energy cosmicray (UHECR) research, based on a series of discussions that took place during the “The High-Energy Universe: Gamma-Ray, Neutrino, and Cosmic-ray Astronomy” MIAPP workshop in ...R. Alves Batista, J. Biteau, M. Bustamante, K. Dolag, R. Engel, K. Fang, K. Kampert, D. Kostunin, M. Mostafá, K. Murase, F. Oikonomou, A. Olinto, M. Panasyuk, G. Sigl, A. Taylor, M. Unger +15 moresemanticscholar +1 more sourceDirect detection of a break in the teraelectronvolt cosmic-ray spectrum of electrons and positrons [PDF]
Nature, 2017 High-energy cosmic-ray electrons and positrons (CREs), which lose energy quickly during their propagation, provide a probe of Galactic high-energy processes and may enable the observation of phenomena such as dark-matter particle annihilation or decay ...G. Ambrosi, Q. An, R. Asfandiyarov, P. Azzarello, P. Bernardini, B. Bertucci, M. Cai, J. Chang, D. Chen, H. Chen, J. Chen, W. Chen, M. Cui, T. Cui, A. D’Amone, A. Benedittis, I. Mitri, M. D. Santo, J. N. Dong, T. Dong, Y. Dong, Z. Dong, G. Donvito, D. Droz, K. Duan, J. Duan, M. Duranti, D. D’Urso, R. Fan, Y. Fan, F. Fang, C. Feng, L. Feng, P. Fusco, V. Gallo, F. Gan, M. Gao, S. Gao, F. Gargano, S. Garrappa, K. Gong, Y. Gong, D. Guo, J. Guo, Y. Hu, G. Huang, Y. -. Huang, M. Ionica, D. Jiang, W. Jiang, X. Jin, J. Kong, S. Lei, S. Li, X. Li, W. Li, Y. Li, Y. Liang, Y. Liang, N. Liao, H. Liu, J. Liu, S. Liu, W. Liu, Y. Liu, F. Loparco, M. Ma, P. Ma, S. Ma, T. Ma, X. Ma, X. Ma, G. Marsella, M. Mazziotta, D. Mo, X. Niu, X. Peng, W. Peng, R. Qiao, J. Rao, M. Salinas, G. Shang, W. Shen, Z. Shen, Z. Shen, J. Song, H. Su, M. Su, Z. Sun, A. Surdo, X. Teng, X. Tian, A. Tykhonov, V. Vagelli, S. Vitillo, C. Wang, H. Wang, H. Wang, J. Wang, L. Wang, Q. Wang, S. Wang, X. H. Wang, X. Wang, Y. Wang, Y. Wang, Yu Wang, S. Wen, Z. Wang, D. Wei, J. Wei, Y. F. Wei, D. Wu, J. Wu, L. Wu, S. Wu, X. Wu, K. Xi, Z. Xia, Y. Xin, H. Xu, Z. L. Xu, Z. Xu, G. Xue, H. Yang, P. Yang, Y. Q. Yang, Z. L. Yang, H. Yao, Y. Yu, Q. Yuan, C. Yue, J. Zang, C. Zhang, D. L. Zhang, F. Zhang, J. Zhang, J. Zhang, J. Zhang, L. Zhang, P. Zhang, S. Zhang, W. Zhang, Y. Zhang, Y. Zhang, Y. Zhang, Y. Zhang, Y. P. Zhang, Z. Zhang, Z. Zhang, H. Zhao, H. Zhao, X. Zhao, C. Zhou, Y. Zhou, X. Zhu, Y. Zhu, S. Zimmer +157 moresemanticscholar +1 more sourceChromosomal breaks at the origin of small tandem DNA duplications
BioEssays, Volume 45, Issue 1, January 2023., 2023 Small tandem DNA duplications form a specific mutational signature frequently found in human disease alleles and cancer genes. Here we hypothesize that these duplications mainly arise at chromosomal DNA breaks that result from two closely located single‐stranded nicks, through error‐prone repair by the non‐homologous end‐joining pathway. Abstract
Small Joost Schimmel, Marloes D. van Wezel, Robin van Schendel, Marcel Tijsterman +3 morewiley +1 more sourceIntroduction to Cosmic Rays [PDF]
, 2007 Energetic particles, traditionally called Cosmic Rays, were discovered nearly a hundred years ago, and their origin is still uncertain. Their main constituents are the normal nuclei as in the standard cosmic abundances of matter, with some enhancements for the heavier elements; there are also electrons, positrons and anti-protons, but no anti-nuclei ...Biermann, Peter, Sigl, Guenteropenaire +4 more sources
