Neutrinos and Cosmic Rays Observed by IceCube
High Energy Astrophysical Phenomena
2019-01-23 v1
Abstract
The core mission of the IceCube Neutrino observatory is to study the origin and propagation of cosmic rays. IceCube, with its surface component IceTop, observes multiple signatures to accomplish this mission. Most important are the astrophysical neutrinos that are produced in interactions of cosmic rays, close to their sources and in interstellar space. IceCube is the first instrument that measures the properties of this astrophysical neutrino flux, and constrains its origin. In addition, the spectrum, composition and anisotropy of the local cosmic-ray flux are obtained from measurements of atmospheric muons and showers. Here we provide an overview of recent findings from the analysis of IceCube data, and their implications on our understanding of cosmic rays.
Cite
@article{arxiv.1701.03731,
title = {Neutrinos and Cosmic Rays Observed by IceCube},
author = {IceCube Collaboration and M. G. Aartsen and M. Ackermann and J. Adams and J. A. Aguilar and M. Ahlers and M. Ahrens and I. Al Samarai and D. Altmann and K. Andeen and T. Anderson and I. Ansseau and G. Anton and M. Archinger and C. Argüelles and J. Auffenberg and S. Axani and X. Bai and S. W. Barwick and V. Baum and R. Bay and J. J. Beatty and J. Becker Tjus and K. -H. Becker and S. BenZvi and D. Berley and E. Bernardini and A. Bernhard and D. Z. Besson and G. Binder and D. Bindig and E. Blaufuss and S. Blot and C. Bohm and M. Börner and F. Bos and D. Bose and S. Böser and O. Botner and J. Braun and L. Brayeur and H. -P. Bretz and S. Bron and A. Burgman and T. Carver and M. Casier and E. Cheung and D. Chirkin and A. Christov and K. Clark and L. Classen and S. Coenders and G. H. Collin and J. M. Conrad and D. F. Cowen and R. Cross and M. Day and J. P. A. M. de André and C. De Clercq and E. del Pino Rosendo and H. Dembinski and S. De Ridder and P. Desiati and K. D. de Vries and G. de Wasseige and M. de With and T. DeYoung and J. C. Díaz-Vélez and V. di Lorenzo and H. Dujmovic and J. P. Dumm and M. Dunkman and B. Eberhardt and T. Ehrhardt and B. Eichmann and P. Eller and S. Euler and P. A. Evenson and S. Fahey and A. R. Fazely and J. Feintzeig and J. Felde and K. Filimonov and C. Finley and S. Flis and C. -C. Fösig and A. Franckowiak and E. Friedman and T. Fuchs and T. K. Gaisser and J. Gallagher and L. Gerhardt and K. Ghorbani and W. Giang and L. Gladstone and T. Glauch and T. Glüsenkamp and A. Goldschmidt and J. G. Gonzalez and D. Grant and Z. Griffith and C. Haack and A. Hallgren and F. Halzen and E. Hansen and T. Hansmann and K. Hanson and D. Hebecker and D. Heereman and K. Helbing and R. Hellauer and S. Hickford and J. Hignight and G. C. Hill and K. D. Hoffman and R. Hoffmann and K. Hoshina and F. Huang and M. Huber and K. Hultqvist and S. In and A. Ishihara and E. Jacobi and G. S. Japaridze and M. Jeong and K. Jero and B. J. P. Jones and W. Kang and A. Kappes and T. Karg and A. Karle and U. Katz and M. Kauer and A. Keivani and J. L. Kelley and A. Kheirandish and J. Kim and M. Kim and T. Kintscher and J. Kiryluk and T. Kittler and S. R. Klein and G. Kohnen and R. Koirala and H. Kolanoski and R. Konietz and L. Köpke and C. Kopper and S. Kopper and D. J. Koskinen and M. Kowalski and K. Krings and M. Kroll and G. Krückl and C. Krüger and J. Kunnen and S. Kunwar and N. Kurahashi and T. Kuwabara and M. Labare and J. L. Lanfranchi and M. J. Larson and F. Lauber and D. Lennarz and M. Lesiak-Bzdak and M. Leuermann and L. Lu and J. Lünemann and J. Madsen and G. Maggi and K. B. M. Mahn and S. Mancina and M. Mandelartz and R. Maruyama and K. Mase and R. Maunu and F. McNally and K. Meagher and M. Medici and M. Meier and T. Menne and G. Merino and T. Meures and S. Miarecki and T. Montaruli and M. Moulai and R. Nahnhauer and U. Naumann and G. Neer and H. Niederhausen and S. C. Nowicki and D. R. Nygren and A. Obertacke Pollmann and A. Olivas and A. O'Murchadha and T. Palczewski and H. Pandya and D. V. Pankova and P. Peiffer and Ö. Penek and J. A. Pepper and C. Pérez de los Heros and D. Pieloth and E. Pinat and P. B. Price and G. T. Przybylski and M. Quinnan and C. Raab and L. Rädel and M. Rameez and K. Rawlins and R. Reimann and B. Relethford and M. Relich and E. Resconi and W. Rhode and M. Richman and B. Riedel and S. Robertson and M. Rongen and C. Rott and T. Ruhe and D. Ryckbosch and D. Rysewyk and L. Sabbatini and S. E. Sanchez Herrera and A. Sandrock and J. Sandroos and S. Sarkar and K. Satalecka and P. Schlunder and T. Schmidt and S. Schoenen and S. Schöneberg and L. Schumacher and D. Seckel and S. Seunarine and D. Soldin and M. Song and G. M. Spiczak and C. Spiering and J. Stachurska and T. Stanev and A. Stasik and J. Stettner and A. Steuer and T. Stezelberger and R. G. Stokstad and A. Stößl and R. Ström and N. L. Strotjohann and G. W. Sullivan and M. Sutherland and H. Taavola and I. Taboada and J. Tatar and F. Tenholt and S. Ter-Antonyan and A. Terliuk and G. Tešić and S. Tilav and P. A. Toale and M. N. Tobin and S. Toscano and D. Tosi and M. Tselengidou and C. F. Tung and A. Turcati and E. Unger and M. Usner and J. Vandenbroucke and N. van Eijndhoven and S. Vanheule and M. van Rossem and J. van Santen and M. Vehring and M. Voge and E. Vogel and M. Vraeghe and C. Walck and A. Wallace and M. Wallraff and N. Wandkowsky and A. Waza and Ch. Weaver and M. J. Weiss and C. Wendt and S. Westerhoff and B. J. Whelan and S. Wickmann and K. Wiebe and C. H. Wiebusch and L. Wille and D. R. Williams and L. Wills and M. Wolf and T. R. Wood and E. Woolsey and K. Woschnagg and D. L. Xu and X. W. Xu and Y. Xu and J. P. Yanez and G. Yodh and S. Yoshida and M. Zoll},
journal= {arXiv preprint arXiv:1701.03731},
year = {2019}
}
Comments
Review article, to appear in Advances in Space Research, special issue "Origins of Cosmic Rays"