Open Access
| Issue |
EPJ Web of Conferences
Volume 53, 2013
UHECR 2012 - International Symposium on Future Directions in UHECR Physics
|
|
|---|---|---|
| Article Number | 06004 | |
| Number of page(s) | 7 | |
| Section | Cosmic Ray Sources and Propagation | |
| DOI | https://doi.org/10.1051/epjconf/20135306004 | |
| Published online | 25 June 2013 | |
- G. Giacinti, M. Kachelrieß, D. V. Semikoz and G. Sigl, JCAP 1008 (2010) 036 [NASA ADS] [CrossRef] [Google Scholar]
- G. Giacinti, M. Kachelrieß, D. V. Semikoz and G. Sigl, Astropart. Phys. 35 (2011) 192 [CrossRef] [Google Scholar]
- P. Sokolsky, PoS ICHEP 2010 (2010) 444 [Google Scholar]
- Y. Tsunesada [for the Telescope Array Collaboration], “Highlights from Telescope Array,” arXiv:1111.2507 [astro-ph.HE] [Google Scholar]
- J. Abraham et al. [Pierre Auger Observatory Collaboration], Phys. Rev. Lett. 104 (2010) 091101 [NASA ADS] [CrossRef] [MathSciNet] [PubMed] [Google Scholar]
- P. Facal et al. [for the Pierre Auger Collaboration], “The Pierre Auger Observatory II: Studies of Cosmic Ray Composition and Hadronic Interaction models,” arXiv:1107.4804 [astro-ph.HE] [Google Scholar]
- A. V. Glushkov, I. T. Makarov, M. I. Pravdin, I. E. Sleptsov, D. S. Gorbunov, G. I. Rubtsov, S.V. Troitsky, JETP Lett. 87 (2008) 190 [CrossRef] [Google Scholar]
- D. Harari, S. Mollerach and E. Roulet, JHEP 9908 (1999) 022 [Google Scholar]
- D. Harari, S. Mollerach and E. Roulet, JHEP 0010 (2000) 047 [CrossRef] [Google Scholar]
- D. Harari, S. Mollerach and E. Roulet, JHEP 0002 (2000) 035 [Google Scholar]
- H. Takami and K. Sato, Astrophys. J. 724 (2010) 1456 [CrossRef] [Google Scholar]
- S. Vorobiov et al., Nucl. Phys. Proc. Suppl. 196 (2009) 203 [CrossRef] [Google Scholar]
- G. Golup, D. Harari, S. Mollerach and E. Roulet, JCAP 1107 (2011) 006 [CrossRef] [Google Scholar]
- R. -Y. Liu, X. -Y. Wang, W. Wang and A. M. Taylor, Astrophys. J. 755 (2012) 139 [NASA ADS] [CrossRef] [Google Scholar]
- M. Prouza and R. Smida, Astron. Astrophys. 410 (2003) 1 [CrossRef] [EDP Sciences] [Google Scholar]
- M. Kachelrieß, P. D. Serpico and M. Teshima, Astropart. Phys. 26 (2006) 378 [Google Scholar]
- X. H. Sun, W. Reich, A. Waelkens and T. Enslin, Astron. Astrophys. 477 (2008) 573 [CrossRef] [EDP Sciences] [Google Scholar]
- M. S. Pshirkov, P. G. Tinyakov, P. P. Kronberg and K. J. Newton-McGee, Astrophys. J. 738 (2011) 192 [Google Scholar]
- R. Jansson and G. R. Farrar Astrophys. J. 757 (2012) 14 [Google Scholar]
- D. De Marco, P. Blasi and T. Stanev, JCAP 0706 (2007) 027 [Google Scholar]
- G. Giacinti, M. Kachelriess, D. V. Semikoz and G. Sigl, JCAP 1207 (2012) 031 [Google Scholar]
- G. Giacinti, X. Derkx and D. V. Semikoz, JCAP 1003 (2010) 022 [NASA ADS] [CrossRef] [Google Scholar]
- K. Kotera and A. V. Olinto, Ann. Rev. Astron. Astrophys. 49 (2011) 119 [Google Scholar]
- K. Dolag, D. Grasso, V. Springel and I. Tkachev, JETP Lett. 79 (2004) 583 [CrossRef] [Google Scholar]
- [Pisma Zh. Eksp. Teor. Fiz. 79 (2004) 719] [Google Scholar]
- K. Dolag, D. Grasso, V. Springel and I. Tkachev, JCAP 0501 (2005) 009 [NASA ADS] [CrossRef] [Google Scholar]
- G. Sigl, F. Miniati and T. A. Ensslin, Phys. Rev. D 70 (2004) 043007 [NASA ADS] [CrossRef] [Google Scholar]
- G. Sigl, F. Miniati and T. Ensslin, Nucl. Phys. Proc. Suppl. 136 (2004) 224 [Google Scholar]
- G. Golup, D. Harari, S. Mollerach and E. Roulet, Astropart. Phys. 32 (2009) 269 [NASA ADS] [CrossRef] [Google Scholar]
- B. M. Gaensler, R. Beck and L. Feretti, New Astron. Rev. 48 (2004) 1003 [Google Scholar]
- R. Beck and B. M. Gaensler, New Astron. Rev. 48 (2004) 1289 [Google Scholar]
- G. Giacinti and D. V. Semikoz, Phys. Rev. D 83 (2011) 083002 [CrossRef] [Google Scholar]
Current usage metrics show cumulative count of Article Views (full-text article views including HTML views, PDF and ePub downloads, according to the available data) and Abstracts Views on Vision4Press platform.
Data correspond to usage on the plateform after 2015. The current usage metrics is available 48-96 hours after online publication and is updated daily on week days.
Initial download of the metrics may take a while.