Neutrinos: the key to ultrahigh energy cosmic rays
Observations of ultrahigh energy cosmic rays (UHECR) do not uniquely determine both the
injection spectrum and the evolution model for UHECR sources—primarily because …
injection spectrum and the evolution model for UHECR sources—primarily because …
Neutrinos: The Key to UHE cosmic rays
D Seckel, T Stanev - Phys. Rev. Lett., 2005 - inspirehep.net
Observations of ultrahigh energy cosmic rays (UHECR) do not uniquely determine both the
injection spectrum and the evolution model for UHECR sources-primarily because …
injection spectrum and the evolution model for UHECR sources-primarily because …
Neutrinos: the Key to UHE Cosmic Rays
D Seckel, T Stanev - arXiv preprint astro-ph/0502244, 2005 - arxiv.org
Observations of ultrahigh energy cosmic rays (UHECR) do not uniquely determine both the
injection spectrum and the evolution model for UHECR sources-primarily because …
injection spectrum and the evolution model for UHECR sources-primarily because …
Neutrinos: The Key to Ultrahigh Energy Cosmic Rays
D Seckel, T Stanev - Physical Review Letters, 2005 - ui.adsabs.harvard.edu
Observations of ultrahigh energy cosmic rays (UHECR) do not uniquely determine both the
injection spectrum and the evolution model for UHECR sources—primarily because …
injection spectrum and the evolution model for UHECR sources—primarily because …
[引用][C] Neutrinos: The key to ultrahigh energy cosmic rays
D SECKEL, T STANEV - Physical review letters, 2005 - pascal-francis.inist.fr
Neutrinos: The key to ultrahigh energy cosmic rays CNRS Inist Pascal-Francis CNRS
Pascal and Francis Bibliographic Databases Simple search Advanced search Search by …
Pascal and Francis Bibliographic Databases Simple search Advanced search Search by …
[PDF][PDF] Neutrinos: The Key to Ultrahigh Energy Cosmic Rays
D Seckel, T Stanev - 2005 - scholar.archive.org
Observations of ultrahigh energy cosmic rays (UHECR) do not uniquely determine both the
injection spectrum and the evolution model for UHECR sources—primarily because …
injection spectrum and the evolution model for UHECR sources—primarily because …
Neutrinos: The Key to Ultrahigh Energy Cosmic Rays
D Seckel, T Stanev - Physical Review Letters, 2005 - osti.gov
Observations of ultrahigh energy cosmic rays (UHECR) do not uniquely determine both the
injection spectrum and the evolution model for UHECR sources-primarily because …
injection spectrum and the evolution model for UHECR sources-primarily because …
Neutrinos: the key to ultrahigh energy cosmic rays
D Seckel, T Stanev - Physical review letters, 2005 - pubmed.ncbi.nlm.nih.gov
Observations of ultrahigh energy cosmic rays (UHECR) do not uniquely determine both the
injection spectrum and the evolution model for UHECR sources--primarily because …
injection spectrum and the evolution model for UHECR sources--primarily because …
Neutrinos: The Key to Ultrahigh Energy Cosmic Rays
D Seckel, T Stanev - Physical Review Letters, 2005 - inis.iaea.org
[en] Observations of ultrahigh energy cosmic rays (UHECR) do not uniquely determine both
the injection spectrum and the evolution model for UHECR sources-primarily because …
the injection spectrum and the evolution model for UHECR sources-primarily because …
Neutrinos: the key to ultrahigh energy cosmic rays.
D Seckel, T Stanev - Physical Review Letters, 2005 - europepmc.org
Observations of ultrahigh energy cosmic rays (UHECR) do not uniquely determine both the
injection spectrum and the evolution model for UHECR sources--primarily because …
injection spectrum and the evolution model for UHECR sources--primarily because …