The aim of the Conference is to present and discuss some of the most relevant theoretical and experimental results in the field of high energy cosmic rays. Special attention has been paid to the investigation of the various astrophysical sources, using photons, very high energy cosmic rays and neutrinos as probes (multi-messenger observations). The Conference has given the opportunity to collect experimental results; contributions from operating experiments (H.E.S.S., MAGIC, VERITAS, PAMELA, Auger, ARGO, ANTARES, Baikal, IceCube, LOPES, ANITA …). Experiments in progress and future projects (AGILE, GLAST, NEMO, NESTOR, KM3NeT, Telescope Array, ASHRA, TUNKA, ...) have been discussed, debating on the different features and on sensitivities. Particular relevance has been given to examine the different source candidates (point sources, transient sources, diffuse flux sources …); comparison of models and discussions will be promoted.

RICAP'07, Roma International Conference on Astro-Particle physics / Capone, Antonio; Lucarelli, Fabrizio; M., De Vincenzi; A., Morselli. - In: NUCLEAR INSTRUMENTS & METHODS IN PHYSICS RESEARCH. SECTION A, ACCELERATORS, SPECTROMETERS, DETECTORS AND ASSOCIATED EQUIPMENT. - ISSN 0168-9002. - (2007). (Intervento presentato al convegno RICAP'07, Roma International Conference on Astro-Particle physics tenutosi a Università di Roma "La Sapienza" nel 20-22 giugno 2007).

RICAP'07, Roma International Conference on Astro-Particle physics

CAPONE, Antonio;LUCARELLI, FABRIZIO;
2007

Abstract

The aim of the Conference is to present and discuss some of the most relevant theoretical and experimental results in the field of high energy cosmic rays. Special attention has been paid to the investigation of the various astrophysical sources, using photons, very high energy cosmic rays and neutrinos as probes (multi-messenger observations). The Conference has given the opportunity to collect experimental results; contributions from operating experiments (H.E.S.S., MAGIC, VERITAS, PAMELA, Auger, ARGO, ANTARES, Baikal, IceCube, LOPES, ANITA …). Experiments in progress and future projects (AGILE, GLAST, NEMO, NESTOR, KM3NeT, Telescope Array, ASHRA, TUNKA, ...) have been discussed, debating on the different features and on sensitivities. Particular relevance has been given to examine the different source candidates (point sources, transient sources, diffuse flux sources …); comparison of models and discussions will be promoted.
2007
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Utilizza questo identificativo per citare o creare un link a questo documento: https://hdl.handle.net/11573/425661
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