Titlebook: Neutrinos and Explosive Events in the Universe; Maurice M. Shapiro,Todor Stanev,John P. Wefel Conference proceedings 2005 Springer Science

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978-1-4020-3747-4Springer Science+Business Media B.V. 2005

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Neutrinos and Explosive Events in the Universe978-1-4020-3748-1Series ISSN 1568-2609

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FLIRT

時(shí)代錯(cuò)誤

On Dynamics of Relativistic Shock Waves with Losses in Gamma-Ray Burst Sources the shock front or distributed in the downstream medium. It is shown that there are two qualitatively different regimes of shock deceleration, corresponding to small and large losses. We present the temperature, pressure and density distributions in the downstream fluid as well as Lorentz factor as a function of distance from the shock front.

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First Results From the H.E.S.S. Cherenkov Telescope System in Namibia100 GeV to 10 TeV energy range located in Namibia on 1835m a.s.l.. Each telescope is equipped with a 107m. mirror and a high resolution camera build out of 960 photomultipliers. This article reports on first results on the Crab Nebula, the supernova remnant SN 1006, the galactic center and the active galactic nucleus (AGN) PKS 2155-304.

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Surgeon

Humble

Outstanding Problems in Particle Astrophysicsenergy cosmic rays (UHECR) as well as sources of high-energy photons? Are GRBs and/or AGNs also sources of high-energy neutrinos? If there are indeed particles with energies greater than the cutoff expected from propagation through the microwave background radiation, what are their sources? The purp

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