Titlebook: Astronomy, Cosmology and Fundamental Physics; Proceedings of the E Peter A. Shaver,Luigi DiLella,Alvaro Giménez Conference proceedings 2003

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1431-2433 tes, evidence for neutrino oscillations, space experiments on fundamental physics, and discoveries of extrasolar planets. This book will be useful for researchers and graduate students who wish to have a broad overview of the current developments in these fields..978-3-642-07281-9978-3-540-44851-8Series ISSN 1431-2433 Series E-ISSN 1611-6143

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Holger J. Schmidt,Carsten Baumgarthnts, both on the ground and in space, gives fascinating prospects also for observational cosmology and astroparticle physics. Through realistically possible further observational developments at high mountain altitudes a rapid extension of the field is to be expected.

歌唱隊

Charlotte Heyder,Isabelle Hillebrandteutrinos from MeV to EeV energy by a variety of mechanisms. The important conclusion is that, independently of the specific blueprint of the source, it takes a kilometer-scale neutrino observatory to detect the neutrino beam associated with the highest energy cosmic rays and gamma rays. The technology for commissioning such instruments exists.

行乞

Astrophysics with High Energy Gamma Rays,nts, both on the ground and in space, gives fascinating prospects also for observational cosmology and astroparticle physics. Through realistically possible further observational developments at high mountain altitudes a rapid extension of the field is to be expected.

領(lǐng)帶

High-Energy Neutrinos from Cosmic Rays,eutrinos from MeV to EeV energy by a variety of mechanisms. The important conclusion is that, independently of the specific blueprint of the source, it takes a kilometer-scale neutrino observatory to detect the neutrino beam associated with the highest energy cosmic rays and gamma rays. The technology for commissioning such instruments exists.

GEAR

鎮(zhèn)痛劑

Co-creation: Building brands togetherthat it requires scalar fields with extremely flat potentials or four-form fields coupled to branes with an extremely small charge. Some recent suggestions are reviewed on how such features can arise in particle physics models.

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Nina De Cleir,Inga Schmidt-Rossicles, such as neutrinos, or other unknown particles like the axion or the supersymmetric LSP version of the Weakly Interacting Massive Particles (WIMPs)? If WIMPs are the Dark Matter in the Galaxy, how can they be detected? This paper briefly reviews the current status of some searches for this dark component of the Universe.

別炫耀