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Physics and astrophysics of ultra-high-energy cosmic rays / M. Lemoine and G. Sigl, editors.

Colaborador(es): Tipo de material: TextoTextoIdioma: Inglés Series Lecture notes in physics ; 576.Fecha de copyright: Berlin ; New York : Springer, 2010Edición: First EditionDescripción: x, 327 pages : illustrations ; 25 cmISBN:
  • 3540428992 (acidfree paper)
  • 9783540428992
  • 9783642076848
  • 9783540456155
Tema(s): Clasificación CDD:
  • 539.7223 23
Clasificación LoC:
  • QC484.8 .P48 2001
Recursos en línea:
Contenidos parciales:
Phenomenology of Ultra-High-Energy Atmospheric Showers -- The Air Fluorescence Method -- for Measuring Extremely-High-Energy Cosmic Rays -- Fermi Acceleration of Astroparticles -- Rotation Powered Pulsars as Sources of High-Energy Particles -- High-Energy Particles from y-Ray Bursts -- Cosmic Magnetic Fields from the Perspective -- of Ultra-High-Energy Cosmic Rays Propagation -- A Possible Nearby Origin -- for the Highest-Energy Events Observed -- Propagation of Ultra-High-Energy Radiation -- Neutrino Cascades: -- The Byproducts of Propagation of Ultra-High-Energy Neutrinos -- Extreme-Energy Cosmic Rays: -- Hints to New Physics Beyond the Standard Model? -- Summary of the School: A Critical View on the Origin -- of the Ultra-High-Energy Cosmic Rays.
Resumen: The origin of the most energetic particles observed in nature is one of the major unresolved questions in modern astrophysics. Theoretical speculations range from electromagnetic acceleration in some unknown astrophysical source to as yet undiscovered particle physics beyond the Standard Model. These speculations have also lead to the development of new detection concepts and experimental projects, some of which are currently under construction. The present volume consists of a self-contained set of lectures which cover most of these aspects: from the speculative origins and the acceleration and propagation mechanisms to a discussion of the detection techniques. It emphasizes the strong interdisciplinarity of this topic and highlights the many open questions. This volume is intended for students entering this field and for professional astronomers and particle and theoretical physicists.
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Tipo de ítem Biblioteca actual Signatura Copia número Estado Fecha de vencimiento Código de barras Reserva de ítems
Colección general Colección general Biblioteca Yachay Tech 539.7223 P5785 2010 (Navegar estantería(Abre debajo)) Ej. 1 Disponible 005789
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Includes index.

Includes bibliographical references.

Phenomenology of Ultra-High-Energy Atmospheric Showers -- The Air Fluorescence Method -- for Measuring Extremely-High-Energy Cosmic Rays -- Fermi Acceleration of Astroparticles -- Rotation Powered Pulsars as Sources of High-Energy Particles -- High-Energy Particles from y-Ray Bursts -- Cosmic Magnetic Fields from the Perspective -- of Ultra-High-Energy Cosmic Rays Propagation -- A Possible Nearby Origin -- for the Highest-Energy Events Observed -- Propagation of Ultra-High-Energy Radiation -- Neutrino Cascades: -- The Byproducts of Propagation of Ultra-High-Energy Neutrinos -- Extreme-Energy Cosmic Rays: -- Hints to New Physics Beyond the Standard Model? -- Summary of the School: A Critical View on the Origin -- of the Ultra-High-Energy Cosmic Rays.

The origin of the most energetic particles observed in nature is one of the major unresolved questions in modern astrophysics. Theoretical speculations range from electromagnetic acceleration in some unknown astrophysical source to as yet undiscovered particle physics beyond the Standard Model. These speculations have also lead to the development of new detection concepts and experimental projects, some of which are currently under construction. The present volume consists of a self-contained set of lectures which cover most of these aspects: from the speculative origins and the acceleration and propagation mechanisms to a discussion of the detection techniques. It emphasizes the strong interdisciplinarity of this topic and highlights the many open questions. This volume is intended for students entering this field and for professional astronomers and particle and theoretical physicists.

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