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Energy budget in the high energy universe : proceedings of the International Workshop, Kashiwa, Japan, 22-24 February 2006 / editors, Katsuhiko Sato, Junji Hisano.

By: Contributor(s): Material type: TextTextPublication details: Hackensack, NJ : World Scientific, ©2007.Description: 1 online resource (xii, 398 pages) : illustrationsContent type:
  • text
Media type:
  • computer
Carrier type:
  • online resource
ISBN:
  • 9789812708342
  • 9812708340
Subject(s): Genre/Form: Additional physical formats: Print version:: Energy budget in the high energy universe.DDC classification:
  • 539.7/223 22
LOC classification:
  • QC485 .I64 2006eb
Online resources:
Contents:
Preface; CONTENTS; Highest Energy Universe; Around the Knee; GeV Sky; TeV Sky; MeV and keV Sky; Special Lecture; Contributions; Scientific Program.
Summary: The existence of materials with very high specific energies greatly exceeding the local virial temperature is best represented by cosmic rays, whose origin has long been a mystery. Recent astrophysical observations in X-ray, gamma-ray, neutrino, and high energy cosmic ray experiments, in conjunction with theoretical studies, have revealed various new aspects of the high energy universe, including promising candidates for cosmic ray acceleration sites. As each approach has its own advantages and limitations, it is expected that joint efforts by experimentalists and theorists in various related.
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"The International Workshop on Energy Budget in the High Energy Universe was held February 22-24 at Institute of Cosmic Ray Research, Kashiwa campus of the University of Tokyo. This workshop in fourth in the series of international workshops of the 21th century COE program 'Quantum Extreme Systems and their Symmetries' of the University of Tokyo."--Preface

Includes bibliographical references.

Print version record.

Preface; CONTENTS; Highest Energy Universe; Around the Knee; GeV Sky; TeV Sky; MeV and keV Sky; Special Lecture; Contributions; Scientific Program.

The existence of materials with very high specific energies greatly exceeding the local virial temperature is best represented by cosmic rays, whose origin has long been a mystery. Recent astrophysical observations in X-ray, gamma-ray, neutrino, and high energy cosmic ray experiments, in conjunction with theoretical studies, have revealed various new aspects of the high energy universe, including promising candidates for cosmic ray acceleration sites. As each approach has its own advantages and limitations, it is expected that joint efforts by experimentalists and theorists in various related.

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