The cosmic radiation was discovered by Hess in 1912 but its origin is still the subject of much controversy and considerable study. For several decades most workers in the cosmic ray field were interested in the Nuclear Physical aspect of the particle beam and many important dis coveries were made, notably the identification of the positron, the muon, the pion and the strange particles. More recently however, em phasis has changed to the Astrophysical aspect both with re8ard to the origin of the radiation and to its relation with the other radiation fields. Mindful of the increasing importance of the Astrophysical facets of the subject the Cosmic Ray Commission of IUPAP approached the High Energy Astrophysics Commission of the IAU with the suggestion of a joint Symposium on Cosmic Ray Origin. The plan was to bring together workers in all the various astronomical fields - from Radio, through Optical to Gamma Rays - with Cosmic Ray physicists and to fully explore the various interrelations. The approach was received with enthusiasm and this book contains the proceedings of the ensuing Symposium, (styled IUPAP/ IAU Symposium No. 94) which was held in Bologna from 11th - 14th June 1980. Virtually all the papers presented are reproduced here. The Scientific Organizing Committee chose the invited speakers whose papers formed the major scientific component of the meeting. Additional short contributed papers were also called for and very brief 2-page resumes (which have not been refereed) are given in the proceedings.
This volume provides timely coverage of nonaccelerator astroparticle physics. It complements two volumes prepared for earlier schools. Informative and pedagogical, it can serve as the basis for a modern course on the subject.The first section discusses the fundamentals of particle physics, with reviews of the standard model and beyond. The section on neutrinos and neutrino oscillations covers topics including neutrino oscillations, short and long baseline neutrino beams from accelerators, atmospheric and solar neutrinos, neutrinos from gravitational stellar collapses and neutrino telescopes. Another section deals with dark matter searches. Cosmic rays and astrophysics are covered with reviews of experiments in space, extreme energy cosmic rays, and gamma ray bursts. Gravitational waves and gravitational wave detectors are discussed. The final section deals with results from accelerators and future plans for accelerator facilities, computing, and new large and small detectors. Abstracts of the posters presented by participants at the school give a broad picture of world-wide activities in the field.
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