The 1992 Cargese Summer Institute on Quantitative Particle Physics was organized by the Universite Pierre et Marie Curie, Paris (M. Levy and J. -L. Basdevant), CERN (M. Jacob), the Ecole Normale Superieure, Paris (J. Diopoulos), the Katholieke Universiteit te Leuven (R. Gastmans) and the Universite Catholique de Louvain (J-M. Gerard), which, since 1975, have joined their efforts and worked in common. It was the tenth Summer Institute on High Energy Physics organized jointly at Cargese by these three universities. The 1992 School centered on quantitative tests of the Standard Model for electroweak and strong interactions. First, Professor T. D. Lee reviewed the fascinating history of weak interactions. Professor R. Barbieri then discussed the implications of the of LEP presented by Professor Foil. Professor G. Ecker latest experimental results described in detail the interplay between electroweak and strong interactions at low energy. Professors K. Berkelman and J-M. Gerard stressed the necessity to study the effects of CP-violation in both B-and K-physics. The first results of the HERA machine were presented by Professor G. Wolf, while Professor M. Shochet reviewed heavy flavor physics in hadron collider experiments. Recent non-accelerator experiments in neutrino physics were presented by Professor B. Barish. Finally, Professor M. Turner reviewed Cosmology after COBE. We owe many thanks to all those who have made this Summer Institute possible! Special thanks are due to the Scientific Committee of NATO and its President for a generous grant.
Lévy / Basdevant / Gérard
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Weitere Infos & Material
History of Weak Interactions.- Physics at LEP.- Electroweak Precision Tests: What do we Learn?.- Chiral Perturbation Theory.- CP- and T- Violations in the Standard Model.- Heavy Flavor Physics.- Physics at HERA.- Physics with Hadron Colliders.- Neutrino Physics.- Inflation After COBE: Lectures on Inflationary Cosmology.- Oblique Electroweak Parameters and Additional Fermion Generations.- Electroweak Symmetry Breaking from the Top.- Higgs Mass Limits from Electroweak Baryogenesis.- Carbon 60.
