Titlebook: Electroweak Interactions; Heinrich Mitter Conference proceedings 1982 Springer-Verlag Wien 1982 Elektroschwache Wechselwirkung.Interaction

genesis

https://doi.org/10.1007/978-3-322-81536-1 be reviewed. Aspects of this topic include the neutrino oscillation solution to the solar neutrino problem, the missing mass problem in galaxy halos and galaxy clusters, galaxy formation and clustering, and radiative neutrino decay and the cosmic ultraviolet background radiation.

急性

Cervical-Spine

Introduction to Gauge Theories of Electro-Weak Interactions,d if not presumptuous to assert that all of particle physics can be described in terms of gauge theories. Today we speak of the standard gauge model of electromagnetic, weak and strong interactions. In this development, the way was undoubtedly led by the unification of weak and electromagnetic force

原始

The Electroweak Interaction in e+e- Annihilations,e operation of PETRA and PEP which provide values of s (= C.M. energy.) in excess of 1000 GeV.. Although it was clear from the outset that several years would be needed to collect enough data to make an accurate determination of the neutral current parameters, it was not long after PETRA had started

欢乐东方

The Cern Proton-Antiproton Collider,with accelerators. This gives a good chance to discover the weak bosons (W and Z boson), which mediate the weak forces, in the next coming years much before the new accelerators designed to study these bosons are built.

领袖气质

是他笨

Weak Decays of Open and Hidden Top,d b-completes the third weak isodoublet of quarks. Experimentally no signal for toponium has been found up to 37 GeV. Although this may be disappointing one hand, the perspectives to test new and interesting physics get increasingly exciting with increasing quarkonium mass. A variety of QCD predicti

NOCT

Electroweak Processes Beyond the Tree Approximation,ourses of Drs. Ecker and Wagner. Much work has been devoted recently to a careful analysis of the higher order corrections to the tree diagram relations on which the experimental tests of the standard model of electroweak interactions are based. The subject seems by now mature for a clear and reason

Gourmet

Neutrino Masses, Neutrino Oscillations, and Cosmological Implications, searches for masses and oscillations is summarized. This includes a discussion of the solar neutrino problem, reactor, deep mine and accelerator data, tritium decay experiments and double beta-decay data. Finally, the cosmological implications and astrophysical data relating to neutrino masses will

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CP-Nonconservation,sful in accounting for a very wide range of data on these interactions. Consequently, in these lectures concerning CP-nonconservation in the weak interactions, we shall work entirely within the framework of this model, since this is the most economical approach until such time as this framework may