Titlebook: Masses of Fundamental Particles; Cargèse 1996 Maurice Lévy,Jean Iliopoulos,Jean-Marc Gérard Book 1997 Springer Science+Business Media New Y

哺乳動(dòng)物

暫時(shí)中止

Top Quark Mass,some ideas about how it might arise. After a brief introduction to the pattern of masses and couplings of quarks and leptons and an overview of the top quark’s properties, we discuss in Section 2 the role of the top quark in mixing processes, such as particle-antiparticle mixing in the neutral kaon

集中營(yíng)

Heavy-Quark Masses,c, model-independent description of the properties and decays of hadrons containing a heavy quark. I discuss the applications of these concepts to spectroscopy and to the weak decays of . mesons..Despite the title of my lectures, I will have to say little about the numerical values of heavy-quark ma

數(shù)量

東西

Lepton Universality,n universality are reviewed, both for the charged and neutral current sectors. Our knowledge about the Lorentz structure of the .% MathType!MTEF!2!1!+-% feaagCart1ev2aaatCvAUfeBSjuyZL2yd9gzLbvyNv2CaerbuLwBLn% hiov2DGi1BTfMBaeXatLxBI9gBaerbd9wDYLwzYbItLDharqqtubsr% 4rNCHbWexLMBbXgBd9gzLbvyNv2CaeHbl7m

FLORA

CHIDE

觀察

Neutrino Mass Models with an Abelian Family Symmetry,on masses remains unexplained in the Standard Model and most of its extensions, the question of whether the neutrinos are massive or not is still open. On the theoretical side, since neutrino masses are not protected by any fundamental symmetry., there is no reason to expect them to be zero. Now, if

Dorsal

Dark Matter,fty years ago, and it remains largely unresolved. We have learnt much about its distribution in the universe, yet remain abysmally ignorant as to its nature. These lectures will address two questions: where is the dark matter, and what is its nature? In the first lecture, I will, after reviewing the

Bureaucracy