Titlebook: Special Problems in High Energy Physics; Proceedings of the V Paul Urban Conference proceedings 1967 Springer-Verlag Wien 1967 elementary p

词根词缀法

Algebraic Formulation of Dynamical Problems,or hadron physics [1]. By this extension, such a phenomenon as the nuclear anomalous magnetic moment found simple and elegant explanation, despite the expectation that these phenomena could only be understood in the frame of orthodox dynamical theory. This success encouraged the thought that a furth

figure

High Energy Scattering of Hadrons,ergy and small momentum transfers. By “high energy” we mean here the region .% MathType!MTEF!2!1!+-% feaagCart1ev2aaatCvAUfeBSjuyZL2yd9gzLbvyNv2CaerbuLwBLn% hiov2DGi1BTfMBaeXatLxBI9gBaerbd9wDYLwzYbItLDharqqtubsr% 4rNCHbGeaGqiVu0Je9sqqrpepC0xbbL8F4rqqrFfpeea0xe9Lq-Jc9% vqaqpepm0xbba9pwe9Q8fs0-yqaqpep

假设

CULP

Quantum Field Theory in de Sitter Space, the universe. One may have the feeling that cosmological changes of the space-time group will not change its microscopical consequences. On the other hand by contraction some important restrictions may be lost: going from the Poincaré group to the Galilei group the TCP — theorem or the connection b

moratorium

LAY

Constant

Leptonic Decays of the Kaon According to Current Algebra and PCAC,nn [1] and the assumption of a partially conserved axial vector current [2] (PCAC). For the most part this will be a review of the work of Callan and Treiman [3] and Weinberg [4], although some new results, obtained in collaboration with McNamee [5], will also be discussed. The presentation will lar

旧式步枪

Vector Mesons and the Electromagnetic Interactions of Hadrons,-GeV-region. I would like to discuss the question how this has improved our understanding of the electromagnetic (e.m.) interaction of the hadrons, i.e. of the strongly interacting particles. My procedure will be to consider several experimental results under the uniform aspect of a single model, th

演讲

摄取

Quantum Field Theory in de Sitter Space, theory works for systems invariant under the de Sitter group. We do not mean to imply that we consider as established that we live in a de Sitter space but rather consider two different models of space-time, both invariant under the de Sitter group, as interesting possible representations of our cosmos.