This book is a survey of methods used in the study of two-dimensional models in quantum field theory as well as applications of these theories in physics. It covers the subject since the first model, studied in the fifties, up to modern developments in string theories, and includes exact solutions, non-perturbative methods of study, and nonlinear sigma models.
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The development of Relativistic Quantum Field Theory started in 1932 as a natural extension of Quantum Mechanics to the relativistic domain1. The work of Feynman in the late forties provided a powerful tool for the calculation of processes in Quantum Electrodynamics2. Second quantization led, however to new conceptual and technical difficulties. Quantum fields had to be regarded as operator-valued distributions, their local products being ill defined as a result of ultraviolet divergencies, which plagued the higher order computations in perturbation theory. This problem was partially mastered via the techniques of renormalization3,4, and later on completely understood5,6…
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Two dimensional quantum field theory provides a very powerful laboratory for gaining a non perturbative understanding of quantum field theory. The kinematical simplifications resulting from two dimensional space time have allowed for the complete solution of a variety of models involving interacting fields. The non trivial nature of these solutions provide a deeper insight into the structure of quantum field theory, and has found useful applications in several areas of research, such as string theories and systems in statistical mechanics at criticality…
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