Classical Mathematical Physics Dynamical Systems and Field Theories

Classical Mathematical Physics Dynamical Systems and Field Theories by Walter Thirring is a comprehensive volume published by Springer Science & Business Media on October 17, 2003. This 3rd edition spans 543 pages and is presented in English. The book combines the enlarged and corrected editions of Thirring’s renowned course in mathematical physics, focusing on classical physics and its applications in various scientific fields.
Readers will find a detailed exploration of classical dynamical systems, utilizing analysis on manifolds to discuss Hamiltonian systems, canonical transformations, and perturbation theory. The text includes numerous examples and remarks, making it suitable for students in physics, mathematics, and applied mathematics. Additionally, the treatment of classical fields employs differential geometry, covering Maxwell’s and Einstein’s equations, and includes discussions on electromagnetic fields and gauge theories. The book also addresses solutions to the Einstein equations and their implications for astrophysical phenomena, such as the life and death of stars.
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This volume combines the enlarged and corrected editions of both volumes on classical physics of Thirring’s famous course in mathematical physics. With numerous examples and remarks accompanying the text, it is suitable as a textbook for students in physics, mathematics, and applied mathematics. The treatment of classical dynamical systems uses analysis on manifolds to provide the mathematical setting for discussions of Hamiltonian systems, canonical transformations, constants of motion, and pertubation theory. Problems discussed in considerable detail include: nonrelativistic motion of particles and systems, relativistic motion in electromagnetic and gravitational fields, and the structure of black holes. The treatment of classical fields uses the language of differenial geometry throughout, treating both Maxwell’s and Einstein’s equations in a compact and clear fashion. The book includes discussions of the electromagnetic field due to known charge distributions and in the presence of conductors as well as a new section on gauge theories. It discusses the solutions of the Einstein equations for maximally symmetric spaces and spaces with maximally symmetric submanifolds; it concludes by applying these results to the life and death of stars.
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