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The science of statistical mechanics is concerned with defining the thermodynamic properties of a macroscopic sample in terms of the properties of the microscopic systems of which it is composed. This book provides a clear, logical, and self-contained treatment of equilibrium statistical mechanics.
Our understanding of the physical world was revolutionized in the twentieth century the era of "modern physics." The book Introduction to Modern Physics: Theoretical Foundations, aimed at the very best students, presents the foundations and frontiers of today's physics. Typically, students have to wade through several courses to see many of these topics. The goal is to give them some idea of where they were going, and how things fit together, as they go along. The book focuses on the following topics: quantum mechanics; applications in atomic, nuclear, particle, and condensed-matter physics; special relativity; relativistic quantum mechanics, including the Dirac equation and Feynman diagrams; quantum fields; and general relativity. The aim is to cover these topics in sufficient depth that things "make sense" to students, and they achieve an elementary working knowledge of them. The book assumes a one-year, calculus-based freshman physics course, along with a one-year course in calculus. Several appendices bring the reader up to speed on any additional required mathematics. Many problems are included, a great number of which take dedicated readers just as far as they want to go in modern physics. The present book provides solutions to the over 175 problems in Introduction to Modern Physics: Theoretical Foundations in what we believe to be a clear and concise fashion.
Our understanding of the physical world was revolutionized in the twentieth century - the era of modern physics. This book, aimed at the very best students, extends the coverage of the theoretical groundwork of today's physics presented in the previous volume: "Introduction to Modern Physics: Theoretical Foundations (Vol I)".
A working knowledge of Einstein's theory of general relativity is an essential tool for every physicist. This book serves as an introductory text on the subject aimed at first-year graduate students, or advanced undergraduates, in physics.
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