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String theory is a leading candidate for the unification of universal forces and matter, and one of its most striking predictions is the existence of small additional dimensions that have escaped detection so far. This book focuses on the geometry of these dimensions, beginning with the basics of the theory, the mathematical properties of spinors, and differential geometry. It further explores advanced techniques at the core of current research, such as G-structures and generalized complex geometry. Many significant classes of solutions to the theory's equations are studied in detail, from special holonomy and Sasaki–Einstein manifolds to their more recent generalizations involving fluxes for form fields. Various explicit examples are discussed, of interest to graduates and researchers.
Chapter 2 contains the problem statements of the 150 problems in general relativity theory. The chapter is divided into 12 sections with problems organized by different topics defined by the keywords in the section headings.
Chapter 1 contains the problem statements of the 150 problems in special relativity theory. The chapter is divided into nine sections with problems organized by different topics defined by the keywords in the section headings.
Chapter 3 contains the complete and elaborated solutions to all 300 problems stated and described in Chapters 1 and 2, respectively. The idea to present the solutions in a separate chapter is to help the reader to avoid the temptation of peeking at the solutions too soon.
The introductory chapter describes the notation, concepts, and conventions in relativity theory that is used in this problem book. The main purpose of this chapter is to help the reader to relate to the notation and conventions used in textbooks at hand.
Einstein's theories of special relativity and general relativity form a core part of today's undergraduate (or Masters-level) physics curriculum. This is a supplementary problem book or student's manual, consisting of 150 problems in each of special and general relativity. The problems, which have been developed, tested and refined by the authors over the past two decades, are a mixture of short-form and multi-part extended problems, with hints provided where appropriate. Complete solutions are elaborated for every problem, in a different section of the book; some solutions include brief discussions on their physical or historical significance. Designed as a companion text to complement a main relativity textbook, it does not assume access to any specific textbook. This is a helpful resource for advanced students, for self-study, a source of problems for university teaching assistants, or as inspiration for instructors and examiners constructing problems for their lectures, homework or exams.