
Black holes present one of the most fascinating predictions of Einstein's general theory of relativity. There is strong evidence of their existence through observation of active galactic nuclei, including the centre of our galaxy, observations of gravitational waves, and others. There exists a large scientific literature on black holes, including many excellent textbooks at various levels. However, most of these steer clear from the mathematical niceties needed to make the theory of black holes a mathematical theory. Those which maintain a high mathematical standard are either focused on specific topics, or skip many details. The objective of this book is to fill this gap and present a detailed, mathematically oriented, extended introduction to the subject. The book provides a wide background to the current research on all mathematical aspects of the geometry of black hole spacetimes.
This text investigates the rigorous mathematical foundations of black hole spacetimes within the framework of Einstein's general theory of relativity. Piotr T. Chruściel, a specialist in mathematical physics, addresses the gap between introductory textbooks and highly specialized research monographs. The book provides a comprehensive, formal derivation of the geometric properties of black holes, utilizing advanced differential geometry and partial differential equations to establish a precise mathematical theory.
What You Will Find
Scope Limits
Experts recognize this work as a high-level reference for graduate students and researchers in mathematical physics. Readers frequently note the significant mathematical density of the prose, which requires a strong background in differential geometry and general relativity to navigate effectively.
Page Count:
416
Publication Date:
2020-01-01
Publisher:
OUP Oxford
ISBN-10:
019259754X
ISBN-13:
9780192597540
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