Numerical Relativity: Starting from Scratch
Numerical Relativity: Starting from Scratch
Stuart L. Shapiro, University of Illinois, Urbana-Champaign
Numerical relativity has emerged as the key tool to model gravitational waves - recently detected for the first time - that are emitted when black holes or neutron stars collide. This book provides a pedagogical, accessible, and concise introduction to the subject. Relying heavily on analogies with Newtonian gravity, scalar fields and electromagnetic fields, it introduces key concepts of numerical relativity in a context familiar to readers without prior expertise in general relativity. Readers can explore these concepts by working through numerous exercises, and can see them 'in action' by experimenting with the accompanying Python sample codes, and so develop familiarity with many techniques commonly employed by publicly available numerical relativity codes. This is an attractive, student-friendly resource for short courses on numerical relativity, as well as providing supplementary reading for courses on general relativity and computational physics.
- Includes numerous exercises, and answers to selected problems, allowing the reader to explore new concepts in depth, often through analytical examples that illustrate key features of numerical relativity
- Provides Python scripts exemplifying two types of simulations often encountered in numerical relativity, so that readers can perform 'hands-on' computational experiments with some of the new concepts
- Summary boxes highlighting key results, serving as easy-to-find references to important features
- Several appendices provide the reader with additional background information, as well as a summary of important general relativity tools and equations
Reviews & endorsements
'Computational general relativity has now become a central tool for the exploration of the astrophysical universe, and gravitational-wave astronomy would not be possible without it. A burgeoning or seasoned astrophysicist who wishes to be up to date must therefore acquire an awareness of the field's methods and main achievements. But where to begin? With this book! Baumgarte and Shapiro are leading experts (indeed, founding experts) of this field, and with their trademark lucid and engaging prose, they take us gently by the hand on a comprehensive guided tour. Mysterious notions (lapse, shift, extrinsic curvature, constraint equations) are introduced seamlessly, and the book features a gallery of the field's most important results to date. A superb achievement for the great benefit of the scientific community.' Eric Poisson, University of Guelph; author of A Relativist's Toolkit
'Numerical relativity well deserves its reputation as a subject of great beauty yet prodigious conceptual difficulty and daunting technical complexity. This outstanding text, by two leading practitioners of the field, is a wonderful Rosetta Stone for those seeking an efficient path toward a working knowledge of the subject. For me it will serve as an essential reference. I'm sorry only that it was not available sooner.' Robert Eisenstein, Massachusetts Institute of Technology
'This is an excellent book explaining the general relativistic two-body problem and its numerical treatment in a highly pedagogical manner to a broad scientific audience. Besides the main topic, readers will also gain some unexpected insight and new viewpoints on numerous wider aspects of Einstein's theory.' Ulrich Sperhake, University of Cambridge
'Black holes and gravitational waves are, thanks to new observations, fast-advancing frontiers of astronomy that attract wide interest. Their implications are best addressed by powerful computers, so this text, by two acknowledged world experts, is especially welcome and timely.' Martin Rees, Astronomer Royal; author of Gravity's Fatal Attraction
Product details
March 2021Adobe eBook Reader
9781108945936
0 pages
This ISBN is for an eBook version which is distributed on our behalf by a third party.
Table of Contents
- Preface
- 1. Newton's and Einstein's gravity
- 2. Foliations of spacetime: constraint and evolution equations
- 3. Solving the constraint equations
- 4 Solving the evolution equations
- 5. Numerical simulations of black-hole binaries
- Epilogue
- Appendix A. A brief review of tensor properties
- Appendix B. A brief introduction to some numerical techniques
- Appendix C. A very brief introduction to matter sources
- Appendix D. A summary of important results
- Appendix E. Answers to selected problems
- References
- Index.
