Numerical relativity has emerged as the key tool to model gravitational waves that are emitted when two black holes collide. This book provides a pedagogical, accessible and concise introduction to the subject for non-experts, acquainting them with the key concepts underlying publicly available numerical relativity codes.
Numerical relativity has emerged as the key tool to model gravitational waves that are emitted when two black holes collide. This book provides a pedagogical, accessible and concise introduction to the subject for non-experts, acquainting them with the key concepts underlying publicly available numerical relativity codes.Hinweis: Dieser Artikel kann nur an eine deutsche Lieferadresse ausgeliefert werden.
Thomas W. Baumgarte is the William R. Kenan Jr. Professor of Physics at Bowdoin College in Brunswick, Maine. His work in numerical relativity and relativistic astrophysics has been recognized with prizes and fellowships from the Guggenheim Foundation, the Humboldt Foundation, the American Physical Society, and the Simons Foundation. Stuart Shapiro and he have previously co-authored the graduate-level text Numerical Relativity: Solving Einstein's Equations on the Computer (Cambridge, 2010).
Inhaltsangabe
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.
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.
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