- 1. A brief review of general relativity -- 2. A kinetic-theory description of fluids -- 3. Relativistic perfect fluids -- 4. Linear and nonlinear hydrodynamic waves -- 5. Reaction fronts: detonations and deflagrations -- 6. Relativistic non-perfect fluids -- 7. Formulations of the Einstein-Euler equations -- 8. Numerical relativistic hydrodynamics: finite-difference methods -- 9. Numerical relativistic hydrodynamics: HRSC methods -- 10. Numerical relativistic hydrodynamics: high-order methods -- 11. Relativistic hydrodynamics of non-selfgravitating fluids -- 12. Relativistic hydrodynamics of selfgravitating fluids -- Appendix A. Geometrised system of units -- Appendix B. Notable thermodynamic expressions -- Appendix C. Notable tensors -- Appendix D. Common practices in numerical relativistic hydrodynamics -- Appendix E. Numerical building blocks.
- Relativistic hydrodynamics is a very successful theoretical framework to describe the dynamics of matter from scales as small as those of colliding elementary particles, up to the largest scales in the universe. This book provides an up-to-date, lively, and approachable introduction to the mathematical formalism, numerical techniques, and applications of relativistic hydrodynamics. The topic is typically covered either by very formal or by very phenomenological books, but is instead presented here in a form that will be appreciated both by students and researchers in the field. The topics covered in the book are the results of work carried out over the last 40 years, which can be found in rather technical research articles with dissimilar notations and styles. The book is not just a collection of scattered information, but a well-organized description of relativistic hydrodynamics, from the basic principles of statistical kinetic theory, down to the technical aspects of numerical methods devised for the solution of the equations, and over to the applications in modern physics and astrophysics. Numerous figures, diagrams, and a variety of exercises aid the material in the book. The most obvious applications of this work range from astrophysics (black holes, neutron stars, gamma-ray bursts, and active galaxies) to cosmology (early-universe hydrodynamics and phase transitions) and particle physics (heavy-ion collisions). It is often said that fluids are either seen as solutions of partial differential equations or as "wet". Fluids in this book are definitely wet, but the mathematical beauty of differential equations is not washed out. Readership: Graduate and post-graduate students, professors, lecturers, and researchers in astrophysics, particle physics, and applied mathematics. The specification in this catalogue, including without limitation price, format, extent, number of illustrations, and month of publication, was as accurate as possible at the time the catalogue was compiled. Occasionally, due to the nature of some contractual restrictions, we are unable to ship a specific product to a particular territory. Jacket images are provisional and liable to change before publication.
- Bibliography Note:
- Includes bibliographical references (pages -720) and index.
- Source of Acquisition:
- Purchased with funds from the James and Joyce Gettys Libraries Endowment in the Math Library and in the School of Information Sciences and Technology; 2014.
- Endowment Note:
- James and Joyce Gettys Libraries Endowment in the Math Library and in the School of Information Sciences and Technology
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