Relativistische Hydrodynamik, Rezzolla, Luciano, Zanotti, Olindo, 9780198807599-

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Relativistic Hydrodynamics, Rezzolla, Luciano,Zanotti, Olindo, 9780198807599
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ISBN
9780198807599
Kategorie

Über dieses Produkt

Product Identifiers

Publisher
Oxford University Press, Incorporated
ISBN-10
0198807597
ISBN-13
9780198807599
eBay Product ID (ePID)
240111949

Product Key Features

Number of Pages
752 Pages
Language
English
Publication Name
Relativistic Hydrodynamics
Publication Year
2018
Subject
Physics / Relativity, Physics / General
Type
Textbook
Subject Area
Science
Author
Luciano Rezzolla, Olindo Zanotti
Format
Trade Paperback

Dimensions

Item Height
1.4 in
Item Weight
49.4 Oz
Item Length
9.7 in
Item Width
6.7 in

Additional Product Features

Intended Audience
Scholarly & Professional
Dewey Edition
23
Reviews
Relativistic hydrodynamics is an essential tool for astrophysicists and cosmologists in their quest to understand the universe. For many years, they have needed a modern text that introduces the subject pedagogically, and carries the reader to the level of maturity required for modern research. This book, at last, fills this need, and it does so superbly. It is likely to be the definitive book on the subject for many years to come.
Illustrated
Yes
Dewey Decimal
532.05
Table Of Content
Part I The Physics of Relativistic Hydrodynamics1. A Brief Review of General Relativity2. A Kinetic-Theory Description of Fluids3. Relativistic Perfect Fluids4. Linear and Nonlinear Hydrodynamical Waves5. Reaction Fronts: Detonations and Deflagrations6. Relativistic Non-Perfect FluidsPart II Numerical Relativistic Hydrodynamics7. Formulations of the Einstein-Euler Equations8. Numerical Relativistic-Hydrodynamics: Finite-Difference Methods9. Numerical Relativistic-Hydrodynamics: HRSC Methods10. Numerical Relativistic-Hydrodynamics: High-Order MethodsPart III Applications of Relativistic Hydrodynamics11. Relativistic Hydrodynamics of Non-Selfgravitating Fluids12. Relativistic Hydrodynamics of Selfgravitating FluidsAppendix A: Geometrized System of UnitsAppendix B: Notable Thermodynamical ExpressionsAppendix C: Notable TensorsAppendix D: Common Practices in Numerical Relativistic HydrodynamicsAppendix E: Numerical Building Blocks
Synopsis
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., 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., 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 presented here in a form which will be appreciated both by students and researchers in the field., 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.
LC Classification Number
QA912

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