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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.
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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.
Produktdetails
- Produktdetails
- Verlag: Oxford University Press
- Seitenzahl: 760
- Erscheinungstermin: 14. Juni 2018
- Englisch
- Abmessung: 241mm x 170mm x 38mm
- Gewicht: 1397g
- ISBN-13: 9780198807599
- ISBN-10: 0198807597
- Artikelnr.: 48135257
- Herstellerkennzeichnung
- Libri GmbH
- Europaallee 1
- 36244 Bad Hersfeld
- gpsr@libri.de
- Verlag: Oxford University Press
- Seitenzahl: 760
- Erscheinungstermin: 14. Juni 2018
- Englisch
- Abmessung: 241mm x 170mm x 38mm
- Gewicht: 1397g
- ISBN-13: 9780198807599
- ISBN-10: 0198807597
- Artikelnr.: 48135257
- Herstellerkennzeichnung
- Libri GmbH
- Europaallee 1
- 36244 Bad Hersfeld
- gpsr@libri.de
Luciano Rezzolla received his PhD in Astrophysics in 1997 at International School for Advanced Studies (SISSA) in Trieste. After being a Research Associate at the University of Illinois at Urbana-Champaign, he returned to SISSA in 1999 as Associate Professor and Director of the Computing Centre. From 2006 to 2013 he joined the Albert Einstein Institute in Potsdam (Max-Planck Institute for gravitational physics) as the Head of the Numerical-Relativity Research. Since 2013 he is Chair of Theoretical Relativistic Astrophysics at the Institute of Theoretical Physics in Frankfurt. He has worked in several areas of relativistic hydrodynamics and relativistic astrophysics, ranging from the investigation of fundamental issues to the construction of advanced numerical codes for the simulation of sources of gravitational waves. Olindo Zanotti received his PhD is Astrophysics in 2002 at the International School for Advanced Studies (SISSA) in Trieste. Since then he has worked as Research Associate at the University of Valencia (Spain), at the University of Florence (Italy), at the Notre Dame University (USA), and at the Albert Einstein Institute (Germany). His specific interests include accretion-disc physics, plasma physics, and numerical methods for the solution of hyperbolic equations. He carried out research at the University of Trento.
Part I The Physics of Relativistic Hydrodynamics
1: A Brief Review of General Relativity
2: A Kinetic-Theory Description of Fluids
3: Relativistic Perfect Fluids
4: Linear and Nonlinear Hydrodynamical Waves
5: Reaction Fronts: Detonations and Deflagrations
6: Relativistic Non-Perfect Fluids
Part II Numerical Relativistic Hydrodynamics
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
Part III Applications of Relativistic Hydrodynamics
11: Relativistic Hydrodynamics of Non-Selfgravitating Fluids
12: Relativistic Hydrodynamics of Selfgravitating Fluids
Appendix A: Geometrized System of Units
Appendix B: Notable Thermodynamical Expressions
Appendix C: Notable Tensors
Appendix D: Common Practices in Numerical Relativistic Hydrodynamics
Appendix E: Numerical Building Blocks
1: A Brief Review of General Relativity
2: A Kinetic-Theory Description of Fluids
3: Relativistic Perfect Fluids
4: Linear and Nonlinear Hydrodynamical Waves
5: Reaction Fronts: Detonations and Deflagrations
6: Relativistic Non-Perfect Fluids
Part II Numerical Relativistic Hydrodynamics
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
Part III Applications of Relativistic Hydrodynamics
11: Relativistic Hydrodynamics of Non-Selfgravitating Fluids
12: Relativistic Hydrodynamics of Selfgravitating Fluids
Appendix A: Geometrized System of Units
Appendix B: Notable Thermodynamical Expressions
Appendix C: Notable Tensors
Appendix D: Common Practices in Numerical Relativistic Hydrodynamics
Appendix E: Numerical Building Blocks
Part I The Physics of Relativistic Hydrodynamics
1: A Brief Review of General Relativity
2: A Kinetic-Theory Description of Fluids
3: Relativistic Perfect Fluids
4: Linear and Nonlinear Hydrodynamical Waves
5: Reaction Fronts: Detonations and Deflagrations
6: Relativistic Non-Perfect Fluids
Part II Numerical Relativistic Hydrodynamics
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
Part III Applications of Relativistic Hydrodynamics
11: Relativistic Hydrodynamics of Non-Selfgravitating Fluids
12: Relativistic Hydrodynamics of Selfgravitating Fluids
Appendix A: Geometrized System of Units
Appendix B: Notable Thermodynamical Expressions
Appendix C: Notable Tensors
Appendix D: Common Practices in Numerical Relativistic Hydrodynamics
Appendix E: Numerical Building Blocks
1: A Brief Review of General Relativity
2: A Kinetic-Theory Description of Fluids
3: Relativistic Perfect Fluids
4: Linear and Nonlinear Hydrodynamical Waves
5: Reaction Fronts: Detonations and Deflagrations
6: Relativistic Non-Perfect Fluids
Part II Numerical Relativistic Hydrodynamics
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
Part III Applications of Relativistic Hydrodynamics
11: Relativistic Hydrodynamics of Non-Selfgravitating Fluids
12: Relativistic Hydrodynamics of Selfgravitating Fluids
Appendix A: Geometrized System of Units
Appendix B: Notable Thermodynamical Expressions
Appendix C: Notable Tensors
Appendix D: Common Practices in Numerical Relativistic Hydrodynamics
Appendix E: Numerical Building Blocks







