Rudolf Kippenhahn, Alfred Weigert

Stellar Structure and Evolution (eBook, PDF)

• Format: PDF

Produktbeschreibung

The attempt to understand the physics of the structure of stars and their change in time - their evolution - has been bothering many physicists and astronomers ever since the last century. This long chain of successful research is well documented not only by numerous papers in the corresponding journals but also by a series of books. Some of them are so excellently written that despite their age they can still be recommended, and not only as documents of the state of the art at that time. A few outstanding examples are the books of R. Emden (1907), A. S. Eddington (1926), S. Chandrasekhar (1939), and M. Schwarzschild (1958). But our science has rapidly expanded in the last few decades, and new aspects have emerged which could not even be anticipated, say, 30 years ago and which today have to be carefully explored. This does not mean, however, that our ambition is to present a complete account of the latest and most refined numerical results. This can well be left to the large and growing number of excellent review articles. The present book is intended rather to be a textbook that will help students and teachers to understand these results as far as possible and present them in a simple and clear manner. We know how difficult this is since we ourselves have tried for the largest part of our scientific career to understand "how the stars work" - and then to make others believe it.

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Produktdetails

• Verlag: Springer Berlin Heidelberg
• Seitenzahl: 468
• Erscheinungstermin: 6. Dezember 2012
• Englisch
• ISBN-13: 9783642615238
• Artikelnr.: 53396383

Autorenporträt

Rudolf Kippenhahn is author of very successful academic astronomy books as well of a large number of best-selling popular science books on astronomy, atomic physics and cryptology. From 1965-1975 he was professor for astronomy and astrophysics in Göttingen, Germany, and from 1975-1991 he was the director of the Max-Planck Institute for Astrophysics in Garching. He has received several medals and awards including the Eddington medal by the Royal Astronomical Society and the Karl-Schwarzschild medal of the Astronomische Gesellschaft. Alfred Weigert was professor for astrophysics at the University of Hamburg, Germany. His research forcussed on the simulation of stellar evolution and on the solution of the set of equations describing the structure of stars. He was not only Rudolf Kippenhahn's co-author of the first edition of Stellar Structure and Evolution, but also author (with Heinrich J. Wendker) of the successful German introductory textbook "Astronomie und Astrophysik". He died in 1992. Achim Weiss is an astrophysicist at the Max-Planck Instiute for Astrophysics in Garching and lecturer at the Ludwig-Maximilians University in Munich, Germany. Dr. Weiss' research interests are on stellar evolution of low- and intermediate mass stars, population synthesis and AGB- and post-AGB evolution.

Inhaltsangabe

Part I The Basic Equations.- 1 Coordinates, Mass Distribution, and Gravitational Field in Spherical Stars.- 2 Conservation of Momentum.- 3 The Virial Theorem.- 4 Conservation of Energy.- 5 Transport of Energy by Radiation and Conduction.- 6 Stability Against Local, Non-spherical Perturbations.- 7 Transport of Energy by Convection.- 8 The Chemical Composition.- 9 Mass Loss.- Part II The Overall Problem.- 10 The Differential Equations of Stellar Evolution.- 11 Boundary Conditions.- 12 Numerical Procedure.- Part III Properties of Stellar Matter.- 13 The Perfect Gas with Radiation.- 14 Ionization.- 15 The Degenerate Electron Gas.- 16 The Equation of State of Stellar Matter.- 17 Opacity.- 18 Nuclear Energy Production.- Part IV Simple Stellar Models.- 19 Polytropic Gaseous Spheres.- 20 Homology Relations.- 21 Simple Models in the U-V Plane.- 22 The Zero Age Main-Sequence.- 23 Other Main-Sequences.- 24 The Hayashi Line.- 25 Stability Considerations.- Part V Early Stellar Evolution.- 26 The Onset of Star Formation.- 27 The Formation of Protostars.- 28 Pre-Main-Sequence Contraction.- 29 From the Initial to the Present Sun.- 30 Evolution on the Main-Sequence.- Part VI Post-Main-Sequence Evolution.- 31 Evolution Through Helium Burning - Intermediate-Mass Stars.- 32 Evolution Through Helium Burning - Massive Stars.- 33 Evolution Through Helium Burning - Low-Mass Stars.- Part VII Late Phases of Stellar Evolution.- 34 Evolution on the Asymptotic Giant Branch.- 35 Later Phases of Core Evolution.- 36 Final Explosions and Collapse.- Part VIII Compact Objects.- 37 White Dwarfs.- 38 Neutron Stars.- 39 Black Holes.- Part IX Pulsating Stars.- 40 Adiabatic Spherical Pulsations.- 41 Non-adiabatic Spherical Pulsations.- 42 Non-radial Stellar Oscillations.- Part X Stellar Rotation.- 43 The Mechanics of Rotating Stellar Models.- 44 The Thermodynamics of Rotating Stellar Models.- 45 The Angular-Velocity Distribution in Stars.- References.- Index.

Rezensionen

From the reviews of the second edition: "There is an enormous amount of physics and astronomy in this second edition, more ... than a typical first-year-graduate class, or instructor, can master in a semester. Some of the material cannot easily be found in other books ... . Certainly, anyone planning to teach the subject should have the book ... ." (Virginia Trimble, The Observatory, Vol. 133 (1233), April, 2013)