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Hydrodynamic and Hydromagnetic Stability (Dover Books on Physics), by S. Chandrasekhar
Fee Download Hydrodynamic and Hydromagnetic Stability (Dover Books on Physics), by S. Chandrasekhar
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Dr. Chandrasekhar's book received high praise when it first appeared in 1961 as part of Oxford University Press' International Series of Monographs on Physics. Since then it has been reprinted numerous times in its expensive hardcover format. This first lower-priced, sturdy paperback edition will be welcomed by graduate physics students and scientists familiar with Dr. Chandrasekhar's work, particularly in light of the resurgence of interest in the Rayleigh-Bénard problem.
This book presents a most lucid introduction to the Rayleigh-Bénard problem: it has also been applauded for its thorough, clear coverage of the theory of instabilities causing convection.
Dr. Chandrasekhar considers most of the typical problems in hydromagnetic stability, with the exception of viscous shear flow; a specialized domain deserving a book unto itself. Contents include: Rotation; Stability of More General Flows; Bénard Problem; Gravitational Equilibrium and Instability; Stability of a Magnetic Field; Thermal Instability of a Layer of Fluid heated from Below; Rayleigh-Taylor Instability; Kelvin-Helmholtz Instability; and Onset of Thermal Instability in Fluid Spheres and Spherical Shells.
Each chapter is accompanied by a section of bibliographical notes: indexes locating definitions and theorems are also provided. Graduate students in theoretical and experimental physics, as well as physicists in diverse fields, will immediately remark upon the clear exposition, and be glad this book is now so readily available.
- Sales Rank: #1489897 in eBooks
- Published on: 2013-04-26
- Released on: 2013-04-26
- Format: Kindle eBook
About the Author
Subrahmanyan Chandrasekhar: A Shining Star
The great Indian astrophysicist Subrahmanyan Chandrasekhar (1910–1995), recipient of the Nobel Prize in Physics in 1983 for his work on the later evolutionary stages of massive stars, was not only the author of several books reprinted by Dover over many years, but a frequent and highly valued reviewer of titles in his field during the 1970s and 1980s. Chandrasekhar's books, published by Dover, are: An Introduction to the Theory of Stellar Structure, 1967; Hydrodynamic and Hydromagnetic Stability, 1981; Principles of Stellar Dynamics, 2005; Ellipsoidal Figures of Equilibrium, 1987; and Radiative Transfer, 1960.
For those concerned with the distant future ― the really distant future ― Chandrasekhar's name will always be associated with the Chandrasekhar Limit, the figure of 1.44 solar masses, the minimal mass above which a dying star will collapse into a black hole following a supernova. People on Earth need not be bothered anticipating such drama: for us, when the sun dies, the lights will just go out. In astrophysical terms, our sun will at that point be a stable white dwarf.
Critical Acclaim for Subrahmanyan Chandrasekhar:
"Any new fact or insight that I may have found has not seemed to me as a 'discovery' of mine, but rather something that had always been there and that I had chanced to pick up. I discovered true mathematical elegance from Subrahmanyan Chandrasekhar." ― Carl Sagan
Most helpful customer reviews
21 of 23 people found the following review helpful.
Most affordable of the classics on hydrodynamic stability
By stavka
This is one of the standard monographs on hydrodynamic instabilities, considered a classic. It was published by Oxford UP in 1961 and is kept in print (at a bargain price) by Dover. It is still very usable, easy to read, and an excellent introduction, although on some points it is out of date. For Rayleigh-Benard convection, a reader would do well to consult more recent books like Drazin & Reid, Swinney & Gollub, Koschmieder, and Getling. However, nobody covers the linear theory better than Chandrasekhar.
20 of 22 people found the following review helpful.
A practical, beautiful masterpiece
By A Customer
I first read this book just to better understand a small point in a fluid dynamics paper I was reading, but quickly realized it is an encyclopaedic masterpiece, and found myself reading more and more. Chandasekhar's explanations are clear, easily readable, and complete, and should be a model for other writers. Anyone working on fluids should own this.
5 of 10 people found the following review helpful.
A practical, beautiful masterpiece
By A Customer
I first read this book just to better understand a small point in a fluid dynamics paper I was reading, but quickly realized it is an encyclopaedic masterpiece, and found myself reading more and more. Chandasekhar's explanations are clear, easily readable, and complete, and should be a model for other writers. Anyone working on fluids should own this.
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