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An Introduction to the Theory of Stellar Structure and Evolution, by Dina Prialnik
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Using fundamental physics, the theory of stellar structure and evolution can predict how stars are born, how their complex internal structure changes, what nuclear fuel they burn, and their ultimate fate. This textbook is a stimulating introduction for undergraduates in astronomy, physics and applied mathematics, taking a course on the physics of stars. It uniquely emphasizes the basic physical principles governing stellar structure and evolution. This second edition contains two new chapters on mass loss from stars and interacting binary stars, and new exercises. Clear and methodical, it explains the processes in simple terms, while maintaining mathematical rigor. Starting from general principles, this textbook leads students step-by-step to a global, comprehensive understanding of the subject. Fifty exercises and full solutions allow students to test their understanding. No prior knowledge of astronomy is required, and only a basic background in physics and mathematics is necessary.
- Sales Rank: #737018 in Books
- Brand: Brand: Cambridge University Press
- Published on: 2009-11-30
- Original language: English
- Number of items: 1
- Dimensions: 9.72" h x .79" w x 6.85" l, 1.80 pounds
- Binding: Hardcover
- 328 pages
- Used Book in Good Condition
Review
"The unique feature of this book is the emphasis it places, throughout, on the basic physical principles governing stellar evolution. The processes are always explained in the simplest terms, while maintaining full mathematical rigour ... This textbook provides a stimulating introduction for undergraduates in astronomy, physics, planetary science, and applied mathematics who are taking a course on the physics of stars. Because this book requires only basic undergraduate physics and mathematics and no prior knowledge of astronomy it may be read by advanced amateurs as well." - Orion
"Here we have a first-class textbook that spells out in a clear and methodical way the principles that underlie the life cycles of stars and the physics of their interiors. ... The host of student exercises in this book, plus the useful worked answers, ensure that any dedicated physics or mathematics undergraduate can, with some effort, understand what is going on." - David Hughes, New Scientist
"To my mind, this is the first book to be both a candidate for the title of classic and at the same time suitable for undergraduates ... The approach is very different from that of most textbooks on stars ... Throughout the book, the emphasis is on understanding physical principles, and there are well-designed exercises scattered through the text, relating to material that has just been covered; full solutions are clearly set out in an appendix ... This ... is a book that I can strongly recommend as a suitable textbook to anyone teaching a course in stellar structure, at advanced undergraduate or beginning graduate level ... Any undergraduate who masters this book will not only be well prepared to undertake graduate work in the area but will also understand his/her other physics courses better. An excellent book, which certainly deserves to become a classic." - Robert Connon Smith, The Observatory
About the Author
Dina Prialnik is a Professor of Planetary Physics at Tel Aviv University. Her research interests lie in stellar evolution; the structure and evolution of cataclysmic variables, comet nuclei and other small Solar System bodies; and the evolution of planets.
Most helpful customer reviews
8 of 8 people found the following review helpful.
Exactly what the title of the book suggests
By copper
The distinguishing characteristic of this text is its clarity of language. Prialnik's chief gift is her ability to convey complex ideas clearly without neglecting their mathematical basis. There is a very fine line between a full-blown graduate text (intended for future PhD's) and an introductory undergraduate text (intended for non-science majors), and this book walks it superbly. Most other books lie squarely in one camp or the other, which can be frustrating for those seeking an intermediate treatment. The ideal audience for this book is the junior or senior undergraduate who is familiar with calculus and differential equations, thermodynamics, and statistical mechanics, and has a strong interest in astronomy. The more complex physics and mathematics, including the details of nuclear chemistry and particle physics and the numerical solution of non-linear differential equations, is treated on a take-it-or-leave-it basis, without the kind of rigorous derivations that would bog down a middle-of-the-road text. A student properly equipped will come out of the experience with a fine introduction to the theory of stellar structure and evolution, exactly what the title promises.
The text is not perfect, however. Because a large portion of it is devoted to the differential equations governing stellar structure and evolution (not surprisingly), students familiar with numerical methods may be frustrated by Prialnik's sometimes qualitative treatment. Towards the end of the book, the more intricate aspects of stellar structure and evolution (which arise in the numerical solutions to these equations) are presented in a purely descriptive fashion. Like trying to describe a graph rather than simply reproducing it on the page, Prialnik's descriptive approach is meandering at best, and confusing at worst. A much more compelling treatment would have been some kind of interactive numerical solution, either on a CD or the publisher's website. (As an aside, I very much appreciated Prialnik's attempts to relate theory to observation throughout, especially the inclusion of numerically calculated HR diagrams accompanying real ones.) One other feature lacking in this text is a brief appendix giving the meaning of all symbols used in the book, and where appropriate, numerical values. Considering Prialnik has generously provided fully explained solutions to each problem, this is a somewhat surprising omission.
8 of 8 people found the following review helpful.
Excellent book for beginners
By C. Bradley
A truly excellent introductory book. It has worked problems at the back and actually has an index that allows you to find anything you need for reference. I actually used this book more than Padmanabhan's books for my graduate course, because Prialnik explains things very well.
This book should be the basis of any undergraduate stellar astrophysics course.
8 of 8 people found the following review helpful.
Nice book that cover a lot of topics
By Tomas
This is a nice book that covers a lot of astrophysical concepts. The level of detail is fair for a first introduction into the subject and the style is easy to follow. However, the different topics are introduced one after the other without a clear motivation. This makes the book a bit confusing.
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