Skip to product information
Modern Fluid Dynamics for Physics and Astrophysics (2016)

Modern Fluid Dynamics for Physics and Astrophysics

$119.99
Shipping calculated at checkout.
  • Authorized Dealer
  • Ships within 1 business day
  • Free 30-Day Returns
  • Secure Checkout via Shopify Payments
Details

"Modern Fluid Dynamics for Physics and Astrophysics" by Oded Regev, Orkan Umurhan, Philip Yecko is a mathematics book and learning resource focused on General Astronomy. Best for teachers, students, and readers looking for stronger mathematical understanding.

This book grew out of the need to attain a good command of modern fluid dynamics, as the majority of the bodies in the universe are made of fluids. By “modern” we mean that relatively recent discoveries, methods and techniques are included. For example, new ideas on transition to turbulence (via transiently growing stable linear modes and perhaps linear, or non-linear, secondary instabilities), new approaches to turbulence (which, however, still remains, despite intensive research efforts, to be the enigma of fluid dynamics), the use of asymptotic approximation methods, which can give analytical or semi-analytical results and complement fully numerical treatments. We also briefly discuss some important considerations, to be taken into account when one develops a numerical code in an attempt to simulate astrophysical flows on a computer (an ever increasing modern practice). Another special feature of this book is the focus of the text on fluid dynamics, per se. The astrophysics is mainly given in the examples and exercises. We believe that a good and broad command of fluid dynamics can be more fruitful in approaching outstanding astrophysical problems than a review of known classical problems. It is assumed that the students are mathematically equipped with a reasonable knowledge in analysis, including basics of ordinary and partial differential equations a good command of vector calculus and linear algebra. Each chapter is concluded by a “Bibliographical note,” in which we discuss briefly and cite the essential literature used and give recommendations for further, deeper reading. In an effort to make this book useful as a course textbook we have included in each chapter a number of exercises, most (but not all) of them on problems relevant to astrophysics.

Materials + Care

We prioritize quality in selecting the materials for our items, choosing premium fabrics and finishings that ensure durability, comfort, and timeless appeal.

Shipping + Returns

We strive to process and ship all orders in a timely manner, working diligently to ensure that your items are on their way to you as soon as possible.

Best For: Students and researchers in physics and astrophysics seeking to understand fluid dynamics.
Focus: Modern fluid dynamics with recent discoveries, methods, and techniques relevant to physics and astrophysics.
Covers: Transition to turbulence, transiently growing stable linear modes, and approaches to turbulence.
Why It Matters: Most celestial bodies are composed of fluids, making fluid dynamics essential for understanding their behavior in astrophysical contexts.

"Modern Fluid Dynamics for Physics and Astrophysics" by Oded Regev, Orkan Umurhan, Philip Yecko is a mathematics book and learning resource focused on General Astronomy. Best for teachers, students, and readers looking for stronger mathematical understanding.

Topic: General Astronomy

Author: Oded Regev, Orkan Umurhan, Philip Yecko

Who this is for:

  • Teachers and classroom instructors
  • Students building subject mastery
  • Readers looking for practical learning support

Why this book matters: It stands out as a practical math resource that helps explain concepts, strengthen problem-solving, and support classroom or independent learning.

This book grew out of the need to attain a good command of modern fluid dynamics, as the majority of the bodies in the universe are made of fluids. By “modern” we mean that relatively recent discoveries, methods and techniques are included. For example, new ideas on transition to turbulence (via transiently growing stable linear modes and perhaps linear, or non-linear, secondary instabilities), new approaches to turbulence (which, however, still remains, despite intensive research efforts, to be the enigma of fluid dynamics), the use of asymptotic approximation methods, which can give analytical or semi-analytical results and complement fully numerical treatments. We also briefly discuss some important considerations, to be taken into account when one develops a numerical code in an attempt to simulate astrophysical flows on a computer (an ever increasing modern practice). Another special feature of this book is the focus of the text on fluid dynamics, per se. The astrophysics is mainly given in the examples and exercises. We believe that a good and broad command of fluid dynamics can be more fruitful in approaching outstanding astrophysical problems than a review of known classical problems. It is assumed that the students are mathematically equipped with a reasonable knowledge in analysis, including basics of ordinary and partial differential equations a good command of vector calculus and linear algebra. Each chapter is concluded by a “Bibliographical note,” in which we discuss briefly and cite the essential literature used and give recommendations for further, deeper reading. In an effort to make this book useful as a course textbook we have included in each chapter a number of exercises, most (but not all) of them on problems relevant to astrophysics.

AuthorOded Regev, Orkan Umurhan, Philip Yecko
PublisherSpringer
Published2016-03-02
ISBN-139781493931637
BindingHardcover
Pages680
LanguageEnglish
SubjectsScience
TopicGeneral Astronomy
SeriesGraduate Texts in Physics

Format: Hardcover

Length: 680 pages

Language: English

Shop by collection

You might also like...