دسترسی نامحدود
برای کاربرانی که ثبت نام کرده اند
برای ارتباط با ما می توانید از طریق شماره موبایل زیر از طریق تماس و پیامک با ما در ارتباط باشید
در صورت عدم پاسخ گویی از طریق پیامک با پشتیبان در ارتباط باشید
برای کاربرانی که ثبت نام کرده اند
درصورت عدم همخوانی توضیحات با کتاب
از ساعت 7 صبح تا 10 شب
ویرایش:
نویسندگان: Hendrik J. van Eerten
سری:
ISBN (شابک) : 9780367557775, 9781003095088
ناشر: CRC Press
سال نشر: 2024
تعداد صفحات: 326
زبان: English
فرمت فایل : PDF (درصورت درخواست کاربر به PDF، EPUB یا AZW3 تبدیل می شود)
حجم فایل: 14 مگابایت
در صورت تبدیل فایل کتاب Introduction to Fluid Dynamics in Physics and Astrophysics به فرمت های PDF، EPUB، AZW3، MOBI و یا DJVU می توانید به پشتیبان اطلاع دهید تا فایل مورد نظر را تبدیل نمایند.
توجه داشته باشید کتاب مقدمه ای بر دینامیک سیالات در فیزیک و اخترفیزیک نسخه زبان اصلی می باشد و کتاب ترجمه شده به فارسی نمی باشد. وبسایت اینترنشنال لایبرری ارائه دهنده کتاب های زبان اصلی می باشد و هیچ گونه کتاب ترجمه شده یا نوشته شده به فارسی را ارائه نمی دهد.
Cover Half Title Title Page Copyright Page Contents Preface Chapter 1: Preliminaries 1.1. Vectors and Their Bases 1.1.1. Matrix Notation 1.1.2. Limitations of Matrix Notation 1.1.3. The Cross-Product and Coordinate Transformations 1.1.4. Gradient, Divergence and Curl 1.1.5. Gradient, Divergence, Curl and Integration 1.1.6. Divergence, Curl and Curvilinear Coordinates 1.2. Index Notation 1.2.1. The Cross Product and Index Notation 1.2.2. Four-vectors, Indices and (Square) Brackets 1.3. Covariant Components and the Dual Basis 1.4. Partial and Full Differentiation 1.4.1. Exact Differentials 1.4.2. Inexact Differentials Chapter 2: The Conservation Laws of Fluid Dynamics 2.1. A Derivation of the Conservation Laws 2.1.1. Mass Conservation: The Continuity Equation 2.1.2. Sneak Peek at Full Set of Euler’s Equations 2.1.3. Derivation of the Momentum Equation 2.1.4. Derivation of the Energy Equation 2.2. Fluid Dynamics and the Continuum Approximation 2.2.1. The Continuum Approximation and the Mean Free Path 2.3. Energy Transport in Atmospheres and Other Fluids 2.4. Boltzmann’s Equation and Fluid Dynamics 2.4.1. The Continuity Equation 2.4.2. The Momentum Equation 2.4.3. Equations of State Chapter 3: Lagrangian Fluid Dynamics 3.1. Fluid Parcels 3.2. Derivation of Conservation Laws in a Lagrangian Approach 3.2.1. Example: Stellar Wind 3.3. Mass Coordinates 3.4. Polytropic Processes and Thermodynamics 3.4.1. The Polytropic Exponent of a Gas Dominated by Radiation Pressure Chapter 4: Hydrostatics, Atmospheres and Stellar Structure 4.1. Hydrostatics of a Plane-Parallel Atmosphere 4.2. An Isothermal Slab Model 4.2.1. Some Quick Notes on Gravity 4.2.2. General Isothermal Slab Density Profiles 4.3. Idealized Stellar Structure Models 4.3.1. Isothermal Spheres 4.3.2. Polytropic Stellar Structure Models 4.3.3. The Physics of Polytropes 4.4. Stellar Structure Modelling Using Mass Coordinates Chapter 5: Sound Waves and Sub-/supersonic Flow 5.1. The Wave Nature of Sound 5.2. Acoustic Waves 5.2.1. Wave Packets and Fourier Analysis 5.2.2. The Energy of an Acoustic Sound Wave 5.2.3. Spherical Acoustic Waves 5.3. Sound Waves in a Gravitational Field Chapter 6: Properties and Kinematics of Fluid Flow 6.1. An Overview of Terminology 6.2. Streamlines, Streaklines and Path Lines 6.3. Flow Lines of an Incompressible Fluid 6.4. Bernoulli’s Equation 6.5. The de Laval Nozzle 6.6. Vorticity 6.7. Potential Flow, Irrotational Flow and Incompressible Flow Chapter 7: Shock Waves 7.1. The Shock-Jump Conditions 7.2. Compression Shocks, Rarefaction Waves and Contact Discontinuities 7.3. The Entropy Change Across a Shock 7.4. Blast Waves 7.5. Self-Similar Explosions 7.6. First-Order Fermi Acceleration Across Strong Shocks Chapter 8: Fluid Dynamics in Special Relativity 8.1. Core Concepts in Special Relativity 8.1.1. Four-Dimensional Spacetime 8.1.2. Point Particles 8.2. Special Relativistic Fluid Dynamical Equations 8.2.1. The Continuity Equation 8.2.2. Conservation of Energy-Momentum 8.3. The Microphysics of Relativistic Gases 8.4. Relativistic Shocks 8.4.1. Strong Shocks 8.5. Relativistic Blast Waves 8.6. Self-Similar Relativistic Explosions 8.7. First-Order Fermi Shock-Acceleration Revisited Chapter 9: Viscous Flow 9.1. The Navier-Stokes Equation 9.1.1. Angular Momentum and the Stress Tensor 9.1.2. Bulk Viscosity 9.1.3. Shear Viscosity 9.2. Viscosity and Dissipation 9.3. Physical Interpretation of Shear Viscosity 9.4. Flow Through a Pipe 9.5. Two Example Similarity Parameters in Viscous Flows 9.5.1. The Reynold’s Number 9.5.2. The Prandtl Number Chapter 10: Fluid Instabilities 10.1. Convection and Stability 10.2. The Rayleigh-Taylor Instability 10.3. The Kelvin-Helmholtz Instability 10.4. Gravitational Instability 10.5. Thermal Instability 10.6. Homogeneous and Isotropic Turbulence Chapter 11: Accretion Flow 11.1. Accretion as a Source of Energy in Astrophysics 11.2. Bondi Accretion 11.2.1. The Sonic Point 11.2.2. The Bondi Accretion Rate 11.3. The Eddington Luminosity 11.4. Accretion Discs 11.4.1. Thin Discs 11.4.2. Accretion Discs and Viscosity Chapter 12: Concepts in Plasma Physics 12.1. Introduction 12.2. Incorporating Maxwell’s Equations 12.2.1. The Magnetic Field Equation 12.2.2. The Equations of Magnetohydrodynamics 12.3. The Nature of Plasmas 12.4. Field Freezing 12.5. Magnetohydrodynamic Waves 12.6. Two Example Similarity Parameters in Plasma Physics Chapter 13: Computational Fluid Dynamics 13.1. Euler’s Equations in Terms of a State Vector Equation 13.2. Rudimentary Finite Difference Schemes 13.3. Stability, Accuracy and Diffusion 13.3.1. Stability 13.3.2. Accuracy 13.3.3. Diffusion and Dispersion 13.3.4. Lax-Friedrichs & Lax-Wendroff 13.4. Boundary Conditions 13.5. Finite Volume Methods 13.5.1. FDM vs FVM 13.5.2. Basic Finite Volume Methods 13.5.3. Working Code 13.5.4. The HLL Method and Godunov Approach 13.5.5. Wave Speed Estimates 13.5.6. The HLLC Method 13.6. Higher Order in Time and Space 13.6.1. Higher Order in Space 13.6.2. Higher Order in Time 13.7. Alternatives and Extensions to the Finite Volume Approach 13.7.1. Adapting the Fixed Mesh 13.7.2. Arbitrary Lagrangian-Eulerian Methods 13.7.3. Smoothed Particle Hydrodynamics 13.7.4. Finite Element Methods 13.8. Computational Hydrodynamics and Special Relativity Appendix A: Concepts from Thermodynamics A.1. The First and Second Law of Thermodynamics A.2. Legendre Transforms A.3. Heat Capacities A.4. The Ideal Gas Law and Perfect Gases A.5. The Energy Equation in Stellar Structure Modelling Appendix B: Vector Identities and Derivatives B.1. Vector Product Rules B.2. Higher-Order Derivatives B.3. Dot and Cross-Product Combinations B.4. Spherical Coordinates B.5. Cylindrical Coordinates Appendix C: Euler’s Equations in Non-Cartesian Coordinate Systems C.1. Cylindrical Coordinates C.2. Spherical Coordinates Appendix D: List of Symbols Appendix E: Abbreviated Answers to Selected Problems References Index