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9780387200897

Stellar Interiors

by ; ;
  • ISBN13:

    9780387200897

  • ISBN10:

    0387200894

  • Edition: 2nd
  • Format: Hardcover
  • Copyright: 2004-02-26
  • Publisher: Springer Verlag
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Supplemental Materials

What is included with this book?

Summary

This text, designed for beginning students of stellar physics, introduces the fundamentals of stellar structure and evolution. In emphasizing the general picture of the life cycles of stars and the physics responsible, it also allows prospective specialists a taste of many of the detailed aspects of this mature discipline. The authors develop a solid foundation in important theory that is often overlooked in typical courses, yet steer clear of extraneous intensive mathematics and physics. Topics include nuclear physics and stellar energy sources, the equation of state of stellar material, phenomenological approaches to convection, and modern numerical techniques for computation of stellar evolution. Keeping pace with recent developments, the authors incorporate important elements such as asteroseismology, and the effects of rotation and magnetic fields.The text contains the source code for two useful programs, ZAMS (for constructing chemically homogeneous zero-age main sequence models) and PULS (to study the seismological properties of the ZAMS models). Some chapters include exercises. The diskette can be used on any computer with a FORTRAN compiler.

Author Biography

Carl J. Hansen is Professor Emeritus of Astrophysical and Planetary Sciences and Fellow Adjoint of JILA, at the University of Colorado, Boulder.

Table of Contents

1 Preliminaries 1(42)
1.1 Hydrostatic Equilibrium
2(1)
1.2 An Energy Principle
3(4)
1.3 The Vinal Theorem and Its Applications
7(9)
1.3.1 Application: Global Energetics
10(1)
1.3.2 Application: The Kelvin-Helmholtz Time Scale
11(2)
1.3.3 Application: A Dynamic Time Scale
13(1)
1.3.4 Application: Estimates of Stellar Temperatures
13(1)
1.3.5 Application: Another Dynamic Time Scale
14(2)
1.4 The Constant-Density Model
16(5)
1.4.1 Calculation of Molecular Weights
17(4)
1.4.2 The Temperature Distribution
21(1)
1.5 Energy Generation and Transport
21(3)
1.6 Stellar Dimensional Analysis
24(6)
1.7 Evolutionary Lifetimes on the Main Sequence
30(1)
1.8 The Hertzsprung-Russell Diagram
30(2)
1.9 Summary Remarks
32(1)
1.10 Exercises
33(5)
1.11 References and Suggested Readings
38(5)
2 An Overview of Stellar Evolution 43(102)
2.1 Young Stellar Objects (YSOs)
44(3)
2.2 The Zero-Age Main Sequence (ZAMS)
47(4)
2.2.1 Life on the Main Sequence
48(2)
2.2.2 Brown Dwarfs
50(1)
2.3 Leaving the Main Sequence
51(9)
2.3.1 Cluster HR Diagrams
54(3)
Cluster and Galactics Ages
56(1)
2.3.2 Mass Loss From Massive Stars
57(3)
2.4 Red Giants and Supergiants
60(2)
2.5 Hellum Flash or Fizzle
62(8)
2.5.1 Hellum Core Burning
65(2)
Hellum Core Exhaustion
66(1)
2.5.2 Asymptotic Giant Branch
67(3)
2.6 Later Phases, Initial Masses M less than 6-10 Mo 69
2.6.1 A Bit About White Dwarfs
70(3)
2.7 Advanced Phases, Initial Masses M >6-10 Mo
73(2)
2.8 Core Collapse and Nucleosynthesis
75(8)
2.8.1 Abundances and Nucleosynthesis
78(5)
2.9 Variable Stars: A Brief Overview
83(106)
2.9.1 Eclipsing and Ellipsoidal Variables
83(1)
2.9.2 Spotted, Rotating Stars
84(1)
2.9.3 T Tauri Stars, FU Orionis Stars (FUORs), and Luminous Blue Variables
84(1)
2.9.4 Last Helium Flash and Formation of Atmospheric Dust
84(1)
2.10 Pulsational Variables
85(4)
2.11 Explosive Variables
89(14)
2.11.1 Novae
90(4)
2.11.2 Supernovae
94(3)
SN1987A
97(3)
SN Type I
100(2)
SN Remnants
102(1)
2.12 White Dwarfs, Neutron Stars, and Black Holes
103(2)
2.13 Binary Stars
105(11)
2.13.1 Types of Binaries
105(2)
2.13.2 The Roche Geometry
107(2)
2.13.3 Formation and Early Evolution
109(1)
2.13.4 The First Mass Transfer Phase and its Consequences
110(3)
2.13.5 Systems With One Compact Component
113(1)
2.13.6 The Second Phase of Mass Transfer
113(1)
2.13.7 Binaries With Two Compact Components
114(2)
2.14 Star Formation
116(4)
2.15 Supplemental Material
120(2)
2.16 Exercises
122(16)
2.17 References and Suggested Readings
138(7)
3 Equations of State 145(48)
3.1 Distribution Functions
146(4)
3.2 Blackbody Radiation
150(2)
3.3 Ideal Monatomic Gas
152(3)
3.4 The Saha Equation
155(4)
3.5 Fermi-Dirac Equations of State
159(12)
3.5.1 The Completely Degenerate Gas
160(3)
3.5.2 Application to White Dwarfs
163(3)
3.5.3 Effects of Temperature on Degeneracy
166(5)
3.6 "Almost Perfect" Equations of State
171(2)
3.7 Adiabatic Exponents and Other Derivatives
173(11)
3.7.1 Keeping the Composition Fixed
174(6)
Specific Heats
174(1)
Adiabatic Exponents
175(1)
Mixtures of Ideal Gases and Radiation
176(2)
Mixtures of Degenerate and Ideal Gases
178(2)
3.7.2 Allowing for Chemical Reactions
180(4)
3.8 Exercises
184(5)
3.9 References and Suggested Readings
189(4)
4 Radiative and Conductive Heat Transfer 193(48)
4.1 Radiative Transfer
193(6)
4.2 The Diffusion Equation
199(3)
4.2.1 A Brief Diversion into "Vs"
201(1)
4.3 A Simple Atmosphere
202(5)
4.4 Radiative Opacity Sources
207(7)
4.4.1 Electron Scattering
208(1)
4.4.2 Free-Free Absorption
209(3)
4.4.3 Bound-Free and Bound-Bound Absorption
212(1)
4.4.4 H- Opacity and Others
213(1)
4.5 Heat Transfer by Conduction
214(2)
4.6 Tabulated Opacities
216(7)
4.7 Some Observed Spectra
223(3)
4.8 Line Profiles and the Curve of Growth
226(6)
4.8.1 The Lorentz Profile
226(2)
4.8.2 Doppler Broadening
228(2)
4.8.3 Curve of Growth
230(2)
4.9 Exercises
232(4)
4.10 References and Suggested Readings
236(5)
5 Heat Transfer by Convection 241(30)
5.1 The Mixing Length Theory
241(17)
5.1.1 Criteria for Convection
242(5)
5.1.2 Radiative Leakage
247(2)
5.1.3 The Equation of Motion
249(1)
5.1.4 Convective Efficiencies and Time Scales
250(3)
5.1.5 Convective Fluxes
253(1)
5.1.6 Calculations in the MLT
254(1)
5.1.7 Numeric Examples
255(3)
5.2 Variations on the MLT
258(5)
5.2.1 Beyond the MLT
261(1)
5.2.2 Semiconvection
261(2)
5.3 Hydrodynamic Calculations
263(3)
5.4 Exercises
266(1)
5.5 References and Suggested Readings
267(4)
6 Stellar Energy Sources 271(58)
6.1 Gravitational Energy Sources
271(2)
6.2 Thermonuclear Energy Sources
273(26)
6.2.1 Preliminaries
274(2)
6.2.2 Nuclear Energetics
276(3)
6.2.3 Astrophysical Thermonuclear Cross Sections and Reaction Rates
279(3)
6.2.4 Nonresonant Reaction Rates
282(7)
Example: The 12C (p,γ) 13N Reaction
286(3)
6.2.5 Resonant Reaction Rates
289(2)
6.2.6 Other Forms of Reaction Rates
291(6)
Neutron Capture and the S-Process
292(2)
Weak Interactions
294(2)
The Proton-Proton Reaction
296(1)
6.2.7 Special Effects
297(2)
6.3 The Proton-Proton Chains
299(4)
6.3.1 Deuterium and Lithium Burning
303(1)
6.4 The Carbon-Nitrogen-Oxygen Cycles
303(4)
6.5 Helium-Burning Reactions
307(4)
6.6 Carbon, Neon, and Oxygen Burning
311(2)
6.7 Silicon "Burning"
313(1)
6.8 Neutrino Emission Mechanisms
314(4)
Pair Annihilation Neutrinos
315(1)
Photoneutrinos and Bremsstrahlung Neutrinos
316(1)
Plasma Neutrinos
317(1)
6.9 Exercises
318(4)
6.10 References and Suggested Readings
322(7)
7 Stellar Modeling 329(50)
7.1 The Equations of Stellar Structure
329(2)
7.2 Polytropes Equations of State and Polytropes
331(31)
7.2.1 General Properties of Polytropes
332(5)
7.2.2 Numerical Calculation of the Lane-Emden Functions
337(6)
Shooting for a Solution
338(2)
The Fitting Method
340(3)
7.2.3 The U-V Plane
343(2)
7.2.4 Newton-Raphson or "Henyey" Methods
345(4)
7.2.5 Eigenvalue Problems and the Henyey Method
349(2)
7.2.6 Dynamic Problems
351(6)
7.2.7 The Eddington Standard Model
357(4)
7.2.8 Applications to Zero-Temperature White Dwarfs
361(1)
7.3 The Approach to Real Models
362(12)
7.3.1 Central Expansions
362(1)
7.3.2 The Radiative Stellar Envelope
363(4)
The Structure of the Envelope
363(3)
The Radiative Temperature Structure
366(1)
7.3.3 Completely Convective Stars
367(13)
A Question of Entropy
370(3)
Application to Pre-Main Sequence Evolution
373(1)
7.4 Exercises
374(2)
7.5 References and Suggested Readings
376(3)
8 Asteroseismology 379(52)
8.1 Adiabatic Radial Pulsations
380(11)
8.1.1 The Linear Adiabatic Wave Equation
384(1)
8.1.2 Some Examples
385(3)
8.1.3 Asymptotic Analysis
388(3)
8.2 Nonadiabatic Radial Motions
391(13)
8.2.1 The Quasi-Adiabatic Approximation
394(3)
8.2.2 The κ- and γ-Mechanisms
397(3)
The Epstein Weight Function and Cepheids
399(1)
8.2.3 Nonadiabaticity and the Cepheid Strip
400(4)
A Footnote on Nonlinear Modeling
403(1)
8.3 An Introduction to Nonradial Oscillations
404(20)
8.3.1 Linearization of the Hydrodynamic Equations
404(4)
8.3.2 Separation of the Pulsation Equations
408(4)
8.3.3 Properties of the Solutions
412(7)
Mode Classification
415(3)
The Eigenfunctions
418(1)
8.3.4 The Inverse Problem and Rotation
419(15)
Probing for Internal Rotation
421(2)
Solid Stars?!
423(1)
8.4 Exercises
424(3)
8.5 References and Suggested Readings
427(4)
9 Structure and Evolution of the Sun 431(36)
9.1 Vital Statistics of the Sun
432(2)
9.2 From the ZAMS to the Present
434(8)
9.2.1 The Sun on the ZAMS
434(3)
9.2.2 Evolution From the ZAMS
437(2)
9.2.3 The Present-Day Sun
439(3)
9.3 The Solar Neutrino "Problem"
442(6)
9.4 The Role of Rotation in Evolution
448(6)
9.4.1 von Zeipel's Paradox
450(2)
9.4.2 Rotational Mixing of Stellar Interiors
452(2)
9.5 Helioseismology
454(6)
9.5.1 Observed and Predicted Pulsation Frequencies
455(1)
9.5.2 Helioseismology and the Solar Interior
456(13)
Structural Inversions
457(2)
Rotational Inversions
459(1)
9.6 References and Suggested Readings
460(7)
10 Structure and Evolution of White Dwarfs 467(1)
10.1 Observed Properties of White Dwarfs
467(2)
10.2 White Dwarf Evolution
469
10.2.1 Cooling of White Dwarfs
470(2)
10.2.2 Realistic Evolutionary Calculations
472(5)
10.3 The Magnetic White Dwarfs
477(2)
10.3.1 Magnetic Field Decay
479(2)
10.4 The Variable White Dwarfs
481(1)
10.4.1 The Observed Variables
482(1)
10.4.2 White Dwarf Seismology
482(3)
White Dwarfs and the Whole Earth Telescope
485(5)
10.5 Exercises
490(1)
10.6 References and Suggested Readings
490(7)
A Mini Stellar Glossary 497(6)
B Table of Symbols and Physical Constants 503(10)
C List of Journal Abbreviations 513(2)
Index 515

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