Suchen und Finden
Preface
7
Acknowledgments
11
Contents
13
Acronyms
17
Introduction
19
1 Hydrodynamical Limit---Classical Problems of Accretion and Ejection
23
Astrophysical Introduction---Accretion onto Compact Objects
24
Accretion Disks
24
Standard Model
28
ADAF, ADIOS, etc.
31
Main Properties of Transonic Hydrodynamical Flows
33
Basic Equations
33
Spherically Symmetric Flow
35
Potential Plane Flow
39
Nonrelativistic Axisymmetric Stationary Flows
46
Basic Equations
46
Mathematical Intermezzo---the Covariant Approach
48
Two-Dimensional Flow Structure
49
Bondi--Hoyle Accretion
58
Outflow from a Slowly Rotating Star
62
Axisymmetric Stationary Flows in the Vicinity of a Black Hole
71
Physical Intermezzo---(3+1)-Splitting in the Kerr Metric
71
Basic Equations
75
Exact Solutions
81
Bondi--Hoyle Accretion---The Relativistic Regime
84
Accretion onto a Slowly Rotating Black Hole
87
Accretion of Matter with Small Angular Momentum
89
Thin Transonic Disk
95
Conclusion
106
2 Force-Free Approximation---The Magnetosphere of Radio Pulsars
107
Astrophysical Introduction
107
Basic Physical Processes
111
Vacuum Approximation
111
Particle Generation in the Strong Magnetic Field
116
Magnetosphere Structure
119
Secondary Plasma Generation
123
``Inner Gap''
123
Neutron Star Surface
128
Propagation of -Quanta in the Superstrong Magnetic Field
129
General Relativity Effects
130
Particle Generation in the Magnetosphere
132
``Hollow Cone'' Model
134
Secondary Plasma Generation---``Outer Gap''
138
Pulsar Equation
138
Force-Free Approximation. The Magnetization Parameter
138
Integrals of Motion
140
Grad--Shafranov Equation
143
Mathematical Intermezzo---Quasistationary Formalism
146
Energy Losses of Radio Pulsars
149
Current Loss Mechanism
149
Slowing Down of Inclined and Orthogonal Rotators
153
Magnetosphere Structure
161
Exact Solutions
161
Magnetosphere Structure with Longitudinal Currents
180
Magnetosphere Models
187
Conclusion
193
3 Force-Free Approximation---The Black Hole Magnetosphere
194
Astrophysical Introduction---The Central Engine in Active Galactic Nuclei
194
Possible Mechanisms of Black Hole Formation
194
Nature of Activity and Variability
1
Magnetized Accretion Disk
198
Regular Magnetic Field Generation
200
Basic Equations
203
(3+1)-Splitting for the Electromagnetic Field
203
``No Hair'' Theorem
205
Vacuum Approximation
208
Force-Free Grad--Shafranov Equation in the Kerr Metric
213
Particle Generation
218
Energy Release Mechanism
220
Blandford--Znajek Process
220
Physical Intermezzo---Black Hole Thermodynamics
224
Black Hole Magnetosphere Structure
227
General Properties
227
Exact Solutions
228
Magnetosphere Models
236
Conclusion
241
4 Full MHD Version---General Properties
243
Physical Introduction---Magnetohydrodynamic Waves
243
Relativistic Flows in the Kerr Metric
248
Integrals of Motion
248
Singular Surfaces
253
Grad--Shafranov Equation
257
Special Cases
260
Nonrelativistic Flows
260
Anisotropic Pressure
264
General Properties
268
Some Useful Relations
268
Alfvén Surface
272
Fast Magnetosonic Surface---Relativistic Flows
274
Fast Magnetosonic Surface---Nonrelativistic Flows
282
Behavior of the Solution at Large Distances
288
Behavior of the Solution in the Vicinity of the Horizon
295
5 Full MHD Version---Particle Acceleration and Collimation
301
Astrophysical Introduction
301
Radio Pulsars
301
Active Galactic Nuclei
305
Young Stellar Objects
309
Microquasars, Cosmological Gamma-Bursters, etc.
312
Cylindrical Flows
314
Cylindrical Jets---The Force-Free Approximation
314
Relativistic Jets
319
Nonrelativistic Jets
335
General Properties and Application
341
Cold Quasimonopole Outflows
343
Relativistic Slowly Rotating Outflows
343
Relativistic Outflows with Differential Rotation
347
Nonrelativistic Slowly Rotating Outflows
350
Relativistic Fast-Rotating Outflow
352
Relativistic Outflow in the Parabolic Magnetic Field
358
General Properties
362
Black Hole Magnetosphere
363
Slowly Rotating Black Hole Surrounded by a Thin Disk
363
Slowly Rotating Black Hole Surrounded by a Rotating Shell
371
Other Methods
376
Analysis of the Algebraic Relations
376
Self-Similar Solutions
380
Computational Results
387
Conclusion
395
6 Conclusion
397
A From Euler to Grad--Shafranov---The Simplest Way
400
B Nonrelativistic Force-Free Grad--Shafranov Equation
402
C Part-Time Job Pulsars
404
D Special Functions
406
Legendre Polynomials
406
Bessel Functions
407
Hypergeometric Function
408
E List of Symbols
410
References
416
Index
438
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