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Cover image for High-energy-density physics : fundamentals, inertial fusion, and experimental astrophysics
Title:
High-energy-density physics : fundamentals, inertial fusion, and experimental astrophysics
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Series:
Shock wave and high pressure phenomena
Publication Information:
Berlin : Springer, 2006
ISBN:
9783540293149

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30000010113225 QC718.4 D72 2006 Open Access Book Book
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Summary

Summary

This book has two goals. One goal is to provide a means for those new to high-energy-density physics to gain a broad foundation from one text. The second goal is to provide a useful working reference for those in the ?eld. This book has at least four possible applications in an academic c- text. It can be used for training in high-energy-density physics, in support of the growing number of university and laboratory research groups working in this area. It also can be used by schools with an emphasis on ultrafast lasers, to provide some introduction to issues present in all laser-target - perimentswithhigh-powerlasers,andwiththoroughcoverageofthematerial in Chap. 11 on relativistic systems. In addition, it could be used by physics, applied physics, or engineering departments to provide in a single course an introduction to the basics of ?uid mechanics and radiative transfer, with d- matic applications. Finally, it could be used by astrophysics departments for a similar purpose, with the parallel bene?t of training the students in the similarities and di?erences between laboratory and astrophysical systems. The notation in this text is deliberately sparse and when possible a given symbol has only one meaning. A de?nition of the symbols used is given in Appendix A. In various cases, additional subscripts are added to distinguish among cases of the same quantity, as for example in the use of ? and ? 1 2 to distinguish the mass density in two di?erent regions.


Table of Contents

1 Introduction to High-Energy-Density Physicsp. 1
1.1 Some Historical Remarksp. 2
1.2 Regimes of High-Energy-Density Physicsp. 5
1.3 An Introduction to Inertial Confinement Fusionp. 8
1.4 An Introduction to Experimental Astrophysicsp. 11
1.5 Some Connections to Prior Workp. 14
1.6 Variables and Notationp. 16
2 Descriptions of Fluids and Plasmasp. 19
2.1 The Euler Equations for a Polytropic Gasp. 19
2.2 The Maxwell Equationsp. 24
2.3 More General and Complete Single-Fluid Equationsp. 26
2.3.1 General Single-Fluid Equationsp. 27
2.3.2 Magnetohydrodynamicsp. 33
2.3.3 Single Fluid, Three Temperaturep. 36
2.3.4 Approaches to Computer Simulationp. 37
2.4 Plasma Theoriesp. 40
2.4.1 Regimes of Validity of Traditional Plasma Theoryp. 40
2.4.2 The Two-Fluid Equationsp. 44
2.4.3 The Kinetic Descriptionp. 49
2.5 Single-Particle Motionsp. 50
3 Properties of High-Energy-Density Plasmasp. 55
3.1 Simple Equations of Statep. 57
3.1.1 Polytropic Gasesp. 57
3.1.2 Radiation-Dominated Plasmap. 59
3.1.3 Fermi-Degenerate EOSp. 60
3.2 Ionizing Plasmasp. 66
3.2.1 Ionization Balance from the Saha Equationp. 68
3.2.2 Continuum Lowering and the Ion Sphere Modelp. 73
3.2.3 Coulomb Interactionsp. 78
3.3 Thermodynamics of Ionizing Plasmasp. 80
3.3.1 Generalized Polytropic Indicesp. 81
3.3.2 Pressure, Energy, and Their Consequencesp. 84
3.3.3 The EOS Landscapep. 89
3.4 Equations of State for Computationsp. 90
3.4.1 The Thomas-Fermi Model and QEOSp. 91
3.4.2 Tabular Equations of Statep. 93
3.5 Equations of State in the Laboratory and in Astrophysicsp. 96
3.5.1 The Astrophysical Context for EOSp. 97
3.5.2 Connecting EOS from the Laboratory to Astrophysicsp. 99
3.6 Experiments to Measure Equations of Statep. 100
3.6.1 Direct Flyer-Plate Measurementsp. 101
3.6.2 Impedance Matchingp. 101
3.6.3 Other Techniquesp. 103
4 Shocks and Rarefactionsp. 107
4.1 Shock Wavesp. 108
4.1.1 Jump Conditionsp. 109
4.1.2 The Shock Hugoniot and Equations of Statep. 111
4.1.3 Useful Shock Relationsp. 112
4.1.4 Entropy Changes Across Shocksp. 118
4.1.5 Oblique Shocksp. 119
4.1.6 Shocks and Interfaces, Flyer Platesp. 122
4.2 Rarefaction Wavesp. 128
4.2.1 The Planar Isothermal Rarefaction and Self-Similar Analysisp. 129
4.2.2 Riemann Invariantsp. 132
4.2.3 Planar Adiabatic Rarefactionsp. 136
4.3 Blast Wavesp. 139
4.3.1 Energy Conservation in Blast Wavesp. 140
4.3.2 A General Discussion of Self-Similar Motionsp. 142
4.3.3 The Sedov-Taylor Spherical Blast Wavep. 146
4.4 Phenomena at Interfacesp. 149
4.4.1 Shocks at Interfaces and Their Consequencesp. 149
4.4.2 Overtaking Shocksp. 153
4.4.3 Reshocks in Rarefactionsp. 154
4.4.4 Blast Waves at Interfacesp. 156
4.4.5 Rarefactions at Interfacesp. 158
4.4.6 Oblique Shocks at Interfacesp. 162
5 Hydrodynamic Instabilitiesp. 169
5.1 Introduction to the Rayleigh-Taylor Instabilityp. 170
5.1.1 Buoyancy as a Driving Forcep. 171
5.1.2 Fundamentals of the Fluid-Dynamics Descriptionp. 175
5.2 Applications of the Linear Theory of the Rayleigh-Taylor Instabilityp. 180
5.2.1 Rayleigh-Taylor Instability with Two Uniform Fluidsp. 180
5.2.2 Effects of Viscosity on the Rayleigh-Taylor Instabilityp. 182
5.2.3 Rayleigh-Taylor with Density Gradients and the Global Modep. 187
5.3 The Convective Instability or the Entropy Modep. 190
5.4 Buoyancy-Drag Models of the Nonlinear Rayleigh-Taylor Statep. 193
5.5 Mode Couplingp. 195
5.6 The Kelvin-Helmholtz Instabilityp. 202
5.6.1 Fundamental Equations for Kelvin-Helmholtz Instabilitiesp. 203
5.6.2 Uniform Fluids with a Sharp Boundaryp. 206
5.6.3 Otherwise Uniform Fluids with a Distributed Shear Layerp. 208
5.6.4 Uniform Fluids with a Transition Regionp. 209
5.7 Shock Stability and Richtmyer-Meskov Instabilityp. 213
5.7.1 Shock Stabilityp. 213
5.7.2 Interaction of Shocks with Rippled Interfacesp. 217
5.7.3 Postshock Evolution of the Interface; Richtmyer Meshkov Instabilityp. 219
5.8 Hydrodynamic Turbulencep. 224
6 Radiative Transferp. 237
6.1 Basic Conceptsp. 239
6.1.1 Properties and Description of Radiationp. 239
6.1.2 Thermal Radiationp. 244
6.1.3 Types of Interaction Between Radiation and Matterp. 244
6.1.4 Description of the Net Interaction of Radiation and Matterp. 247
6.2 Radiation Transferp. 249
6.2.1 The Radiation Transfer Equationp. 249
6.2.2 Radiative Transfer Calculationsp. 250
6.2.3 Opacities in Astrophysics and the Laboratoryp. 255
6.2.4 Radiation Transfer in the Equilibrium Diffusion Limitp. 258
6.2.5 Nonequilibrium Diffusion and Two-Temperature Modelsp. 261
6.3 Relativistic Considerations for Radiative Transferp. 262
7 Radiation Hydrodynamicsp. 267
7.1 Radiation Hydrodynamic Equationsp. 270
7.1.1 Fundamental Equationsp. 270
7.1.2 Thermodynamic Relationsp. 272
7.2 Radiation and Fluctuationsp. 274
7.2.1 Radiative Acoustic Waves; Optically Thick Casep. 274
7.2.2 Cooling When Transport Mattersp. 277
7.2.3 Optically Thin Acoustic Wavesp. 282
7.2.4 Radiative Thermal Instabilityp. 285
7.3 Radiation Diffusion and Marshak Wavesp. 287
7.3.1 Marshak Wavesp. 287
7.3.2 Ionizing Radiation Wavep. 291
7.3.3 Constant-Energy Radiation Diffusion Wavep. 293
7.4 Radiative Shocksp. 296
7.4.1 Regimes of Radiative Shocksp. 296
7.4.2 Fluid Dynamics of Radiative Shocksp. 301
7.4.3 Models of Radiative Precursorsp. 309
7.4.4 Optically Thin Radiative Shocksp. 317
7.4.5 Radiative Shocks that are Thick Downstream and Thin Upstreamp. 320
7.4.6 Fluid Dynamics of Optically Thick Radiative Shocksp. 324
7.4.7 Optically Thick Shocks-Radiative-Flux Regimep. 326
7.4.8 Radiation-Dominated Optically Thick Shocksp. 328
7.4.9 Electron-Ion Coupling in Shocksp. 330
7.5 Ionization Frontsp. 332
8 Creating High-Energy-Density Conditionsp. 335
8.1 Direct Laser Irradiationp. 336
8.1.1 Laser Technologyp. 336
8.1.2 Laser Focusingp. 338
8.1.3 Propagation and Absorption of Electromagnetic Wavesp. 341
8.1.4 Laser Scattering and Laser-Plasma Instabilitiesp. 347
8.1.5 Electron Heat Transportp. 354
8.1.6 Ablation Pressurep. 361
8.2 Hohlraumsp. 366
8.2.1 X-Ray Conversion of Laser Lightp. 367
8.2.2 X-Ray Production by Ion Beamsp. 372
8.2.3 X-Ray Ablationp. 372
8.2.4 Problems with Hohlraumsp. 376
8.3 Z-Pinches and Related Methodsp. 379
8.3.1 Z-Pinches for High-Energy-Density Physicsp. 380
8.3.2 Dynamic Hohlraumsp. 387
8.3.3 Magnetically Driven Flyer Platesp. 390
9 Inertial Confinement Fusionp. 391
9.1 The Final Statep. 392
9.1.1 What Fuel, Under What Conditions?p. 393
9.1.2 Energy Gain: Is This Worth Doing?p. 396
9.1.3 Properties of Compressed DT Fuelp. 397
9.2 Creating and Igniting the Final Statep. 402
9.2.1 Achieving a Highly Compressed Statep. 402
9.2.2 Igniting the Fuelp. 407
9.2.3 Igniting from a Central Hot Spotp. 410
9.2.4 Fast Ignitionp. 412
9.3 Pitfalls and Problemsp. 415
9.3.1 Rayleigh Taylorp. 415
9.3.2 Symmetryp. 418
9.3.3 Laser-Plasma Instabilitiesp. 419
10 Experimental Astrophysicsp. 423
10.1 Scaling in Hydrodynamic Systemsp. 424
10.2 A Thorough Example: Interface Instabilities in Type II Supernovaep. 428
10.2.1 The Astrophysical Context for Type II Supernovaep. 429
10.2.2 The Scaling Problem for Interface Instabilities in Supernovaep. 432
10.2.3 Experiments on Interface Instabilities in Type II Supernovaep. 436
10.3 A Second Example: Cloud-Crushing Interactionsp. 439
10.4 Scaling in Radiation Hydrodynamic Systemsp. 441
10.5 Radiative Astrophysical Jets: Context and Scalingp. 443
10.5.1 The Context for Jets in Astrophysicsp. 443
10.5.2 Scaling from Radiative Astrophysical Jets to the Laboratoryp. 445
10.5.3 Radiative Jet Experimentsp. 447
11 Relativistic High-Energy-Density Systemsp. 449
11.1 Development of Ultrafast Lasersp. 451
11.2 Single-Electron Motion in Intense Electromagnetic Fieldsp. 452
11.3 Initiating Relativistic Laser-Plasma Interactionsp. 461
11.4 Absorption Mechanismsp. 464
11.5 Harmonic Generationp. 467
11.6 Relativistic Self-Focusing and Induced Transparencyp. 469
11.7 Particle Accelerationp. 470
11.7.1 Acceleration Within Plasmasp. 470
11.7.2 Acceleration by Surface Potentials on Solid Targetsp. 474
11.7.3 Acceleration by Coulomb Explosionsp. 475
11.8 Hole Drilling and Collisionless Shocksp. 478
11.9 Other Phenomenap. 482
12 Appendix A: Constants, Acronyms, and Standard Variablesp. 485
13 Appendix B: Sample Mathematica Codep. 491
14 Appendix C: A List of the Homework Problemsp. 501
Indexp. 529
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