High energy density laboratory astrophysics /
During the past several years, research teams around the world have developed astrophysics-relevant utilizing high energy-density facilities such as intense lasers and z-pinches. This work covers topics such as: hydrodynamic instabilities in astrophysics, supernovae and supernova remnant evolution,...
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| Format: | Conference Proceeding Book |
| Language: | English |
| Published: |
[Dordrecht] :
Springer,
2005
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| Series: | Astrophysics and space science ;
v. 298, no. 1-2 |
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Table of Contents:
- Cover
- Table of Contents
- Preface
- Asymmetric Supernovae: Yes, Rotation and Magnetic Fields are Important
- Progress Toward the Study of Laboratory Scale, Astrophysically Relevant, Turbulent Plasmas
- Effects of Initial Conditions on Compressible Mixing in Supernova-Relevant Laboratory Experiments
- Laboratory Astrophysics Experiments for Simulation Code Validation: A Case Study
- How Did Cassiopeia A Explode? A Chandra VLP
- Studies of Laser-Driven Radiative Blast Waves
- Radiative Shocks in Astrophysics and the Laboratory
- Laboratory Simulations of Supernova Shockwave Propagation
- Radiative Shock Experiments at Luli
- Analytical Study of Supernova Remnant Non-Stationary Expansions
- Hypernovae and Gamma-Ray Bursts
- Radiation Hydrodynamics in Supernovae
- Experiment on Collisionless Plasma Interaction with Applications to Supernova Remnant Physics
- Laboratory Experiments of Stellar Jets from the Perspective of an Observer
- A Hed Laboratory Astrophysics Testbed Comes of Age: Jet Deflection via Cross Winds
- Relativistic Jets from Accretion Disks
- Recent Experimental Results and Modelling of High-Mach-Number Jets and the Transition to Turbulence
- Hydrogen EOS at Megabar Pressures and the Search for Jupiter's Core
- Astrophysical Implications of the Recent Shocked Deuterium Experiments
- Deuterium Hugoniot up to 120 GPa (1.2 Mbar)
- Modeling X-Ray Photoionized Plasmas Produced at the Sandia Z-Facility
- Radiation Properties of High-Energy Astrophysical Plasmas
- Preliminary Results from an Astrophysically Relevant Radiation Transfer Experiment
- X-Ray Line Transfer in Plasmas with Large Velocity Gradients
- Eagle Nebula Pillars: From Models to Observations
- Two Models of Magnetic Support for Photoevaporated Molecular Clouds
- Shock Propagation Through Multiphase Media
- Hydrodynamic Instability of Ionization Front in HII Regions: From Linear to Nonlinear Evolution
- Simulating Astrophysical Jets in Laboratory Experiments
- Particle Acceleration in Relativistic Magnetized Plasmas
- Magnetic Reconnection, Turbulence, and Collisionless Shock
- Direct-Drive Inertial Confinement Fusion Implosions on Omega
- Accessing High Pressure States Relevant to Core Conditions in the Giant Planets
- Formation of Working Surfaces in Radiatively Cooled Laboratory Jets
- Boltzmann Equilibrium of Endothermic Heavy Nuclear Synthesis in the Universe and a Quark Relation to the Magic Numbers
- Richtmyer-Meshkov Experiments on the Omega Laser
- Molecular Clouds: Observation to Experiment
- Preheat Issues in Hydrodynamic Hedla Experiments
- Zeus-2D Simulations of Laser-Driven Radiative Shock Experiments
- Modeling Magnetic Tower Jets in the Laboratory
- Tailored Blast Wave Production Pertaining to Supernova Remnants
- A Neutron Star Atmosphere in the Laboratory with Petawatt Lasers
- Laboratory Simulation of Magnetospheric Plasma Shocks
- Studying Hydrodynamic Instability Using Shock-Tube Experiments
- Novel Diagnostic of Shock Fronts in Low-Z Dense Plasmas
- Evolution and Fragmentation of Wide-Angle Wind Driven Molecular Outflows
- X-Ray Line and Recombination Emission in the Afterglow of GRB
- Richtmyer ... Meshkov Instability Reshock Experiments Using Laser-Driven Double-Cylinder Implosions
- Density and Temperature Measurements on Laser Generated Radiative Shocks
- Linear Analysis of Axial Sheared Flow in Astrophysi