Titlebook: High Energy Density Laboratory Astrophysics; G.A. Kyrala Book 2005 Springer Science+Business Media B.V. 2005 Accretion.MHD.Plasma.astrophy

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Hypernovae and Gamma-Ray Bursts,o the enigmatic Gamma-Ray Bursts. The optical properties of hypernovae indicate that they are significantly aspherical. Synthetic light curves and late-phase spectra of aspherical supernova/hypernova models are presented. These models can account for the optical observations of SNe 1998bw and 2002ap

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Radiation Hydrodynamics in Supernovae,e and thermonuclear supernovae. In supernovae, one of the main issues is the coupling between a radiation field and properties of the matter. Due to the low densities, nonthermal excitation by high-energy photons from radioactive decays and the time dependence of the problem, significant departures

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Experiment on Collisionless Plasma Interaction with Applications to Supernova Remnant Physics,rnova remnant (SNR) are discussed. Ideal magneto-hydrodynamic scaling indicates that the experimental plasma matches the SNR plasma at 500 ps. Experimental data show that the magnetic field can alter the plasma density profile when two similar plasmas interact in a colliding geometry. These results

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,Hydrogen EOS at Megabar Pressures and the Search for Jupiter’s Core, from ～0.1.. to ～80.. (1.. = Jupiter mass = 1.9.30g), comprising hydrogen-rich giant planets (mass < 13..) and brown dwarfs (mass > 13.. but ～<80..), the so-called substellar objects (SSOs). Formation of giant planets may involve nucleated collapse of nebular gas onto a solid, dense core of mass ～0.

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How Did Cassiopeia A Explode? A Chandra VLP,The Cassiopeia A supernova remnant will be observed by Chandra for 1 Ms this spring. We discuss our motivations and plans for acquiring and analyzing these data.