Author: Publisher:
ISBN:
Category :
Languages : en
Pages : 8
Book Description
Resonant Bound-Free Contributions to Thomson Scattering of X-rays by Warm Dense Matter
Author: X-ray Sources for X-ray Thomson Scattering of Warm Dense Matter on the Z-Accelerator
Author: Simulations of X-ray Thomson Scattering from Warm Dense Matter
Author: Ghulam Shabbir NazX-ray Thomson Scattering of Warm Dense Matter on the Z-accelerator
Author: X-ray Thomson Scattering of Warm Dense Matter on Z-accelerator
Author: Modeling X-ray Thomson Scattering Spectra of Warm Dense Matter
Author: Simulations of X-ray Thomson Scattering From Warm Dense Matter
Author: G. S. N. NazTheory of X-ray Thomson Scattering in Warm Dense Matter
Author: Kathrin WünschX-ray Thomson Scattering Measurements of Warm Dense Matter
Author: Frontiers and Challenges in Warm Dense Matter
Author: Frank GrazianiPublisher: Springer Science & Business
ISBN: 3319049127
Category : Computers
Languages : en
Pages : 294
Book Description
Warm Dense Matter (WDM) occupies a loosely defined region of phase space intermediate between solid, liquid, gas, and plasma, and typically shares characteristics of two or more of these phases. WDM is generally associated with the combination of strongly coupled ions and moderately degenerate electrons, and careful attention to quantum physics and electronic structure is essential. The lack of a small perturbation parameter greatly limits approximate attempts at its accurate description. Since WDM resides at the intersection of solid state and high energy density physics, many high energy density physics (HEDP) experiments pass through this difficult region of phase space. Thus, understanding and modeling WDM is key to the success of experiments on diverse facilities. These include the National Ignition Campaign centered on the National Ignition Facility (NIF), pulsed-power driven experiments on the Z machine, ion-beam-driven WDM experiments on the NDCX-II, and fundamental WDM research at the Linear Coherent Light Source (LCLS). Warm Dense Matter is also ubiquitous in planetary science and astrophysics, particularly with respect to unresolved questions concerning the structure and age of the gas giants, the nature of exosolar planets, and the cosmochronology of white dwarf stars. In this book we explore established and promising approaches to the modeling of WDM, foundational issues concerning the correct theoretical description of WDM, and the challenging practical issues of numerically modeling strongly coupled systems with many degrees of freedom.