| 书目名称 | Frontiers and Challenges in Warm Dense Matter |
| 编辑 | Frank Graziani,Michael P. Desjarlais,Samuel B. Tri |
| 视频video | |
| 概述 | Each paper is a review or tutorial of a key aspect of warm dense matter physics written by a leader in the field.The book is perfect for those wanting to learn more about WDM as well as those who are |
| 丛书名称 | Lecture Notes in Computational Science and Engineering |
| 图书封面 |  |
| 描述 | 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 |
| 出版日期 | Conference proceedings 2014 |
| 关键词 | High energy density phyiscs; Highly correlated systems; Statistical phyiscs |
| 版次 | 1 |
| doi | https://doi.org/10.1007/978-3-319-04912-0 |
| isbn_softcover | 978-3-319-37962-3 |
| isbn_ebook | 978-3-319-04912-0Series ISSN 1439-7358 Series E-ISSN 2197-7100 |
| issn_series | 1439-7358 |
| copyright | Springer International Publishing Switzerland 2014 |
发表于 2025-3-21 17:15:20
