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Titlebook: High-Energy-Density Physics; Fundamentals, Inerti R. Paul Drake,Lee Davison,Yasuyuki Horie Textbook 20061st edition Springer-Verlag Berlin

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發(fā)表于 2025-3-21 17:31:33 | 只看該作者 |倒序?yàn)g覽 |閱讀模式
書(shū)目名稱(chēng)High-Energy-Density Physics
副標(biāo)題Fundamentals, Inerti
編輯R. Paul Drake,Lee Davison,Yasuyuki Horie
視頻videohttp://file.papertrans.cn/427/426594/426594.mp4
概述First textbook on an emerging topic.Renders advanced research accessible to novices.Provides directions for further research
叢書(shū)名稱(chēng)Shock Wave and High Pressure Phenomena
圖書(shū)封面Titlebook: High-Energy-Density Physics; Fundamentals, Inerti R. Paul Drake,Lee Davison,Yasuyuki Horie Textbook 20061st edition Springer-Verlag Berlin
描述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 sy
出版日期Textbook 20061st edition
關(guān)鍵詞Confinement; Plasma; astrophysical plasmas; astrophysics; high-energy density; inertial fusion; laboratory
版次1
doihttps://doi.org/10.1007/3-540-29315-9
isbn_softcover978-3-642-06726-6
isbn_ebook978-3-540-29315-6Series ISSN 2197-9529 Series E-ISSN 2197-9537
issn_series 2197-9529
copyrightSpringer-Verlag Berlin Heidelberg 2006
The information of publication is updating

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Radiative Transfer,ems: radiation. It is easy to see why radiation often matters. At any given pressure, the temperature increases as density decreases, and there is some density below which radiative fluxes will exceed material fluxes.
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https://doi.org/10.1007/3-540-29315-9Confinement; Plasma; astrophysical plasmas; astrophysics; high-energy density; inertial fusion; laboratory
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Shock Wave and High Pressure Phenomenahttp://image.papertrans.cn/h/image/426594.jpg
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