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Relativistic mirrors in laser plasmas (analytical methods)
https://repo.qst.go.jp/records/48054
https://repo.qst.go.jp/records/48054ab65adb3-97e4-4769-bd54-5e71c961ba93
Item type | 学術雑誌論文 / Journal Article(1) | |||||
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公開日 | 2017-06-15 | |||||
タイトル | ||||||
タイトル | Relativistic mirrors in laser plasmas (analytical methods) | |||||
言語 | ||||||
言語 | eng | |||||
資源タイプ | ||||||
資源タイプ識別子 | http://purl.org/coar/resource_type/c_6501 | |||||
資源タイプ | journal article | |||||
アクセス権 | ||||||
アクセス権 | metadata only access | |||||
アクセス権URI | http://purl.org/coar/access_right/c_14cb | |||||
著者 |
ブラノフ, セルゲイ
× ブラノフ, セルゲイ× エシロケポフ, ティムル× 神門, 正城× コーガ, ジェームズ× ブラノフ セルゲイ× エシロケポフ ティムル× 神門 正城× コーガ ジェームズ |
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抄録 | ||||||
内容記述タイプ | Abstract | |||||
内容記述 | Relativistic flying mirrors in plasmas are realized as thin dense electron (or electron–ion) layers accelerated by high-intensity electromagnetic waves to velocities close to the speed of light in vacuum. The reflection of an electromagnetic wave from the relativistic mirror results in its energy and frequency changing. In a counter-propagation configuration, the frequency of the reflected wave is multiplied by the factor proportional to the Lorentz factor squared. This scientific area promises the development of sources of ultrashort x-ray pulses in the attosecond range. The expected intensity will reach the level at which the effects predicted by nonlinear quantum electrodynamics start to play a key role. We present an overview of theoretical methods used to describe relativistic flying, accelerating, oscillating mirrors emerging in intense laser-plasma interactions. | |||||
書誌情報 |
Plasma Sources Sci. Technol. 巻 25, 号 5, p. 053001-1-053001-17, 発行日 2016-07 |
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出版者 | ||||||
出版者 | IOP Publishing | |||||
DOI | ||||||
識別子タイプ | DOI | |||||
関連識別子 | 10.1088/0963-0252/25/5/053001 |