Ultrabright Attosecond Sources from Relativistically Oscillating Mirrors

被引：0

作者：

Zepf, M. ^{[1
]}

Adams, D. ^{[1
]}

Dromey, B. ^{[1
]}

Geissler, M. ^{[1
]}

Hoerlein, R. ^{[2
]}

Nomura, Y. ^{[2
]}

Rykovanov, S. ^{[2
]}

Tsakiris, G. D. ^{[2
]}

机构：

[1] Queens Univ, Dept Phys & Astron, Belfast, Antrim, North Ireland

[2] Max Planck Inst Quantum Opt, Garching, Germany

来源：

HARNESSING RELATIVISTIC PLASMA WAVES AS NOVEL RADIATION SOURCES FROM TERAHERTZ TO X-RAYS AND BEYOND | 2009年 / 7359卷

基金：

英国工程与自然科学研究理事会;

关键词：

X-ray generation; Coherent X-ray radiation; Relativistic Plasmas; HARMONIC-GENERATION; LASER HARMONICS; PULSE;

D O I：

10.1117/12.820848

中图分类号：

O43 [光学];

学科分类号：

070207 ; 0803 ;

摘要：

The interaction of relativistically intense (I lambda(2)>>1.3 10(18)Wcm(-2)mu m(2)) laser pulses with a near step-like plasma density profile results in relativistic oscillations of the reflection point. This process results in efficient conversion of the incident laser to a phase-locked high harmonic spectrum, which allows the generation of attosecond pulses and pulse trains. Recent experimental results on efficiency scaling, highest harmonic generated and beam quality suggest that very high focused intensities can be achieved opening up the possibility of ultra-intense attosecond X-ray interactions for the first time.

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页数：6

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