Dynamics of relativistic transparency and optical shuttering in expanding overdense plasmas

Overdense plasmas are usually opaque to laser light. However, when the light is of sufficient intensity to drive electrons in the plasma to near light speeds, the plasma becomes transparent. This process—known as relativistic transparency—takes just a tenth of a picosecond. Yet all studies of relati...

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Veröffentlicht in:Nature physics 2012-10, Vol.8 (10), p.763-769
Hauptverfasser: Palaniyappan, Sasi, Hegelich, B. Manuel, Wu, Hui-Chun, Jung, Daniel, Gautier, Donald C., Yin, Lin, Albright, Brian J., Johnson, Randall P., Shimada, Tsutomu, Letzring, Samuel, Offermann, Dustin T., Ren, Jun, Huang, Chengkun, Hörlein, Rainer, Dromey, Brendan, Fernandez, Juan C., Shah, Rahul C.
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Sprache:eng
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Zusammenfassung:Overdense plasmas are usually opaque to laser light. However, when the light is of sufficient intensity to drive electrons in the plasma to near light speeds, the plasma becomes transparent. This process—known as relativistic transparency—takes just a tenth of a picosecond. Yet all studies of relativistic transparency so far have been restricted to measurements collected over timescales much longer than this, limiting our understanding of the dynamics of this process. Here we present time-resolved electric field measurements (with a temporal resolution of ∼ 50 fs) of the light, initially reflected from, and subsequently transmitted through, an expanding overdense plasma. Our result provides insight into the dynamics of the transparent-overdense regime of relativistic plasmas, which should be useful in the development of laser-driven particle accelerators, X-ray sources and techniques for controlling the shape and contrast of intense laser pulses. When electrons are accelerated to near light-speeds through an overdense plasma by an intense laser beam, the usually opaque plasma becomes optically transparent. High-speed laser experiments provide unprecedented insight into the dynamics of this process.
ISSN:1745-2473
1745-2481
DOI:10.1038/nphys2390