Control of Laser Contrast for Harmonic Generation from Relativistic Plasma Surfaces

30.01.2026, 08:30
30m
Darmstädter Haus

Darmstädter Haus

Oberseitestr. 38 D- 87568 Hirschegg

Sprecher

Jordan Young (Queen's University Belfast)

Beschreibung

High power laser systems driving relativistic plasmas have applications in the generation of high energy, short duration particle and photon secondary sources. These mechanisms are typically extremely sensitive to laser contrast - pre-pulses and amplified spontaneous emission (ASE) that can trigger an expanding plasma long before the peak intensity is reached. As we enter the multi-petawatt regime, the requirements on laser contrast will become more stringent as peak intensity rises.

One commonly used method of improving a laser’s contrast is using plasma mirrors. These optical systems take advantage of the fast switch on time of an initially transparent medium as it is turned to plasma by the intense laser pulse itself. This has the effect that any light impinging before the peak of the pulse will not be reflected and is removed prior to the main interaction. Using a chain of two such optics, Double Plasma Mirror (DPM) systems have been effectively demonstrated to improve the contrast of laser pulses by 4-5 orders of magnitude, well before the rising edge at a few picoseconds before the peak of the pulse [1,2]. However, the impact very close to the peak as the intensity rises rapidly is less clear despite these timescales still being very impactful on the final plasma conditions.

Surface high harmonic generation (SHHG) from overdense plasmas is one application of high-power lasers that is extremely sensitive to laser pulse contrast [3]. Not only is SHHG a powerful source of extreme ultraviolet (XUV) and attosecond duration radiation, but it can also provide an effective benchmark of laser pulse contrast. Here we present characterisations of a DPM system currently in operation on the Gemini laser and its impact on the observed SHHG signal when a controlled pre-pulse is added. Furthermore, we discuss planned developments on the JETI-200 laser and the expected performance for SHHG experiments.

[1] A. Lévy et al., “Double plasma mirror for ultrahigh temporal contrast ultraintense laser pulses,” Optics Letters, vol. 32, no. 3, p. 310, Jan. 2007, doi: https://doi.org/10.1364/ol.32.000310.
[2] I. W. Choi et al., “Highly efficient double plasma mirror producing ultrahigh-contrast multi-petawatt laser pulses,” Optics Letters, vol. 45, no. 23, pp. 6342–6342, Oct. 2020, doi: https://doi.org/10.1364/ol.409749.
[3] S. Kahaly et al., “Direct Observation of Density-Gradient Effects in Harmonic Generation from Plasma Mirrors,” Physical review letters, vol. 110, no. 17, Apr. 2013, doi: https://doi.org/10.1103/physrevlett.110.175001

Autor

Jordan Young (Queen's University Belfast)

Co-Autoren

Brendan Dromey (Queens UIniversity Belfast) Cara McDonald (Queen's University Belfast) Dr. Chris Biard (CLF) Ciara McHugh (Queen's University Belfast) Colm Fitzpatrick (Queen's university Belfast) Elliott Denis (University of Oxford) Holly Huddleston (Queen's University Belfast) Jeremy Rebenstock (University of Michigan) Jimmy Weeks (Queen's University Belfast, CLF) John Neely (AWE) Jonathan Kennedy (Queen's University Belfast) Joshua Redfern (University of Oxford) Kark Krushelnick (University of Michigan) Mark Yeung (Queen's University Belfast) Matt Zepf (Helmholtz Institute Jena) Nicolas Bourgeois (Central Laser Facility RAL) Oliver Finlay (Central Laser Facility RAL) Dr. Peter Hilz (Helmholtz Institute Jena) Peter Norreys (University of Oxford) Robin Timmis (University of Oxford) Sam Astbury (Central Laser Facility RAL) Stefan Kiesel (GSI Helmholtzzentrum für Schwerionenforschung GmbH(GSI)) Steve Hawkes (Central Laser Facility RAL)

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