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Relativistic Surface High Harmonic Generation
A route to intense attosecond pulses ? Christian Rödel, Silvio Fuchs, Martin Heyer, Oliver Jäckel, Gerhard G. Paulus FSU Jena, Institut für Optik und Quantenelektronik, Helmholtz Institut Jena Michael Behmke, Toma Toncian, Dirk Hemmers, Mirela Cercez, Monika Toncian, Georg Pretzler, Oswald Willi HHU Düsseldorf, Institut für Laser- und Plasmaphysik Daniel an der Brügge, Alexander Pukhov HHU Düsseldorf, Institut für Theoretische Physik
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Attosecond science - Introduction
Hentschel et al.: Attosecond metrology, Nature 2007 shortest attosecond pulses: 80 as E. Goulielmakis et al. Science, 320, 1614 (2008)
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High harmonic generation in gases
3-step model: (a) ionization, (b,c) motion of the free electron in the laser field, (d) recollision Corkum, Krausz: Attosecond science, Nature 2007
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High Harmonic Spectra HHG spectrum in Neon, 50 fs, 1014 W/cm²
Agostini, DiMauro: The physics of attosecond light pulses, Reports on Progress in Physics
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But… … laser pulses were getting stronger
Small-scale TW laser systems, Ti:Sapphire 800nm, 10 Hz JETI IOQ: 27 fs, 800mJ ARCTURUS ILPP: 27 fs, 2.5 J 30% of laser energy in a 7µm2 focus I=1020 W/cm2
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What happens at an ideal surface at Relativistic intensity ?
Corkum, Krausz: Attosecond science, Nature 2007
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Relativistic surface High harmonic generation
PIC simulation with LPIC JETI laser parameters: a0=4.5, t=80fs, ° p-pol incidence lambda/20 scale length oscillating plasma vacuum boundary
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Relativistic surface High harmonic generation
intensity harmonic number
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Steep density gradient – high contrast laser pulses
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High contrast laser pulses – plasma mirror
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High contrast laser pulses - Plasma mirror
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High contrast laser pulses - Plasma mirror
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High contrast laser pulses - scale length
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Experimental setup @ arcturus
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Diagnostics - XUV Spectrometer
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Experimental spectra with different contrast
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Experimental spectra with different contrast
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Where does the modulation come from?
space / wavelength
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Where does the modulation come from?
space / wavelength
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… Unequal temporal spacing of the attosecond pulse train ?
sdf superposition of attosecond pulses emitted at times tk with assumed identical shape spectrum is given by the absolute square of the Fourier transform plasma surface motion can be approximated by a simple parabola, which corresponds to a linear chirp with emission times
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… Unequal temporal spacing of the attosecond pulse train
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… Unequal temporal spacing of the attosecond pulse train…
… describes the spectral modulations indirect evidence of attosecond time structure of relativistic surface harmonics !!! And just as a outlook …
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… according to the same Pic simulations ...
… they are very short (100as)
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Thank you for your attention
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