| Literature DB >> 34903823 |
S Petrakis1,2, M Bakarezos2,3, M Tatarakis2,4, E P Benis5, N A Papadogiannis6,7.
Abstract
The quantum phases of the electron paths driven by an ultrafast laser in high harmonic generation in an atomic gas depends linearly on the instantaneous cycle-averaged laser intensity. Using high laser intensities, a complete single ionisation of the atomic gas may occur before the laser pulse peak. Therefore, high harmonic generation could be localised only in a temporal window at the leading edge of laser pulse envelope. Varying the laser frequency chirp of an intense ultrafast laser pulse, the centre, and the width of the temporal window, that the high harmonic generation phenomenon occurs, could be controlled with high accuracy. This way, both the duration and the phase of the electron trajectories, that generate efficiently high harmonics, is fully controlled. A method of spectral control and selection of the high harmonic extreme ultraviolet light from distinct quantum paths is experimentally demonstrated. Furthermore, a phenomenological numerical model enlightens the physical processes that take place. This novel approach of the electron quantum path selection via laser chirp is a simple and versatile way of controlling the time-spectral characteristics of the coherent extreme ultraviolet light with applications in the fields of attosecond pulses and soft x-ray nano-imaging.Entities:
Year: 2021 PMID: 34903823 PMCID: PMC8668923 DOI: 10.1038/s41598-021-03424-3
Source DB: PubMed Journal: Sci Rep ISSN: 2045-2322 Impact factor: 4.379
Figure 1Schematic layout of HHG experiments performed with femtosecond high intensity chirped IR Ti:Sa laser pulses. Femtosecond amplified laser pulses are chirped by varying the spacing between the compressor gratings (CG). Laser high harmonics are generated after focusing the chirped laser pulses on a semi-infinite noble gas (Ar) cell. High harmonic spectra are measured by an XUV CCD camera after IR filtering by silicon wafers (Si-W) and XUV dispersion by a flat-field XUV concave grating (FFG). (a) HHG E-fields for three cases of chirped laser pulses having the same energy; (a1) Fourier limited (unchirped) pulses; (a2) Low negatively chirped pulses; (a3) High negatively chirped pulses. Note that HHG occurs at the same laser pulse intensity (controlled by electron ionisation) corresponding to different time instants of the laser intensity envelope. (b) [Bottom] Schematic of electron trajectories within an E-field laser period leading to the recollision with the parent nucleus. [Top] HHG spectral images from long and short electron trajectories exhibiting different spectral and geometrical characteristics. D: Adjustable grating distance; M: Low dispersion fs mirror; L: Low dispersion thin focusing lens.
Figure 2(a) Representative measurements of XUV harmonic spectral images for various laser pulse durations controlled by the imposed chirp. The harmonics spectral locations, estimated according to the experimental setup optical geometry, are noted at the bottom of the figure. Negative and positive signs of the laser pulses durations correspond to negative and positive laser pulse chirp, respectively. The spectral separation between the short and long trajectories, indicated by the letters “” and “s” in the spectral images, respectively, is clearly demonstrated for certain chirp values. Note that for the duration of +33 fs, the long trajectories contribution to the HHG is severely suppressed, thus leaving only the HHG by short trajectories in the spectral image. (b) XUV harmonic spectra obtained with our model calculations corresponding to the experimental conditions of their counterpart XUV harmonic spectral images in (a). Both short and long trajectory contributions, as well as their coherent addition, are presented. It is seen that the calculations fairly reproduce the main qualitative characteristics of the measured spectral images. Note that the 17th and 15th order harmonics are seen to be strongly suppressed in the experimental spectral images due to their strong absorption by the Ar gas, a condition not included in the simulations.
Figure 3Details of our model calculations corresponding to the cases presented in Fig. 2. Black line: Laser intensity; Blue line: Laser angular frequency accounting for the linear laser chirp and SPM effects in the non-linear Ar medium and the plasma; Green line: ionisation probability of Ar according to the ADK model; Red line: Generated XUV radiation E-field, arbitrarily scaled along the y-axis in each graph for presentation purposes.