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Revealing quantum path details in high-field physics
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2014 (engelsk)Inngår i: Physical Review A. Atomic, Molecular, and Optical Physics, ISSN 1050-2947, E-ISSN 1094-1622, Vol. 90, nr 1, artikkel-id 013822Artikkel i tidsskrift (Fagfellevurdert) Published
Abstract [en]

The fundamental mechanism underlying harmonic emission in the strong-field regime is governed by tunnel ionization of the atom, followed by the motion of the electron wave packet in the continuum, and finally by its recollision with the atomic core. Due to the quantum nature of the process, the properties of the electron wave packet strongly correlate with those of the emitted radiation. Here, by spatially resolving the interference pattern generated by overlapping the harmonic radiation emitted by different interfering electron quantum paths, we have succeeded in unravelling the intricacies associated with the recollision process. This has been achieved by mapping the spatial extreme-ultraviolet (EUV)-intensity distribution onto a spatial ion distribution, produced in the EUV focal area through the linear and nonlinear processes of atoms. By in situ manipulation of the intensity-dependent motion of the electron wave packets, we have been able to directly measure the difference between the harmonic emission times and electron path lengths resulting from different electron trajectories. Due to the high degree of accuracy that the present approach provides, we have been able to demonstrate the quantum nature of the recollision process. This is done by quantitatively correlating the photoemission time and the electron quantum path-length differences, taking into account the energy-momentum transfer from the driving laser field into the system. This information paves the way for electron-photon correlation studies at the attosecond time scale, while it puts the recollision process from the semiclassical prospective into a full quantum-mechanical context.

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American Physical Society, 2014. Vol. 90, nr 1, artikkel-id 013822
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URN: urn:nbn:se:umu:diva-134420DOI: 10.1103/PhysRevA.90.013822ISI: 000339443600007OAI: oai:DiVA.org:umu-134420DiVA, id: diva2:1093445
Tilgjengelig fra: 2017-05-06 Laget: 2017-05-06 Sist oppdatert: 2018-06-09bibliografisk kontrollert

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