By Peter Hommelhoff, Matthias Kling
The 1st huge and in-depth review of present learn in attosecond nanophysics, overlaying the sphere of lively plasmonics through attosecond technology in metals and dielectrics to novel imaging options with the top spatial and temporal resolution.
The authors are pioneers within the box and current the following new advancements and power novel purposes for ultra-fast information verbal exchange and processing, discussing the research of the typical timescale of electron dynamics in nanoscale reliable kingdom systems.
either an creation for beginning graduate scholars, in addition to a glance on the present cutting-edge during this scorching and rising box.
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Extra info for Attosecond Nanophysics: From Basic Science to Applications
The dashed green line indicates the noise ﬂoor caused by dark counts from the electron multiplier. Interestingly, no plasma line contributions for wavelengths larger than 95 nm are found in the spectrum. However, a pronounced peak at 90 nm is present, which does not directly coincide with xenon plasma lines. 4. 15 Measured spectra in xenon with 200 nm bow-tie antennae at a backing pressure of 200 mbar. Grey background shading indicates harmonic orders of the driving laser, whereas orange lines represent xenon plasma lines and their respective relative intensities.
On the basis of available experimental data also a considerably reduced harmonic yield in case of nano-antenna assisted EUV generation was concluded. Recently, additional experiments carried out by Sivis et al.  demonstrate a suﬃcient ﬁeld enhancement exhibited by the nano antennae to reach intensities necessary for HHG to occur. In experiments carried out with an ampliﬁer system at identical peak intensities as in the respective ones based on nano antennae, HHG in combination with atomic line emission is observed.
15b was measured with the grating with a design wavelength from 110 to 310 nm due to alignment purposes. 15b has not been corrected for it. Also note that the central wavelength is slightly shifted to 810 nm. The dashed green line indicates the noise ﬂoor caused by dark counts from the electron multiplier. Interestingly, no plasma line contributions for wavelengths larger than 95 nm are found in the spectrum. However, a pronounced peak at 90 nm is present, which does not directly coincide with xenon plasma lines.