2010
DOI: 10.1063/1.3353050
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Enhanced relativistic harmonics by electron nanobunching

Abstract: It is shown that when an few-cycle, relativistically intense, p-polarized laser pulse is obliquely incident on overdense plasma, the surface electrons may form ultra-thin, highly compressed layers, with a width of a few nanometers. These electron "nanobunches" emit synchrotron radiation coherently. We calculate the one-dimensional synchrotron spectrum analytically and obtain a slowly decaying power-law with an exponent of 4/3 or 6/5. This is much flatter than the 8/3 power of the BGP (Baeva-Gordienko-Pukhov) s… Show more

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Cited by 164 publications
(158 citation statements)
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“…Furthermore, based on the phenomenological assumption of electron nanobunches appearing in the plasma and emitting radiation, it was shown in Ref. [21] that the spectra can be much flatter than predicted by the OMM. Moreover, the OMM assumes as a prerequisite that the incident and backradiated amplitudes at the ARP are equal, in accordance with the Leontovich boundary conditions (which is in direct correspondence to the local energy conservation).…”
Section: Introductionmentioning
confidence: 99%
“…Furthermore, based on the phenomenological assumption of electron nanobunches appearing in the plasma and emitting radiation, it was shown in Ref. [21] that the spectra can be much flatter than predicted by the OMM. Moreover, the OMM assumes as a prerequisite that the incident and backradiated amplitudes at the ARP are equal, in accordance with the Leontovich boundary conditions (which is in direct correspondence to the local energy conservation).…”
Section: Introductionmentioning
confidence: 99%
“…In figures 6(a-d) the radiation spectra for various combinations of the parameter S are shown, and where the power decay indexes 5/3 are observed for these cases. Figure 6(c) shows for comparison a PIC harmonic spectrum from an ultrarelativistic laser-plasma interaction, characterized by a ∼4/3 power decay index, reported by other authors [13]. …”
Section: Plasma and Harmonic Emission From Relativistic Electrons Permentioning
confidence: 99%
“…The situation for HHG from plasma surfaces is similar to HHG from noble gases; a circularly polarized laser pulse is generally not suitable to generate circularly polarized laser harmonics. Under normal incidence geometry, it is not efficient in driving the motion of electron population at plasma surfaces which is required to Doppler upshift the laser fundamental frequency [17][18][19]. Under oblique incidence, although a circularly polarized incident laser has equal energy in its p− and s−polarized components, the harmonic yields from these two polarization components are not the same.…”
Section: Introductionmentioning
confidence: 99%
“…In fact, the field has become a focus of research in the nonlinear optics of HHG. Compared to HHG from noble gases, HHG from plasma surfaces [10][11][12][13][14][15][16][17][18][19][20][21][22][23][24][25][26][27][28] does not subject to the limitation of maximum applied laser intensity and can thus use the state-of-the-art terawatt and petawatt laser technology, which will improve attosecond pulse energy, making it potentially useful to pump-probe experiments [29]. There is a strong motivation to seek circularly polarized attosecond XUV light source by HHG from plasma surfaces.…”
Section: Introductionmentioning
confidence: 99%