Publication | Closed Access
Emergence from nonrelativistic strong-field rescattering to ultrastrong-field laser-atom physics: A semiclassical analysis
51
Citations
44
References
2006
Year
Nonrelativistic Strong-field RescatteringEngineeringLaser ScienceLaser-plasma InteractionRelativistic PlasmaPlasma PhysicsUltrastrong-field Rescattering DynamicsUltrastrong-field Laser-atom PhysicsQuantum SciencePhysicsRelativistic Laser-matter InteractionAtomic PhysicsCosmic RaySemiclassical AnalysisSynchrotron RadiationUltrastrong-field InteractionNatural SciencesParticle PhysicsApplied PhysicsRescattering Deflection Parameter
We discuss a rescattering deflection parameter to gauge the progression from strong- to ultrastrong-field rescattering dynamics. Our analytical and numerical treatments of rescattering quantify the change from nonrelativistic, dipole approximation strong-field dynamics to an ultrastrong-field interaction where $v∕c\ensuremath{\ne}0$ and ${\mathbf{B}}_{\text{laser}}\ensuremath{\ne}0$. At the threshold between these two regimes the Lorentz deflection reduces the returning electron flux at the core and suppresses rescattering related phenomena. Both radiation and nonsequential ionization from rescattering are studied. We show the ultrastrong-field regime can occur at intensities as low as ${10}^{14}\phantom{\rule{0.3em}{0ex}}\mathrm{W}∕{\mathrm{cm}}^{2}$ for mid-IR $(2\phantom{\rule{0.3em}{0ex}}\ensuremath{\mu}\mathrm{m}\phantom{\rule{0.3em}{0ex}}\text{to}\phantom{\rule{0.3em}{0ex}}5\phantom{\rule{0.3em}{0ex}}\ensuremath{\mu}\mathrm{m})$ wavelengths or as high as ${10}^{18}\phantom{\rule{0.3em}{0ex}}\mathrm{W}∕{\mathrm{cm}}^{2}$ for UV radiation.
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