2013
DOI: 10.1117/12.2017379
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Simulation studies of radiation pressure-driven light sail and shock acceleration

Abstract: Simulation results are reported for two ion acceleration mechanisms driven by radiation pressure. Threedimensional (3D) simulations of the acceleration of thin foils by circularly polarized pulses ("light sail" regime) at ultra-relativistic intensities (a 0 > 100) show an ion energy that is higher than observed in 1D and 2D simulations, presumably due to density rarefaction and self-wrapping of the laser pulse as the foil is deformed. Simulations of the interaction of linearly polarized pulses with long-scalel… Show more

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(4 citation statements)
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“…The electrons are assumed to be isothermal so that the electron number density obeys the Boltzmann distribution of the form [45] n e (φ, φ max ) = n i (0, φ max ) exp(φ/θ), (7) where θ = T e /T i . Equation (7) ensures that n e = n i when φ = 0. It should be noted that kinetic models for the electrons have been used both in the non-relativistic [32,47] and relativistic [49,50] regimes; to obtain Eq.…”
Section: Kinetic Shock Modelmentioning
confidence: 99%
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“…The electrons are assumed to be isothermal so that the electron number density obeys the Boltzmann distribution of the form [45] n e (φ, φ max ) = n i (0, φ max ) exp(φ/θ), (7) where θ = T e /T i . Equation (7) ensures that n e = n i when φ = 0. It should be noted that kinetic models for the electrons have been used both in the non-relativistic [32,47] and relativistic [49,50] regimes; to obtain Eq.…”
Section: Kinetic Shock Modelmentioning
confidence: 99%
“…is Dawson's integral. The electrons are assumed to be isothermal so that the electron number density obeys the Boltzmann distribution of the form [45] n e (φ, φ max ) = n i (0, φ max ) exp(φ/θ), (7) where θ = T e /T i . Equation (7) ensures that n e = n i when φ = 0.…”
Section: Kinetic Shock Modelmentioning
confidence: 99%
See 2 more Smart Citations