2009
DOI: 10.1016/j.crhy.2009.03.002
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Theory and simulation of ion acceleration with circularly polarized laser pulses

Abstract: Ion acceleration driven by the radiation pressure of circularly polarized pulses is investigated via analytical modeling and particle-in-cell simulations. Both thick and thin targets, i.e. the "hole boring" and "light sail" regimes are considered. Parametric studies in one spatial dimension are used to determine the optimal thickness of thin targets and to address the effects of preformed plasma profiles and laser pulse ellipticity in thick targets. Three-dimensional (3D) simulations show that "flat-top" radia… Show more

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Cited by 19 publications
(9 citation statements)
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“…It is worth noting that CSA is different from hole-boring (HB) where ions are reflected by the charge-separation field that is built up due to purely piling-up of plasma electron density by the laser ponderomotive force (radiation pressure), where the plasma keeps opaque to the laser and the plasma temperature is rather low. As a result, both the HB velocity ( = v I mnc i i hb 3 ) and the reflected ion energy (ò i ∼I/m i n i c 3 ) are mainly determined by the laser intensity I (divided by the plasma density), where the plasma temperature has negligible contribution, and almost all ions are reflected to offset the charge-separation [14,[31][32][33][34]. However, CSA is based on the formation of an electrostatic shock that is typically associated with the excitation of ion acoustic waves in plasmas with cold ions and high electron temperatures, where the plasma is eventually transparent to the laser and an efficient plasma heating is the key factor.…”
Section: Introductionmentioning
confidence: 99%
“…It is worth noting that CSA is different from hole-boring (HB) where ions are reflected by the charge-separation field that is built up due to purely piling-up of plasma electron density by the laser ponderomotive force (radiation pressure), where the plasma keeps opaque to the laser and the plasma temperature is rather low. As a result, both the HB velocity ( = v I mnc i i hb 3 ) and the reflected ion energy (ò i ∼I/m i n i c 3 ) are mainly determined by the laser intensity I (divided by the plasma density), where the plasma temperature has negligible contribution, and almost all ions are reflected to offset the charge-separation [14,[31][32][33][34]. However, CSA is based on the formation of an electrostatic shock that is typically associated with the excitation of ion acoustic waves in plasmas with cold ions and high electron temperatures, where the plasma is eventually transparent to the laser and an efficient plasma heating is the key factor.…”
Section: Introductionmentioning
confidence: 99%
“…A more detailed analysis shows that electron heating is quenched when the parameter exceeds some threshold value, seeMacchi et al (2009b) andRykovanov et al (2008).…”
mentioning
confidence: 99%
“…At mechanical equilibrium, i.e. in the so-called regime of ponderomotive acceleration 48 , we have . Consequently, the equation of motion for radially accelerated ions can be recast as 49 : where A and Z are the ion mass number and the atomic number, respectively.…”
Section: Pic Simulation Results and Analytical Estimatesmentioning
confidence: 99%
“…The ion density spike splits up rapidly (see Fig. 6 b) and a short bunch of fast ions is generated 48 . The onset of hydrodynamical breaking causes the formation of an ambipolar sheath field with a sharp gradient, around the breaking point (i.e.…”
Section: Pic Simulation Results and Analytical Estimatesmentioning
confidence: 99%