Abstract

Ion acceleration in electrostatic collisionless shocks is driven by the interaction of the high-power laser with specially tailored near-relativistic critical density plasma. 2D EPOCH particle-in-cell simulations show that the ion acceleration is dependent on the target material used. In materials with low charge-to-mass ratio.

Highlights

  • The development of high-intensity laser systems has opened a new era for laser-driven ions acceleration and there are several promising mechanisms for laser-driven ion acceleration

  • Ion acceleration in electrostatic collisionless shocks is driven by the interaction of the high-power laser with specially tailored near-relativistic critical density plasma. 2D EPOCH particle-in-cell simulations show that the ion acceleration is dependent on the target material used

  • The velocity distribution of the upstream expanding protons is further broadened toward the higher velocity by the electrostatic ion two-stream instability between reflected protons, which results in large number of protons being accelerated by the shock

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Summary

INTRODUCTION

The development of high-intensity laser systems has opened a new era for laser-driven ions acceleration and there are several promising mechanisms for laser-driven ion acceleration. The most widely understood mechanism is Target Normal Sheath Acceleration (TNSA) This mechanism [6] and a related radiation-pressure hybrid-scheme [7] can drive protons to energies approaching 100 MeV. Collisionless shock acceleration (CSA) has been proposed separately by Denavit [11] and Silva [12], with a detailed theoretical investigation complemented by Fiuza [13] These studies suggest that a special near-critical density profile, Ncr, is important in order to control the sheath electric field, ETNSA, at the plasma-vacuum interface. This in turn affects the ion spectrum in CSA. This paper is the first investigation on the material (or hZ=Ai) dependence of EITI on CSA

SIMULATIONS
Collisionless shock formation
Electrostatic ion two-stream instability
DISCUSSION AND SUMMARY
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