Abstract

We have studied energy distribution of fast electrons passing through a highly compressed core plasma for fast ignition research in inertial confinement fusion. Recent PIC calculations indicate that the collective effect of electric and magnetic fields on the transport may be less significant than the binary collisions in the case of a high density fusion pellet. In order to understand the net effect of binary collisions in dense plasma, we calculate electron energy distributions at several viewing angles using an electromagnetic cascade Monte-Carlo simulation, EGS5, for estimation of the contribution of multi collisional process. Here, the construction of physical parameters in the code were taken from the calculation results given by 2 dimensional particle-in-cell simulations. In the result, the number of electrons detected on the laser axis within the range to 15 MeV significantly decreases for the superdense region (max: 1.6 · 10 25 (/cm 3 )) compared with the low density plasma. The reduction on the electron number decreases with increase of observation angles gradually and finally the number almost coincides more than 40 degrees.

Highlights

  • In Fast ignition [1] in inertial confinement fusion research, it is one of the key issues to heat the compressed core plasma by fast electrons generated via ultraintense laser pulse

  • We have studied energy distribution of fast electrons passing through a highly compressed core plasma for fast ignition research in inertial confinement fusion

  • In order to understand the net effect of binary collisions in dense plasma, we calculate electron energy distributions at several viewing angles using an electromagnetic cascade Monte-Carlo simulation, Electron Gamma Shower 5 (EGS5), for estimation of the contribution of multi collisional process

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Summary

INTRODUCTION

In Fast ignition [1] in inertial confinement fusion research, it is one of the key issues to heat the compressed core plasma by fast electrons generated via ultraintense laser pulse. The estimation of electron energy distributions is crucially important for understanding of heating processes to the core plasma. EPJ Web of Conferences via ionization and electron propagation direction is shifted by multiple scattering, resulting that the electromagnetic cascade shower happens. In EGS5, the type of Fredholm transportation equation is used as a basis for the electromagnetic cascade shower and can treat multiple scattering under completely ionized plasma

SIMULATION SET UP
Initial particle condition
Material condition
Inhomogeneous vs homogenous
Effect of emission divergence
CONCLUSION
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