105 / 2023-04-13 21:13:59
Quasistatic simulations of long-distance laser wakefield acceleration
simulations,laser wakefield acceleration,plasma
Abstract Pending
Konstantin Lotov / Novosibirsk State University;Budker Institute of Nuclear Physics
Daniil Kutergin / Novosibirsk State University
Igor Lotov / Novosibirsk State University
Roman Spitsyn / Novosibirsk State University;Budker Institute of Niclear Physics
Petr Tuev / Novosibirsk State University;Budker Institute of Niclear Physics
Laser-driven plasma wakefield acceleration (LWFA) is a promising technology for compact sources of high-energy electron beams. With advent of more powerful laser systems, new parameter regions for LWFA become accessible, including relatively low plasma densities that provide higher energies and charges of accelerated bunches. Numerical simulations of a plasma accelerator operating at low plasma densities are computationally demanding because of the large ratio of laser frequency w0 to the plasma frequency wp, especially if the driver is channeled and the acceleration distance is long.

If the frequency ratio w0/wp is large, it is especially advantageous to use a quasistatic code and the envelope model of the laser pulse for numerical simulations. The envelope equation increases the temporal and spatial scales to be resolved by a factor of w0/wp. Accordingly, it is possible to increase the simulation grid step and reduce the simulation time. The quasistatic approximation additionally allows increasing the grid step along the longitudinal coordinate by the ratio of Rayleigh length to plasma wavelength, i.e., by another w0/wp times. However, in order to correctly simulate strongly depleted laser pulses, the time step of the grid must be further reduced by a factor of w0/wp. Thus, the quasistatic approximation combined with the envelope model for the laser pulse gives a w02/wp2 times speedup of calculations compared to simulations without simplifying assumptions by the particle-in-cell (PIC) method.

As an example, we consider the acceleration of electrons in a long plasma channel with a single drive laser pulse, the parameters of which correspond to the discussed project XCELS. The maximum electron energy reaches 91 GeV at a plasma density of 3 1015 cm-3 and a bunch charge of 50 pC. The quasistatic code (LCODE) allows to simulate the driver evolution with high accuracy up to the termination of acceleration, which is confirmed by controlling the energy balance of the system. A typical run requires about 103 CPU hours, and the use of the reduced models gives a speedup of 6 orders of magnitude compared to the traditional PIC method.

 
Important Date
  • Conference Date

    Jun 05

    2023

    to

    Jun 09

    2023

  • Apr 30 2023

    Early Bird Registration

  • May 01 2023

    Abstract Submission Deadline

  • May 01 2023

    Abstract Notification of Acceptance

  • May 01 2023

    Draft paper submission deadline

  • May 31 2023

    Registration deadline

Sponsored By
Science and Technology on Plasma Physics Laboratory
Department of Astronomy, Beijing Normal University
Organized By
Matter and Radiation at Extremes
Institute of Fluid Physics, China Academy of Engineering Physics, China
Institute of Applied Physics and Computational Mathematics, Beijing, China
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