Bulletin of the American Physical Society
60th Annual Meeting of the APS Division of Plasma Physics
Volume 63, Number 11
Monday–Friday, November 5–9, 2018; Portland, Oregon
Session YO8: Space and Astrophysical Plasmas
9:30 AM–12:06 PM,
Friday, November 9, 2018
OCC
Room: C120-122
Chair: Li-Jen Chen, NASA Goddard
Abstract ID: BAPS.2018.DPP.YO8.13
Abstract: YO8.00013 : Fully conservative scheme for relativistic Landau–Fokker–Planck equation*
11:54 AM–12:06 PM
Presenter:
Takashi Shiroto
(Osaka Univ)
Authors:
Takashi Shiroto
(Osaka Univ)
Takashi Asahina
(Osaka Univ)
Yasuhiko Sentoku
(Osaka Univ)
In our previous work, a charge-momentum-energy-conserving algorithm was developed for the relativistic Vlasov–Maxwell system by the finite-difference method [T. Shiroto et al., arXiv 1802.07238 (2018)]. The scheme is based on the central difference scheme, so numerical dissipations are not included in the algorithm. This is why we extend the conservative algorithm to the relativistic Vlasov–Fokker–Planck–Maxwell system in order to introduce the effect of dissipation by the collision terms. In the non-relativistic regime, a conservative scheme has already been developed [W.T. Taitano et al., JCP 297, 357 (2015)], and our approach is similar to theirs but based on the potential equations of Braams and Karney [B.J. Braams and C.F.F. Karney, PRL 59, 1817 (1987)]. At the moment, a mass-momentum-energy-conserving scheme for the relativistic Landau–Fokker–Planck equation is composed with explicit time integration, and one-dimensional and three-velocity-components numerical experiments are performed. However, our conservative Vlasov–Maxwell scheme is based on an implicit time integration. Therefore, we will improve the conservative scheme with the combination of the implicit scheme and the Jacobian-Free Newton–Krylov method.
*This work was supported by KAKENHI (15K21767).
To cite this abstract, use the following reference: http://meetings.aps.org/link/BAPS.2018.DPP.YO8.13
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