2019
DOI: 10.1016/j.jcpx.2019.100030
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Active flux schemes on moving meshes with applications to geometric optics

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Cited by 2 publications
(6 citation statements)
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“…Recently, numerical schemes for Liouville's equation were developed that incorporate the optical interfaces. In [33] van Lith et al derived a first-order upwind finite difference scheme and in [32] van Lith et al introduced a third-order active flux finite volume scheme on moving meshes. The third-order active flux scheme was proved to be faster and more accurate compared to classical ray tracing for obtaining an energy distribution on phase space.…”
Section: Rtmentioning
confidence: 99%
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“…Recently, numerical schemes for Liouville's equation were developed that incorporate the optical interfaces. In [33] van Lith et al derived a first-order upwind finite difference scheme and in [32] van Lith et al introduced a third-order active flux finite volume scheme on moving meshes. The third-order active flux scheme was proved to be faster and more accurate compared to classical ray tracing for obtaining an energy distribution on phase space.…”
Section: Rtmentioning
confidence: 99%
“…This restriction invites us to use spherical coordinates to represent the momentum vector p as p = ( p, p z ) = n (sin θ cos ϕ, sin θ sin ϕ, cos θ ) , (7) where θ represents the polar angle, describing the angle between the z-axis and p measured from the z-axis, and ϕ the azimuthal angle for describing the direction in the q-plane. Therefore, at a given position z 0 along the optical axis, one can visualise the phase space coordinates on the screen that is perpendicular to the z-axis and intersects the z-axis at z 0 , where q is the position on the screen and p describes the projection of p on the screen [32]. The restriction of the momentum for physical rays p to Descartes' sphere also implies that the two-dimensional momentum vector is restricted by | p| ≤ n, describing a region known as Descartes' disc [35].…”
Section: Liouville's Equationmentioning
confidence: 99%
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“…Standard forward ray-tracing methods for geometrical optics, based on Monte Carlo methods with bin counting, are in general not energy conservative and exhibit a slow convergence. A recently new approach is based on a phasespace description of light, where each light ray propagating through an optical system evolves according to an optical Hamiltonian [1,2]. The 'time' parameter for Hamilton's equations can be the arc length of the ray, or in our case it will be the distance along a chosen optical axis, denoted by z.…”
Section: Introductionmentioning
confidence: 99%