S. K. Nielsen
Research Interests
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Articles (18)
Three-wave interactions may occur in media with quadratic nonlinearities, which allow for a flow of power between linear waves. The interactions require selection rules similar to conservation of energy and momentum to be satisfied. Equations are presented to solve these selection rules efficiently along the ray trajectory of a pump wave via integration similar to how ray trajectories are determined numerically. This is convenient when dealing with large amplitude beams which may interact with waves along its trajectory. Reformulating the selection rules as a system of ODEs means that the selection rules may be solved using dispersion relations for the three waves, even if the dispersion relations cannot be solved for frequency or wavevector, which would otherwise be needed. In numerical implementations, root-finding algorithms, which may be unstable for complicated dispersion relations, can be avoided. A simple set of equations valid in one-dimensional are presented first. The corresponding equations in arbitrary dimension, including 2D and 3D, are then derived. A set of equations are also derived to find different solutions to the selection rules at a fixed point. Examples with the derived equations applied to plasma physics are presented.
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2024
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2024
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2024
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2024
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2023
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2023
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2023
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2023
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2023
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2023
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2022
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2022
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2022
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2022
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2022
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2021
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2021
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2021
Collaborators (10)
Miklos Vecsei
Max-Planck-Institut für Plasmaphysik Teilinstitut Greifswald
Alexander Simon Thrysøe
Technical University of Denmark
Thomas Jensen
Technical University of Denmark
Riccardo Ragona
Danmarks Tekniske Universitet
Jesper Rasmussen
Technical University of Denmark
Umesh Kumar
EPFL (École Polytechnique Fédérale de Lausanne)
Laurent Krier
Max-Planck-Institut für Plasmaphysik Teilinstitut Greifswald
Anders Henry Nielsen
Technical University of Denmark
Roddy Vann
Professor of Physics & Director of the EPSRC Centre for Doctoral Training in Fusion Power
University of York
Søren Bang Korsholm
Technical University of Denmark
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