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024 7 _ |a 10.1063/1.4994705
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024 7 _ |a 1089-7674
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037 _ _ |a FZJ-2017-05054
041 _ _ |a English
082 _ _ |a 530
100 1 _ |a Siddi, Lorenzo
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245 _ _ |a Mesh-free Hamiltonian implementation of two dimensional Darwin model
260 _ _ |a [S.l.]
|c 2017
|b American Institute of Physics
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520 _ _ |a A new approach to Darwin or magnetoinductive plasma simulation is presented, which combines amesh-free field solver with a robust time-integration scheme avoiding numerical divergence errorsin the solenoidal field components. The mesh-free formulation employs an efficient parallelBarnes-Hut tree algorithm to speed up the computation of fields summed directly from the particles,avoiding the necessity of divergence cleaning procedures typically required by particle-incellmethods. The time-integration scheme employs a Hamiltonian formulation of the Lorentzforce, circumventing the development of violent numerical instabilities associated with time differentiationof the vector potential. It is shown that a semi-implicit scheme converges rapidly and isrobust to further numerical instabilities which can develop from a dominant contribution of the vectorpotential to the canonical momenta. The model is validated by various static and dynamicbenchmark tests, including a simulation of the Weibel-like filamentation instability in beam-plasmainteractions.
536 _ _ |a 511 - Computational Science and Mathematical Methods (POF3-511)
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536 _ _ |a Kinetic Plasma Simulation with Highly Scalable Particle Codes (jzam04_20130501)
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|f Kinetic Plasma Simulation with Highly Scalable Particle Codes
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588 _ _ |a Dataset connected to CrossRef
700 1 _ |a Lapenta, Giovanni
|0 0000-0002-3123-4024
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700 1 _ |a Gibbon, Paul
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773 _ _ |a 10.1063/1.4994705
|g Vol. 24, no. 8, p. 082103 -
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|t Physics of plasmas
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|y 2017
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856 4 _ |y Published on 2017-07-20. Available in OpenAccess from 2018-07-20.
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856 4 _ |y Published on 2017-07-20. Available in OpenAccess from 2018-07-20.
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856 4 _ |y Published on 2017-07-20. Available in OpenAccess from 2018-07-20.
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