Investigating the use of field solvers for simulating classical systems
arXiv:2001.05791 · doi:10.1103/PhysRevD.101.043011
Abstract
We explore the use of field solvers as approximations of classical Vlasov-Poisson systems. This correspondence is investigated in both electrostatic and gravitational contexts. We demonstrate the ability of field solvers to be excellent approximations of problems with cold initial condition into the non linear regime. We also investigate extensions of the Schrödinger-Poisson system that employ multiple stacked cold streams, and the von Neumann-Poisson equation as methods that can successfully reproduce the classical evolution of warm initial conditions. We then discuss how appropriate simulation parameters need to be chosen to avoid interference terms, aliasing, and wave behavior in the field solver solutions. We present a series of criteria clarifying how parameters need to be chosen in order to effectively approximate classical solutions.
arXiv comment28 pages, 14 figures. Matches published version Phys. Rev. D
References in corpus (23)
- The cosmological simulation code GADGET-2
- Cold and Fuzzy Dark Matter
- Matrix Product Density Operators: Simulation of finite-T and dissipative systems
- Cosmic Structure as the Quantum Interference of a Coherent Dark Wave
- Mixed-state dynamics in one-dimensional quantum lattice systems: a time-dependent superoperator renormalization algorithm
- Understanding the Core-Halo Relation of Quantum Wave Dark Matter, DM, from 3D Simulations
- Galaxy Formation with BECDM: I. Turbulence and relaxation of idealised haloes
- Gravitational Bose-Einstein condensation in the kinetic regime
- A Review on the Scalar Field/ Bose-Einstein Condensate Dark Matter Model
- High-Resolution Simulation on Structure Formation with Extremely Light Bosonic Dark Matter
- Statistical Effects in the Multistream Model for Quantum Plasmas
- On the Schrodinger-Poisson--Vlasov-Poisson correspondence
- A new approach to simulating collisionless dark matter fluids
- Spiral Instabilities in N-body Simulations I: Emergence from Noise
- Schrödinger method as N-body double and UV completion of dust
- Direct Integration of the Collisionless Boltzmann Equation in Six-dimensional Phase Space: Self-gravitating Systems
- Solving the Vlasov equation in two spatial dimensions with the Schrödinger method
- Stable interpolation with isotropic and anisotropic Gaussians using Hermite generating function
- A massively parallel semi-Lagrangian solver for the six-dimensional Vlasov-Poisson equation
- Coarse-scale representations and smoothed Wigner transforms
- Gravitational collapse in the Schrödinger-Poisson system
- Particle-in-cell simulations of the relaxation of electron beams in inhomogeneous solar wind plasmas
- A new framework for numerical simulations of structure formation
Cited by in corpus (6)
- Large-scale dark matter simulations
- Relaxation times for Bose-Einstein condensation in axion miniclusters
- A hierarchical field-level inference approach to reconstruction from sparse Lyman- forest data
- Cosmological Vlasov-Poisson equations for dark matter: Recent developments and connections to selected plasma problems
- One-Dimensional Fuzzy Dark Matter Models: Structure Growth and Asymptotic Dynamics
- When quantum corrections alter the predictions of classical field theory for scalar field dark matter