Abstract
We revisit the integer lattice (IL) method to numerically solve the Vlasov-Poisson equations, and show that a slight variant of the method is a very easy, viable, and efficient numerical approach to study the dynamics of self-gravitating, collisionless systems. The distribution function lives in a discretized lattice phase-space, and each time-step in the simulation corresponds to a simple permutation of the lattice sites. Hence, the method is Lagrangian, conservative, and fully time-reversible. IL complements other existing methods, such as N-body/ particle mesh (computationally efficient, but affected by Monte Carlo sampling noise and two-body relaxation) and finite volume (FV) direct integration schemes (expensive, accurate but diffusive). We also present improvements to the FV scheme, using a moving-mesh approach inspired by IL, to reduce numerical diffusion and the time-step criterion. Being a direct integration scheme like FV, IL is memory limited (memory requirement for a full 3D problem scales as N-6, where N is the resolution per linear phase- space dimension). However, we describe a new technique for achieving N-4 scaling. The method offers promise for investigating the full 6D phase- space of collisionless systems of stars and dark matter.
Anno
2017
Tipo pubblicazione
Altri Autori
Mocz, Philip; Succi, Sauro
Editore
Blackwell Scientific Publications
Rivista
Monthly notices of the Royal Astronomical Society (Print)