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SWIFT: SPH With Inter-dependent Fine-grained Tasking

Posted: Thu May 24, 2018 9:27 pm
by Ada Coda
SWIFT: SPH With Inter-dependent Fine-grained Tasking

Abstract: SWIFT runs cosmological simulations on peta-scale machines for solving gravity and SPH. It uses the Fast Multipole Method (FMM) to calculate gravitational forces between nearby particles, combining these with long-range forces provided by a mesh that captures both the periodic nature of the calculation and the expansion of the simulated universe. SWIFT currently uses a single fixed but time-variable softening length for all the particles. Many useful external potentials are also available, such as galaxy haloes or stratified boxes that are used in idealised problems. SWIFT implements a standard LCDM cosmology background expansion and solves the equations in a comoving frame; equations of state of dark-energy evolve with scale-factor. The structure of the code allows implementation for modified-gravity solvers or self-interacting dark matter schemes to be implemented. Many hydrodynamics schemes are implemented in SWIFT and the software allows users to add their own.

Credit: Schaller, Matthieu; Gonnet, Pedro; Draper, Peter W.; Chalk, Aidan B. G.; Bower, Richard G.; Willis, James; Hausammann, Loïc


Bibcode: 2018ascl.soft05020S

Preferred citation method: Please see citation information here: ... t-citation

ID: ascl:1805.020