SWIFT: SPH With Inter-dependent Fine-grained Tasking
Disclaimer, Citing SWIFT & Giving Credit
Getting Started
Command line options
Parameter Files
Initial Conditions
Snapshots
Hydrodynamics Schemes
Time integration details
Galaxy Formation Subgrid Models
EAGLE model
Quick Lyman-alpha (QLA) model
GEAR model
Pressure Floor
Star formation
Cooling: Grackle
Chemistry
Stellar evolution and feedback
GEAR supernova feedback
Sink particles and star formation in GEAR model
Introduction
Compiling and running the model
Model summary
Sink timesteps
Model parameters
Snapshots ouputs
Basic model (others)
AGN jets and black hole spin in hydrodynamical simulations
AGORA model
Planetary Simulations
Friends-Of-Friends (FOF) Halo Finder
VELOCIraptor Interface
Line-of-sights outputs
Light Cone Outputs
Equations of State
External Potentials
Neutrino implementation
Radiative Transfer Schemes
General information for adding new schemes
Task System
Analysis Tools
Continuous Simulation Data Stream (CSDS)
Implementation details
SWIFT: SPH With Inter-dependent Fine-grained Tasking
Galaxy Formation Subgrid Models
GEAR model
Sink particles and star formation in GEAR model
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Sink particles and star formation in GEAR model
Table of Contents
Introduction
Compiling and running the model
Model summary
Conversion from comoving to physical space
Sink formation
Gas accretion
Sink merging
IMF sampling
Star spawning
Stellar feedback
Sink timesteps
Sink 2-body encounters
Timesteps per sink’s age categories
Star formation constraint
Model parameters
Sink accretion radius
Guide to choose the the accretion radius or the density threshold
Comment on star formation efficiency