SWIFT: SPH With Inter-dependent Fine-grained Tasking
0.9
  • 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
    • Basic model (others)
    • AGN jets and black hole spin in hydrodynamical simulations
  • 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
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  • Galaxy Formation Subgrid Models
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Galaxy Formation Subgrid Models

Multiple models are available in SWIFT. The ‘Basic’ model can be use as an empty canvas to be copied to create additional models.

Available models:

  • EAGLE model
    • Gas entropy floors
    • Chemical tracers
    • Gas cooling: Wiersma+2009a
    • Particle tracers
    • Star formation: Schaye+2008 modified for EAGLE
    • Stellar enrichment: Wiersma+2009b
    • Supernova feedback: Dalla Vecchia+2012 & Schaye+2015
    • Supernova and enrichment parameters in the EAGLE-Ref model
    • Black-hole creation
    • Black-hole accretion
    • Black-hole repositioning
    • AGN feedback
  • Quick Lyman-alpha (QLA) model
    • Gas entropy floor
    • Gas cooling: Wiersma+2009a with fixed primordial metallicity
    • Star formation
  • GEAR model
    • Pressure Floor
    • Cooling: Grackle
    • Star formation
    • Chemistry
    • Feedback
  • Basic model (others)
    • Cooling: Analytic models
  • AGN jets and black hole spin in hydrodynamical simulations
    • Model summary
    • Compiling and running the model
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