Phantom
  • Getting started
  • User guide
  • Examples
    • Protoplanetary discs
    • Stellar relaxation
    • Binary stars and common envelope evolution
    • Tidal disruption events
    • Setting up a softened star
    • Running the dust settling test
    • Running a simulation with dust growth and fragmentation
    • Setting up hierarchical (triple) systems embedded in accretion discs
    • Simulation of self-gravitating and gravitationally unstable accretion discs
    • PhantomNR
    • Running a simulation with stellar wind and dust formation
    • Computing accretion rates from Phantom data
    • How to compute density on a set of particles with Phantom
  • External utilities
  • Physics guide
  • Developer guide
  • Frequently Asked Questions
  • Release notes
  • API Documentation
Phantom
  • Examples
  • View page source

Examples

This section contains some examples of physical problems that you can solve with Phantom.

Contents:

  • Protoplanetary discs
  • Stellar relaxation
  • Binary stars and common envelope evolution
  • Tidal disruption events
  • Setting up a softened star
  • Running the dust settling test
  • Running a simulation with dust growth and fragmentation
  • Setting up hierarchical (triple) systems embedded in accretion discs
  • Simulation of self-gravitating and gravitationally unstable accretion discs
  • PhantomNR
  • Running a simulation with stellar wind and dust formation
  • Computing accretion rates from Phantom data
  • How to compute density on a set of particles with Phantom
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