The Astrophysical Multipurpose Software Environment¶
Contents:
- Installation
- Tutorials
- Working with Units
- Quantities
- Working with arrays
- Estimating the typical mass of the most massive star in a cluster
- Working with Particle Sets
- Integrate a C++ code
- Integrate a Fortran 90 code
- Adding a Gravitational Dynamics Code
- Create an low-level Interface to a Code
- Plotting with amuse
- Setting values for grid boundaries
- Interactive tutorial
- Reference documentation
- Quantities and Units
- Datamodel
- Particle Attributes
- Currently supported Community Codes
- Reporting during a run
- Stopping Conditions
- Asynchronous calls
- Bridge
- Supported File Formats
- Input / Output Framework
- Directory Structure
- Sets and Grids in Codes
- Interface Specifications
- Simplified interface function specification
- Options
- From Codes to Data
- Support code for AMUSE framework
- Support code for the community code interfaces
- Message protocol between python and community codes
- Distributed AMUSE
- Setting up GPGPU with CUDA
- Running AMUSE on The Cartesius supercomputer
- Running AMUSE through slurm
- AMUSE Style Guide
- Source Code Management
- Glossary
- Design documentation