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The Astrophysical Multipurpose Software Environment
Journal article   Open access   Peer reviewed

The Astrophysical Multipurpose Software Environment

F. I. Pelupessy, A. van Elteren, N. de Vries, S. L. W. McMillan, N. Drost and S. F. Portegies Zwart
Astronomy and astrophysics (Berlin), v 557, pp np-np
Sep 2013
url
https://doi.org/10.1051/0004-6361/201321252View
Published, Version of Record (VoR)Maybe Open Access (Publisher Bronze) Open

Abstract

hydrodynamics methods: numerical radiative transfer stars: evolution stars: kinematics and dynamics
We present the open source Astrophysical Multi-purpose Software Environment (AMUSE), a component library for performing astrophysical simulations involving different physical domains and scales. It couples existing codes within a Python framework based on a communication layer using MPI. The interfaces are standardized for each domain and their implementation based on MPI guarantees that the whole framework is well-suited for distributed computation. It includes facilities for unit handling and data storage. Currently it includes codes for gravitational dynamics, stellar evolution, hydrodynamics and radiative transfer. Within each domain the interfaces to the codes are as similar as possible. We describe the design and implementation of AMUSE, as well as the main components and community codes currently supported and we discuss the code interactions facilitated by the framework. Additionally, we demonstrate how AMUSE can be used to resolve complex astrophysical problems by presenting example applications.

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Astronomy & Astrophysics
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