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Simulations of Dense Stellar Systems with the AMUSE Software Toolkit

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arxiv 1111.3987 v1 pith:IYDWHCJZ submitted 2011-11-16 astro-ph.IM astro-ph.GA

classification astro-ph.IMastro-ph.GA
keywords amuseframeworkstellarcomputationaldifferentdomainsdynamicsmodules
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We describe AMUSE, the Astrophysical Multipurpose Software Environment, a programming framework designed to manage multi-scale, multi-physics simulations in a hierarchical, extensible, and internally consistent way. Constructed as a collection of individual modules, AMUSE allows computational tools for different physical domains to be easily combined into a single task. It facilitates the coupling of modules written in different languages by providing inter-language tools and a standard programming interface that represents a balance between generality and computational efficiency. The framework currently incorporates the domains of stellar dynamics, stellar evolution, gas dynamics, and radiative transfer. We present some applications of the framework and outline plans for future development of the package.

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Cited by 2 Pith papers

Reviewed papers in the Pith corpus that reference this work. Sorted by Pith novelty score. OpenAlex reports about 5 citations worldwide. Full citation record

  1. Dynamical evolution and dissolution timescale of young stellar clusters in the Orion star-forming complex

    astro-ph.GA 2026-06 unverdicted novelty 5.0 of 10

    Gaia-derived parameters for 13 Orion clusters fed into N-body simulations reveal two regimes: seven with α_vir ≲ 7 retain bound cores for ≳170 Myr while six with α_vir ≳ 7 dissolve before 120 Myr.

  2. Population Synthesis of Gravitational Wave Sources

    astro-ph.HE 2025-02 accept novelty 1.0 of 10

    A review of population synthesis: the codes, the environments, and the predicted rates and features of gravitational wave sources, with an emphasis on breaking degeneracies.

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