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title: 'pynucastro: an interface to nuclear reaction rates and code generator for reaction network equations' | ||
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tags: | ||
- nuclear | ||
- reactions | ||
- astrophysics | ||
- physics | ||
- integration | ||
- differential equations | ||
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authors: | ||
- name: AMReX-Astro Microphysics Development Team | ||
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affiliations: | ||
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date: 27 January 2018 | ||
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bibliography: paper.bib | ||
--- | ||
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# Summary | ||
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The AMReX-Astrophysics Microphysics library provides a common set of | ||
microphysics routines (reaction networks, equations of state, and | ||
other transport coefficients) for astrophysical simulation codes built | ||
around the AMReX library. | ||
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# History | ||
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This project started out as Starkiller Microphysics, which was an | ||
attempt to codevelop microphysics routines for the Castro and Flash | ||
simulation codes. Originally the library used Fortran and was | ||
restricted to CPUs, but C++ ports were added over time to take | ||
advantage of GPU-offloading afforded by the AMReX library. Eventually | ||
as the development of the two codes diverged, the C++ ports of the | ||
Microphysis were split off into the AMReX-Astrophysics Microphysics | ||
library. Today, the library is completely written in C++ and relies | ||
on the AMReX data structures. | ||
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# Design | ||
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Porting many classic solvers from old Fortran to C++ | ||
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header-only library as much as possible | ||
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C++17 | ||
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pynucastro integration | ||
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# Capabilities | ||
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# Unit tests / examples | ||
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# References | ||
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