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CITATION
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MAESTROeX derives from MAESTRO. When citing the code, please cite the
two primary algorithm papers below as well as any of the MAESTRO
papers appropriate to the discussion.
@ARTICLE{2019ApJ...887..212F,
author = {{Fan}, Duoming and {Nonaka}, Andrew and {Almgren}, Ann S. and
{Harpole}, Alice and {Zingale}, Michael},
title = "{MAESTROeX: A Massively Parallel Low Mach Number Astrophysical Solver}",
journal = {\apj},
keywords = {Stellar convective zones, Hydrodynamics, Computational methods, Nuclear astrophysics, Nucleosynthesis, Nuclear abundances, Physics - Computational Physics, Astrophysics - Solar and Stellar Astrophysics},
year = "2019",
month = "Dec",
volume = {887},
number = {2},
eid = {212},
pages = {212},
doi = {10.3847/1538-4357/ab4f75},
archivePrefix = {arXiv},
eprint = {1908.03634},
primaryClass = {physics.comp-ph},
adsurl = {https://ui.adsabs.harvard.edu/abs/2019ApJ...887..212F},
adsnote = {Provided by the SAO/NASA Astrophysics Data System}
}
@ARTICLE{2010ApJS..188..358N,
author = {{Nonaka}, A. and {Almgren}, A.~S. and {Bell},
J.~B. and {Lijewski}, M.~J. and {Malone}, C.~M. and
{Zingale}, M.},
title = "{MAESTRO: An Adaptive Low Mach Number Hydrodynamics
Algorithm for Stellar Flows}",
journal = {\apjs},
archivePrefix = "arXiv",
eprint = {1005.0112},
primaryClass = "astro-ph.IM",
keywords = {convection, hydrodynamics, methods: numerical,
nuclear reactions, nucleosynthesis, abundances,
supernovae: general, white dwarfs},
year = 2010,
month = jun,
volume = 188,
pages = {358-383},
doi = {10.1088/0067-0049/188/2/358},
adsurl = {http://adsabs.harvard.edu/abs/2010ApJS..188..358N},
adsnote = {Provided by the SAO/NASA Astrophysics Data System}
}
For the software itself, please cite the JOSS paper:
@ARTICLE{2019JOSS....4.1757F,
author = {{Fan}, Duoming and {Nonaka}, Andrew and {Almgren}, Ann and
{Willcox}, Donald and {Harpole}, Alice and {Zingale}, Michael},
title = "{MAESTROeX: A Massively Parallel Low Mach Number Astrophysical Solver}",
journal = {The Journal of Open Source Software},
keywords = {abundances, supernovae, Fortran, Fortran90, nucleosynthesis, C++, Python, Jupyter Notebook, nuclear reactions, hydrodynamics, convection},
year = "2019",
month = "Nov",
volume = {4},
number = {43},
eid = {1757},
pages = {1757},
doi = {10.21105/joss.01757},
adsurl = {https://ui.adsabs.harvard.edu/abs/2019JOSS....4.1757F},
adsnote = {Provided by the SAO/NASA Astrophysics Data System}
}
There are several other papers that may be appropriate to cite,
depending on which capabilities you are using. These are discussed
below.
The development of the low Mach number formulation is described in the
following papers -- we ask that they be cited if you are discussing
the low Mach asymptotics or expansion of the background state (paper
II in particular):
@ARTICLE{2006ApJ...637..922A,
author = {{Almgren}, A.~S. and {Bell}, J.~B. and {Rendleman},
C.~A. and {Zingale}, M.},
title = "{Low Mach Number Modeling of Type Ia
Supernovae. I. Hydrodynamics}",
journal = {\apj},
eprint = {astro-ph/0509892},
keywords = {Convection, Hydrodynamics, Methods: Numerical,
Nuclear Reactions, Nucleosynthesis, Abundances,
Stars: Supernovae: General, Stars: White Dwarfs},
year = 2006,
month = feb,
volume = 637,
pages = {922-936},
doi = {10.1086/498426},
adsurl = {http://adsabs.harvard.edu/abs/2006ApJ...637..922A},
adsnote = {Provided by the SAO/NASA Astrophysics Data System}
}
@ARTICLE{2006ApJ...649..927A,
author = {{Almgren}, A.~S. and {Bell}, J.~B. and {Rendleman},
C.~A. and {Zingale}, M.},
title = "{Low Mach Number Modeling of Type Ia
Supernovae. II. Energy Evolution}",
journal = {\apj},
eprint = {astro-ph/0606496},
keywords = {Convection, Hydrodynamics, Methods: Numerical, Nuclear
Reactions, Nucleosynthesis, Abundances, Stars:
Supernovae: General, Stars: White Dwarfs},
year = 2006,
month = oct,
volume = 649,
pages = {927-938},
doi = {10.1086/507089},
adsurl = {http://adsabs.harvard.edu/abs/2006ApJ...649..927A},
adsnote = {Provided by the SAO/NASA Astrophysics Data System}
}
@ARTICLE{2008ApJ...684..449A,
author = {{Almgren}, A.~S. and {Bell}, J.~B. and {Nonaka},
A. and {Zingale}, M. },
title = "{Low Mach Number Modeling of Type Ia
Supernovae. III. Reactions}",
journal = {\apj},
keywords = {convection, hydrodynamics, methods: numerical,
nuclear reactions, nucleosynthesis, abundances,
supernovae: general, white dwarfs },
year = 2008,
month = sep,
volume = 684,
eid = {449-470},
pages = {449-470},
doi = {10.1086/590321},
adsurl = {http://adsabs.harvard.edu/abs/2008ApJ...684..449A},
adsnote = {Provided by the SAO/NASA Astrophysics Data System}
}
If you use diffusion, we appreciate citing the following paper which
introduced the diffusion algorithm:
@ARTICLE{2011ApJ...728..118M,
author = {{Malone}, C.~M. and {Nonaka}, A. and {Almgren},
A.~S. and {Bell}, J.~B. and {Zingale}, M.},
title = "{Multidimensional Modeling of Type I X-ray
Bursts. I. Two-dimensional Convection Prior to the
Outburst of a Pure $^{4}$He Accretor}",
journal = {\apj},
archivePrefix = "arXiv",
eprint = {1012.0609},
primaryClass = "astro-ph.HE",
keywords = {convection, hydrodynamics, methods: numerical, stars:
neutron, X-rays: bursts},
year = 2011,
month = feb,
volume = 728,
eid = {118},
pages = {118},
doi = {10.1088/0004-637X/728/2/118},
adsurl = {http://adsabs.harvard.edu/abs/2011ApJ...728..118M},
adsnote = {Provided by the SAO/NASA Astrophysics Data System}
}
If you are dealing with a spherical geometry, we appreciate citing
this paper, which describes the spherical geometry:
@ARTICLE{2009ApJ...704..196Z,
author = {{Zingale}, M. and {Almgren}, A.~S. and {Bell},
J.~B. and {Nonaka}, A. and {Woosley}, S.~E.},
title = "{Low Mach Number Modeling of Type IA
Supernovae. IV. White Dwarf Convection}",
journal = {\apj},
archivePrefix = "arXiv",
eprint = {0908.2668},
primaryClass = "astro-ph.HE",
keywords = {convection, hydrodynamics, methods: numerical,
nuclear reactions, nucleosynthesis, abundances,
supernovae: general, white dwarfs},
year = 2009,
month = oct,
volume = 704,
pages = {196-210},
doi = {10.1088/0004-637X/704/1/196},
adsurl = {http://adsabs.harvard.edu/abs/2009ApJ...704..196Z},
adsnote = {Provided by the SAO/NASA Astrophysics Data System}
}