ws.bib

%comment{This file was created with betterbib v4.0.6.}


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@article{HEGER_ETAL07B,
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@article{Bell:2004,
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@article{almgren:2000,
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@article{timmes_swesty:2000,
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 note = {Source code obtained from http://cococubed.asu.edu/codes/eos.shtml/helmholtz.tbz},
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}

@article{timmes_aprox13,
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@phdthesis{Lin:2005,
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 title = {Implementing the Low Mach Number Approximation for Multidimensional Hydrodynamical Modeling of Type I X-Ray Bursts},
 school = {Field of Physics and Astronomy, Northwestern University},
 year = {2005},
 month = may,
}

@article{ABRZ:I,
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 pages = {922-936},
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 publisher = {American Astronomical Society},
 issn = {0004-637X, 1538-4357},
}

@article{ABRZ:II,
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 journal = {ApJ},
 year = {2006},
 volume = {649},
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 month = oct,
 note = {paper II},
 doi = {10.1086/507089},
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 publisher = {American Astronomical Society},
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}

@article{ABNZ:III,
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 note = {paper III},
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 publisher = {American Astronomical Society},
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@article{ZABNW:IV,
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@article{MAESTRO:Multilevel,
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@article{Lin:2006,
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@article{HEG_ETAL07,
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 publisher = {American Astronomical Society},
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 source = {Crossref},
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@article{MUNO_ETAL02,
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 publisher = {American Astronomical Society},
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@article{HEGER_ETAL00,
 author = {Heger, A. and Langer, N. and Woosley, S. E.},
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 publisher = {American Astronomical Society},
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@article{ARNETT_ETAL09,
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 keywords = {Astrophysics - Solar and Stellar Astrophysics},
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 publisher = {American Astronomical Society},
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 acmid = {1251845},
 publisher = {Institute of Electrical and Electronics Engineers (IEEE)},
 address = {Piscataway, NJ, USA},
 keywords = {Python, Python, scripting languages, application development, scientific programming, application development, scientific programming, scripting languages},
 source = {Crossref},
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 publisher = {Institute of Electrical and Electronics Engineers (IEEE)},
 address = {Piscataway, NJ, USA},
 keywords = {Python, Python, computer languages, scientific programming, scientific computing, computer languages, scientific computing, scientific programming},
 source = {Crossref},
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 primaryclass = {astro-ph.IM},
 keywords = {Hydrodynamics, Methods: numerical},
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 author = {Meurer, Aaron and Smith, Christopher P. and Paprocki, Mateusz and Čertík, Ondřej and Kirpichev, Sergey B. and Rocklin, Matthew and Kumar, AMiT and Ivanov, Sergiu and Moore, Jason K. and Singh, Sartaj and Rathnayake, Thilina and Vig, Sean and Granger, Brian E. and Muller, Richard P. and Bonazzi, Francesco and Gupta, Harsh and Vats, Shivam and Johansson, Fredrik and Pedregosa, Fabian and Curry, Matthew J. and Terrel, Andy R. and Roučka, Štěpán and Saboo, Ashutosh and Fernando, Isuru and Kulal, Sumith and Cimrman, Robert and Scopatz, Anthony},
 title = {SymPy: Symbolic computing in Python},
 year = {2017},
 month = jan,
 keywords = {Python, Computer algebra system, Symbolics},
 abstract = {SymPy is an open source computer algebra system written in pure Python. It is built with a focus on extensibility and ease of use, through both interactive and programmatic applications. These characteristics have led SymPy to become a popular symbolic library for the scientific Python ecosystem. This paper presents the architecture of SymPy, a description of its features, and a discussion of select submodules. The supplementary material provide additional examples and further outline details of the architecture and features of SymPy.},
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@ARTICLE{eiden:2020,
       author = {{Eiden}, Kiran and {Zingale}, Michael and {Harpole}, Alice and {Willcox}, Donald and {Cavecchi}, Yuri and {Katz}, Max P.},
        title = "{Dynamics of Laterally Propagating Flames in X-Ray Bursts. I. Burning Front Structure}",
      journal = {\apj},
     keywords = {1814, 1131, 1866, 1963, 1965, 767, 1108, 1129, Astrophysics - High Energy Astrophysical Phenomena},
         year = 2020,
        month = may,
       volume = {894},
       number = {1},
          eid = {6},
        pages = {6},
          doi = {10.3847/1538-4357/ab80bc},
archivePrefix = {arXiv},
       eprint = {1912.04956},
 primaryClass = {astro-ph.HE},
       adsurl = {https://ui.adsabs.harvard.edu/abs/2020ApJ...894....6E},
      adsnote = {Provided by the SAO/NASA Astrophysics Data System}
}

@ARTICLE{harpole:2021,
       author = {{Harpole}, A. and {Ford}, N.~M. and {Eiden}, K. and {Zingale}, M. and {Willcox}, D.~E. and {Cavecchi}, Y. and {Katz}, M.~P.},
        title = "{Dynamics of Laterally Propagating Flames in X-Ray Bursts. II. Realistic Burning and Rotation}",
      journal = {\apj},
     keywords = {X-ray bursts, Nucleosynthesis, Open source software, Hydrodynamics, Hydrodynamical simulations, Neutron stars, Computational methods, 1814, 1131, 1866, 1963, 767, 1108, 1965, Astrophysics - High Energy Astrophysical Phenomena},
         year = 2021,
        month = may,
       volume = {912},
       number = {1},
          eid = {36},
        pages = {36},
          doi = {10.3847/1538-4357/abee87},
archivePrefix = {arXiv},
       eprint = {2102.00051},
 primaryClass = {astro-ph.HE},
       adsurl = {https://ui.adsabs.harvard.edu/abs/2021ApJ...912...36H},
      adsnote = {Provided by the SAO/NASA Astrophysics Data System}
}

@article{castro_joss,
  doi = {10.21105/joss.02513},
  url = {https://doi.org/10.21105/joss.02513},
  year = {2020},
  publisher = {The Open Journal},
  volume = {5},
  number = {54},
  pages = {2513},
  author = {Ann Almgren and Maria Barrios Sazo and John Bell and Alice Harpole and Max Katz and Jean Sexton and Donald Willcox and Weiqun Zhang and Michael Zingale},
  title = {CASTRO: A Massively Parallel Compressible Astrophysics Simulation Code},
  journal = {Journal of Open Source Software}
}

@inproceedings{castro_gpu,
   author = {Katz, Max P. and Almgren, Ann and Sazo, Maria Barrios and
                  Eiden, Kiran and Gott, Kevin and Harpole, Alice and
                  Sexton, Jean M. and Willcox, Don E. and Zhang,
                  Weiqun and Zingale, Michael},
   title = {Preparing Nuclear Astrophysics for Exascale},
   year = {2020},
   isbn = {9781728199986},
   publisher = {IEEE Press},
   abstract = {Astrophysical explosions such as supernovae are
                  fascinating events that require sophisticated
                  algorithms and substantial computational power to
                  model. Castro and MAESTROeX are nuclear astrophysics
                  codes that simulate thermonuclear fusion in the
                  context of supernovae and X-ray bursts. Examining
                  these nuclear burning processes using high
                  resolution simulations is critical for understanding
                  how these astrophysical explosions occur. In this
                  paper we describe the changes that have been made to
                  these codes to transform them from standard MPI +
                  OpenMP codes targeted at petascale CPU-based systems
                  into a form compatible with the pre-exascale systems
                  now online and the exascale systems coming soon. We
                  then discuss what new science is possible to run on
                  systems such as Summit and Perlmutter that could not
                  have been achieved on the previous generation of
                  supercomputers.},
booktitle = {Proceedings of the International Conference for High
                  Performance Computing, Networking, Storage and
                  Analysis},
articleno = {91},
numpages = {12},
keywords = {gravity, hydrodynamics, computational fluid dynamics, adaptive mesh refinement, nuclear reactions, astrophysics},
location = {Atlanta, Georgia},
series = {SC '20},
  subject = {high-performance computing},
   url = {https://dl.acm.org/doi/abs/10.5555/3433701.3433822}
}