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@ARTICLE{pynucastro.joss.2018,
author = {{Willcox}, D.~E. and {Zingale}, M.},
title = "{pynucastro: an interface to nuclear reaction rates and code generator for reaction network equations}",
journal = {Journal of Open Source Software},
volume = {3},
number = {23},
pages = {588},
url = {https://doi.org/10.21105/joss.00588},
year = {2018}
}
@article{Reaclib.2010,
author={Richard H. Cyburt and A. Matthew Amthor and Ryan Ferguson
and Zach Meisel and Karl Smith and Scott Warren and
Alexander Heger and R. D. Hoffman and Thomas
Rauscher and Alexander Sakharuk and Hendrik Schatz
and F. K. Thielemann and Michael Wiescher},
title="{The JINA REACLIB Database: Its Recent Updates and Impact on Type-I X-ray Bursts}",
journal={The Astrophysical Journal Supplement Series},
volume={189},
number={1},
pages={240},
url={https://doi.org/10.1088/0067-0049/189/1/240},
year={2010}
}
@article{Suzuki.2016,
author={Toshio Suzuki and Hiroshi Toki and Ken'ichi Nomoto},
title="{Electron-capture and $\rm{\beta}$-decay Rates for sd-Shell Nuclei in Stellar Environments Relevant to High-density O-Ne-Mg Cores}",
journal={The Astrophysical Journal},
volume={817},
number={2},
pages={163},
url={https://doi.org/10.3847/0004-637x/817/2/163},
year={2016}
}
@article{CODATA.2014,
title = "{CODATA recommended values of the fundamental physical constants: 2014}",
author = {Mohr, Peter J. and Newell, David B. and Taylor, Barry N.},
journal = {Rev. Mod. Phys.},
volume = {88},
issue = {3},
pages = {035009},
numpages = {73},
year = {2016},
month = {Sep},
publisher = {American Physical Society},
doi = {10.1103/RevModPhys.88.035009},
url = {https://link.aps.org/doi/10.1103/RevModPhys.88.035009}
}
@misc{CODATA.2014.web,
title = "{The 2014 CODATA Recommended Values of the Fundamental Physical Constants (Web Version 7.2)}",
howpublished = {\url{https://physics.nist.gov/constants}},
note = {Accessed: 2018-01-27}
}
@article{AME2016.1,
author={W.J. Huang and G. Audi and Meng Wang and F.G. Kondev and S. Naimi and Xing Xu},
title="{The AME2016 atomic mass evaluation (I). Evaluation of input data; and adjustment procedures}",
journal={Chinese Physics C},
volume={41},
number={3},
pages={030002},
url={https://doi.org/10.1088/1674-1137/41/3/030002},
year={2017}
}
@article{AME2016.2,
author={Meng Wang and G. Audi and F.G. Kondev and W.J. Huang and S. Naimi and Xing Xu},
title="{The AME2016 atomic mass evaluation (II). Tables, graphs and references}",
journal={Chinese Physics C},
volume={41},
number={3},
pages={030003},
url={https://doi.org/10.1088/1674-1137/41/3/030003},
year={2017}
}
@article{AME2012.1,
author={G. Audi and M. Wang and A.H. Wapstra and F.G. Kondev and M. MacCormick and X. Xu and B. Pfeiffer},
title="{The Ame2012 atomic mass evaluation}",
journal={Chinese Physics C},
volume={36},
number={12},
pages={1287},
url={http://stacks.iop.org/1674-1137/36/i=12/a=002},
year={2012}
}
@article{AME2012.2,
author={M. Wang and G. Audi and A.H. Wapstra and F.G. Kondev and M. MacCormick and X. Xu and B. Pfeiffer},
title="{The Ame2012 atomic mass evaluation}",
journal={Chinese Physics C},
volume={36},
number={12},
pages={1603},
url={http://stacks.iop.org/1674-1137/36/i=12/a=003},
year={2012}
}
@article{Zingale.astronum.2017,
author={M. Zingale and A. S. Almgren and M. G. Barrios Sazo and V. E. Beckner and J. B. Bell and B. Friesen and A. M. Jacobs and M. P.
Katz and C. M. Malone and A. J. Nonaka and D. E. Willcox and W. Zhang},
title="{Meeting the Challenges of Modeling Astrophysical Thermonuclear Explosions: Castro, Maestro, and the AMReX Astrophysics Suite}",
journal={Journal of Physics: Conference Series},
volume={1031},
number={1},
pages={012024},
url={http://stacks.iop.org/1742-6596/1031/i=1/a=012024},
year={2018},
abstract={We describe the AMReX suite of astrophysics codes and their application to modeling problems in stellar astrophysics. Maestro is tuned to efficiently model subsonic convective flows while Castro models the highly compressible flows associated with stellar explosions. Both are built on the block-structured adaptive mesh refinement library AMReX. Together, these codes enable a thorough investigation of stellar phenomena, including Type Ia supernovae and X-ray bursts. We describe these science applications and the approach we are taking to make these codes performant on current and future many-core and GPU-based architectures.}
}
@article{VODE.1989,
author = {{Brown}, Peter N. and {Byrne}, George D. and {Hindmarsh}, Alan C.},
title = "{VODE: A Variable-Coefficient ODE Solver}",
journal = {SIAM Journal on Scientific and Statistical Computing},
volume = {10},
number = {5},
pages = {1038-1051},
year = {1989},
doi = {10.1137/0910062},
URL = {https://doi.org/10.1137/0910062},
eprint = {https://doi.org/10.1137/0910062}
}
@ARTICLE{Screening.Graboske.1973,
author = {{Graboske}, H.~C. and {Dewitt}, H.~E. and {Grossman}, A.~S. and
{Cooper}, M.~S.},
title = "{Screening Factors for Nuclear Reactions. II. Intermediate Screening and Astrophysical Applications}",
journal = {The Astrophysical Journal},
year = 1973,
month = apr,
volume = 181,
pages = {457-474},
doi = {10.1086/152062},
adsurl = {http://adsabs.harvard.edu/abs/1973ApJ...181..457G},
adsnote = {Provided by the SAO/NASA Astrophysics Data System}
}
@ARTICLE{Screening.Alastuey.1978,
author = {{Alastuey}, A. and {Jancovici}, B.},
title = "{Nuclear reaction rate enhancement in dense stellar matter}",
journal = {The Astrophysical Journal},
keywords = {Astrophysics, Magnetohydrodynamics, Nuclear Astrophysics, Reaction Kinetics, Thermonuclear Reactions, Correlation, Nuclei (Nuclear Physics), Perturbation Theory, Potential Theory, Quantum Mechanics},
year = 1978,
month = dec,
volume = 226,
pages = {1034-1040},
doi = {10.1086/156681},
adsurl = {http://adsabs.harvard.edu/abs/1978ApJ...226.1034A},
adsnote = {Provided by the SAO/NASA Astrophysics Data System}
}
@ARTICLE{Screening.Itoh.1979,
author = {{Itoh}, N. and {Totsuji}, H. and {Ichimaru}, S. and {Dewitt}, H.~E.
},
title = "{Enhancement of thermonuclear reaction rate due to strong screening. II - Ionic mixtures}",
journal = {The Astrophysical Journal},
keywords = {Nonuniform Plasmas, Reaction Kinetics, Thermonuclear Reactions, Astrophysics, Binary Mixtures, Dense Plasmas, Monte Carlo Method},
year = 1979,
month = dec,
volume = 234,
pages = {1079-1084},
doi = {10.1086/157590},
adsurl = {http://adsabs.harvard.edu/abs/1979ApJ...234.1079I},
adsnote = {Provided by the SAO/NASA Astrophysics Data System}
}
@article{SymPy.2017,
title = "{SymPy: symbolic computing in Python}",
author = {Meurer, Aaron and Smith, Christopher P. and Paprocki, Mateusz and \v{C}ert\'{i}k, Ond\v{r}ej 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 Rou\v{c}ka, \v{S}t\v{e}p\'{a}n and Saboo, Ashutosh and Fernando, Isuru and Kulal, Sumith and Cimrman, Robert and Scopatz, Anthony},
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.
},
volume = 3,
pages = {e103},
journal = {PeerJ Computer Science},
issn = {2376-5992},
url = {https://doi.org/10.7717/peerj-cs.103},
doi = {10.7717/peerj-cs.103}
}
@ARTICLE{MAESTRO:Multilevel,
author = {A. Nonaka and A. S. Almgren and J. B. Bell and M. J. Lijewski and C. M. Malone and M. Zingale},
title = {{\tt MAESTRO}:An Adaptive Low Mach Number Hydrodynamics Algorithm for Stellar Flows},
journal = {The Astrophysical Journal Supplement Series},
year = {2010},
volume = {188},
pages = {358-383},
note = {paper V},
url = {https://doi.org/10.1088/0067-0049/188/2/358}
}
@ARTICLE{castro,
author = {{Almgren}, A.~S. and {Beckner}, V.~E. and {Bell}, J.~B. and
{Day}, M.~S. and {Howell}, L.~H. and {Joggerst}, C.~C. and {Lijewski}, M.~J. and
{Nonaka}, A. and {Singer}, M. and {Zingale}, M.},
title = "{CASTRO: A New Compressible Astrophysical Solver. I. Hydrodynamics and Self-gravity}",
journal = {The Astrophysical Journal},
archivePrefix = "arXiv",
eprint = {1005.0114},
keywords = {equation of state, gravitation, hydrodynamics, methods:
numerical, nuclear reactions, nucleosynthesis,
abundances },
year = 2010,
month = jun,
volume = 715,
pages = {1221-1238},
doi = {10.1088/0004-637X/715/2/1221},
adsurl = {http://adsabs.harvard.edu/abs/2010ApJ...715.1221A},
adsnote = {Provided by the SAO/NASA Astrophysics Data System}
}
@ARTICLE{RaTh2000,
author = {{Rauscher}, T. and {Thielemann}, F.-K.},
title = "{Astrophysical Reaction Rates From Statistical Model Calculations}",
journal = {Atomic Data and Nuclear Data Tables},
eprint = {astro-ph/0004059},
year = 2000,
month = may,
volume = 75,
pages = {1-351},
doi = {10.1006/adnd.2000.0834},
adsurl = {http://adsabs.harvard.edu/abs/2000ADNDT..75....1R},
adsnote = {Provided by the SAO/NASA Astrophysics Data System}
}
@ARTICLE{Rauscher2003,
author = {{Rauscher}, T.},
title = "{Nuclear Partition Functions at Temperatures Exceeding 10$^{10}$ K}",
journal = {The Astrophysical Journal Supplement Series},
eprint = {astro-ph/0304047},
keywords = {Nuclear Reactions, Nucleosynthesis, Abundances},
year = 2003,
month = aug,
volume = 147,
pages = {403-408},
doi = {10.1086/375733},
adsurl = {http://adsabs.harvard.edu/abs/2003ApJS..147..403R},
adsnote = {Provided by the SAO/NASA Astrophysics Data System}
}
@ARTICLE{SkyNet.2017,
author = {{Lippuner}, J. and {Roberts}, L.~F.},
title = "{SkyNet: A Modular Nuclear Reaction Network Library}",
journal = {The Astrophysical Journal Supplement Series},
archivePrefix = "arXiv",
eprint = {1706.06198},
primaryClass = "astro-ph.HE",
keywords = {methods: numerical, nuclear reactions, nucleosynthesis, abundances },
year = 2017,
month = dec,
volume = 233,
eid = {18},
pages = {18},
doi = {10.3847/1538-4365/aa94cb},
adsurl = {http://adsabs.harvard.edu/abs/2017ApJS..233...18L},
adsnote = {Provided by the SAO/NASA Astrophysics Data System}
}