SkyNet: A Modular Nuclear Reaction Network Library

Almost all of the elements heavier than hydrogen that are present in our solar system were produced by nuclear burning processes either in the early universe or at some point in the life cycle of stars. In all of these environments, there are dozens to thousands of nuclear species that interact with...

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Published inThe Astrophysical journal. Supplement series Vol. 233; no. 2; pp. 18 - 48
Main Authors Lippuner, Jonas, Roberts, Luke F.
Format Journal Article
LanguageEnglish
Published Saskatoon The American Astronomical Society 01.12.2017
IOP Publishing
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ISSN0067-0049
1538-4365
DOI10.3847/1538-4365/aa94cb

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Abstract Almost all of the elements heavier than hydrogen that are present in our solar system were produced by nuclear burning processes either in the early universe or at some point in the life cycle of stars. In all of these environments, there are dozens to thousands of nuclear species that interact with each other to produce successively heavier elements. In this paper, we present SkyNet, a new general-purpose nuclear reaction network that evolves the abundances of nuclear species under the influence of nuclear reactions. SkyNet can be used to compute the nucleosynthesis evolution in all astrophysical scenarios where nucleosynthesis occurs. SkyNet is free and open source, and aims to be easy to use and flexible. Any list of isotopes can be evolved, and SkyNet supports different types of nuclear reactions. SkyNet is modular so that new or existing physics, like nuclear reactions or equations of state, can easily be added or modified. Here, we present in detail the physics implemented in SkyNet with a focus on a self-consistent transition to and from nuclear statistical equilibrium to non-equilibrium nuclear burning, our implementation of electron screening, and coupling of the network to an equation of state. We also present comprehensive code tests and comparisons with existing nuclear reaction networks. We find that SkyNet agrees with published results and other codes to an accuracy of a few percent. Discrepancies, where they exist, can be traced to differences in the physics implementations.
AbstractList Almost all of the elements heavier than hydrogen that are present in our solar system were produced by nuclear burning processes either in the early universe or at some point in the life cycle of stars. In all of these environments, there are dozens to thousands of nuclear species that interact with each other to produce successively heavier elements. In this paper, we present SkyNet, a new general-purpose nuclear reaction network that evolves the abundances of nuclear species under the influence of nuclear reactions. SkyNet can be used to compute the nucleosynthesis evolution in all astrophysical scenarios where nucleosynthesis occurs. SkyNet is free and open source, and aims to be easy to use and flexible. Any list of isotopes can be evolved, and SkyNet supports different types of nuclear reactions. SkyNet is modular so that new or existing physics, like nuclear reactions or equations of state, can easily be added or modified. Here, we present in detail the physics implemented in SkyNet with a focus on a self-consistent transition to and from nuclear statistical equilibrium to non-equilibrium nuclear burning, our implementation of electron screening, and coupling of the network to an equation of state. We also present comprehensive code tests and comparisons with existing nuclear reaction networks. We find that SkyNet agrees with published results and other codes to an accuracy of a few percent. Discrepancies, where they exist, can be traced to differences in the physics implementations.
Author Lippuner, Jonas
Roberts, Luke F.
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  orcidid: 0000-0002-5936-3485
  surname: Lippuner
  fullname: Lippuner, Jonas
  email: jlippuner@lanl.gov
  organization: Los Alamos National Laboratory Center for Theoretical Astrophysics, P.O. Box 1663, Los Alamos, NM, 87545, USA
– sequence: 2
  givenname: Luke F.
  orcidid: 0000-0001-7364-7946
  surname: Roberts
  fullname: Roberts, Luke F.
  organization: Michigan State University Department of Physics and Astronomy, East Lansing, MI 48824, USA
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Snippet Almost all of the elements heavier than hydrogen that are present in our solar system were produced by nuclear burning processes either in the early universe...
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SubjectTerms Equations of state
Hydrogen
methods: numerical
Nuclear fusion
Nuclear reactions
nuclear reactions, nucleosynthesis, abundances
Physics
Solar system
Stellar evolution
Title SkyNet: A Modular Nuclear Reaction Network Library
URI https://iopscience.iop.org/article/10.3847/1538-4365/aa94cb
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