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 in | The Astrophysical journal. Supplement series Vol. 233; no. 2; pp. 18 - 48 |
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Main Authors | , |
Format | Journal Article |
Language | English |
Published |
Saskatoon
The American Astronomical Society
01.12.2017
IOP Publishing |
Subjects | |
Online Access | Get full text |
ISSN | 0067-0049 1538-4365 |
DOI | 10.3847/1538-4365/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. |
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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. |
Author_xml | – sequence: 1 givenname: Jonas 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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ContentType | Journal Article |
Copyright | 2017. The American Astronomical Society. All rights reserved. Copyright IOP Publishing Dec 2017 |
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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 |
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