Thermonuclear reaction rate libraries and software tools for nuclear astrophysics research

被引：0

作者：

Smith, Michael S. ^{[1
]}

Cyburt, Richard ^{[2
]}

Schatz, Hendrik ^{[2
]}

Wiescher, Michael ^{[3
]}

Smith, Karl ^{[2
]}

Warren, Scott ^{[2
]}

Ferguson, Ryan ^{[2
]}

Lingerfelt, Eric ^{[1
,4
]}

Buckner, Kim ^{[1
,4
]}

Nesaraja, Caroline D. ^{[1
,4
]}

机构：

[1] Oak Ridge Natl Lab, Div Phys, Oak Ridge, TN 37831 USA

[2] Michigan State Univ, Dept Phys & Astron, Natl Superconduct Cyclotron Lab, E Lansing, MI 48824 USA

[3] Univ Notre Dame, Dept Phys, Notre Dame, IN 46556 USA

[4] Univ Tennessee, Dept Phys & Astron, Knoxville, TN 37996 USA

来源：

ORIGIN OF MATTER AND EVOLUTION OF GALAXIES | 2008年 / 1016卷

基金：

美国国家科学基金会;

关键词：

reaction rate; nucleosynthesis; stellar modeling; software; nuclear data; evaluations;

D O I：

暂无

中图分类号：

P1 [天文学];

学科分类号：

0704 ;

摘要：

Thermonuclear reaction rates are a crucial input for simulating a wide variety of astrophysical environments. A new collaboration has been formed to ensure that astrophysical modelers have access to reaction rates based on the most recent experimental and theoretical nuclear physics information. To reach this goal, a new version of the REACLIB library has been created by the Joint Institute for Nuclear Astrophysics (JINA), now available online at http://www.nscl.msu.edu/-nero/db. A complementary effort is the development of software tools in the Computational Infrastructure for Nuclear Astrophysics, online at nucastrodata.org, to streamline, manage, and access the workflow of the reaction evaluations from their initiation to peer review to incorporation into the library. Details of these new projects will be described.

引用

页码：466 / +

页数：2