AZURE: An<mml:math xmlns:mml="http://www.w3.org/1998/Math/MathML" display="inline"><mml:mrow><mml:mi>R</mml:mi></mml:mrow></mml:math>-matrix code for nuclear astrophysics
R.E. AzumaDepartment of Physics, University of Toronto, Toronto, Ontario M5S 1A7, CanadaE. UbersederUniversity of Notre Dame, Department of Physics, Notre Dame, Indiana 46556, USAE. C. SimpsonDepartment of Physics, Faculty of Engineering and Physical Sciences, University of Surrey, Guildford, Surrey GU2 7XH, United KingdomC. R. BruneDepartment of Physics and Astronomy, Ohio University, Ohio 45701, USAH. CostantiniIstituto Nazionale Fisica Nucleare (INFN), Genova, ItalyR. J. de BoerUniversity of Notre Dame, Department of Physics, Notre Dame, Indiana 46556, USAJ. GörresUniversity of Notre Dame, Department of Physics, Notre Dame, Indiana 46556, USAM. HeilGSI Darmstadt, Planckstr. 1, 64291 Darmstadt, GermanyP. J. LeBlancUniversity of Notre Dame, Department of Physics, Notre Dame, Indiana 46556, USAC. UgaldeUniversity of Notre Dame, Department of Physics, Notre Dame, Indiana 46556, USAM. WiescherUniversity of Notre Dame, Department of Physics, Notre Dame, Indiana 46556, USA
2010lv
ABI
Annotatsiya
The paper describes a multilevel, multichannel $R$-matrix code, AZURE, for applications in nuclear astrophysics. The code allows simultaneous analysis and extrapolation of low-energy particle scattering, capture, and reaction cross sections of relevance to stellar hydrogen, helium, and carbon burning. The paper presents a summary of $R$-matrix theory, code description, and a number of applications to demonstrate the applicability and versatility of AZURE.
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