An efficient nonclassical quadrature for the calculation of nonresonant nuclear fusion reaction rate coefficients from cross section data

被引:0
|
作者
Shizgal, Bernie D. [1 ,2 ]
机构
[1] Univ British Columbia, Dept Chem, 2036 Main Mall, Vancouver, BC V6T 1Z1, Canada
[2] Univ British Columbia, Inst Appl Math, Vancouver, BC V6T 1Z1, Canada
关键词
Nonclassical polynomials; Quadrature; Astrophysical factor; Nuclear reaction rate coefficient; DISCRETIZATION METHOD; EQUATION; COMPILATION; NUCLEOSYNTHESIS;
D O I
10.1016/j.cpc.2016.04.008
中图分类号
TP39 [计算机的应用];
学科分类号
081203 ; 0835 ;
摘要
Nonclassical quadratures based on a new set of half-range polynomials, T-n(x), orthogonal with respect to w(x) = e(-x-b/root x) for x epsilon [0, infinity) are employed in the efficient calculation of the nuclear fusion reaction rate coefficients from cross section data. The parameter b = B/root k(B)T in the weight function is temperature dependent and B is the Gamow factor. The polynomials T-n(x) satisfy a three term recurrence relation defined by two sets of recurrence coefficients, alpha(n) and beta(n). These recurrence coefficients define in turn the tridiagonal Jacobi matrix whose eigenvalues are the quadrature points and the weights are calculated from the first components of the eigenfunctions. For nonresonant nuclear reactions for which the astrophysical function can be expressed as a lower order polynomial in the relative energy, the convergence of the thermal average of the reactive cross section with this nonclassical quadrature is extremely rapid requiring in many cases 2-4 quadrature points. The results are compared with other libraries of nuclear reaction rate coefficient data reported in the literature. (C) 2016 Elsevier B.V. All rights reserved.
引用
收藏
页码:61 / 68
页数:8
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