Hostname: page-component-78c5997874-g7gxr Total loading time: 0 Render date: 2024-11-20T05:40:19.345Z Has data issue: false hasContentIssue false
  • English
  • Français

The R-matrix Method in Nuclear Astrophysics

Published online by Cambridge University Press:  27 September 2007

M. Busso ,
R.G. Pizzone ,
C. Rolfs ,
C. Spitaleri ,
A. Tumino  and
P. Descouvemont
P. Descouvemont*
Affiliation:
Physique Nucléaire Théorique et Physique Mathématique, CP 229, Université Libre de Bruxelles, 1050 Brussels, Belgium
*
[email protected]
Get access

Abstract

We present a short overview of the R-matrix method in nuclear physics, with emphasis on nuclear astrophysics.The method can be applied in two ways: solving the Schrödinger equation for scattering states, orfitting experimental cross sections. Both variants are presented in a common framework. The methodis illustrated with the α + α scattering, and the 12C(p,γ)13N and 3He(d,p)4He reactions.

Type
Research Article
Information
European Astronomical Society Publications Series , Volume 27: The Third European Summer School on Experimental Nuclear Astrophysics , 2007 , pp. 67 - 81
Copyright
© EAS, EDP Sciences, 2007

Access options

Get access to the full version of this content by using one of the access options below. (Log in options will check for institutional or personal access. Content may require purchase if you do not have access.)