Title of article
DWBA momentum distribution and its effect on THM Original Research Article
Author/Authors
M. La Cognata، نويسنده , , C. Spitaleri، نويسنده , , A. Mukhamedzhanov، نويسنده , , V. Goldberg، نويسنده , , B. Irgaziev، نويسنده , , L. Lamia، نويسنده , , R.G. Pizzone، نويسنده , , M.L. Sergi، نويسنده , , R.E. Tribble، نويسنده ,
Issue Information
هفته نامه با شماره پیاپی سال 2010
Pages
3
From page
658
To page
660
Abstract
The 18O(p,α)15N reaction is of primary importance to pin down the uncertainties affecting present-day models of asymptotic giant branch stars. An indirect measurement of the low-energy region of the 18O(p,α)15N reaction has been performed by means of the Trojan Horse Method. We discuss why the plane wave approximation is justified by evaluating what changes the more correct DWBA approach introduces.
Journal title
Nuclear physics A
Serial Year
2010
Journal title
Nuclear physics A
Record number
1205879
Link To Document