Title of article
Indirect study of 19Ne states near the image threshold Original Research Article
Author/Authors
N. de Séréville، نويسنده , , A. Coc، نويسنده , , C. Angulo، نويسنده , , M. Assunç?o، نويسنده , , D. Beaumel، نويسنده , , E. Berthoumieux، نويسنده , , B. Bouzid، نويسنده , , S. Cherubini، نويسنده , , M. Couder، نويسنده , , P. Demaret، نويسنده , , F. de Oliveira Santos، نويسنده , , P. Figuera، نويسنده , , Gary S. Fortier ، نويسنده , , M. Gaelens، نويسنده , , F. Hammache، نويسنده , , J. Kiener، نويسنده , , A. Lefebvre-Schuhl، نويسنده , , D. Labar، نويسنده , , P. Leleux، نويسنده , , M. Loiselet، نويسنده , , et al.، نويسنده ,
Issue Information
هفته نامه با شماره پیاپی سال 2007
Pages
16
From page
251
To page
266
Abstract
The early E⩽511 keV gamma-ray emission from novae depends critically on the View the MathML source reaction. Unfortunately the reaction rate of the View the MathML source reaction is still largely uncertain due to the unknown strengths of low-lying proton resonances near the View the MathML source threshold which play an important role in the nova temperature regime. We report here our last results concerning the study of the View the MathML source transfer reaction. We show in particular that these two low-lying resonances cannot be neglected. These results are then used to perform a careful study of the remaining uncertainties associated to the View the MathML source and View the MathML source reaction rates.
Keywords
related features , DWBA , astrophysical implications discussed , Nuclear reactions , View the MathML source , E=14 MeV , Measured , EP , ?(E , ?) , E? , 19F deduced , analog states spectroscopic factors , analysis
Journal title
Nuclear physics A
Serial Year
2007
Journal title
Nuclear physics A
Record number
1204913
Link To Document