Astrophysical S factor for the radiative capture 12N(p,gamma)13O determined from the 14N(12N,13O)13C...
Astrophysical S factor for the radiative capture 12N(p,gamma)13O determined from the 14N(12N,13O)13C proton transfer reaction
About this item
Full title
Author / Creator
Banu, A , Al-Abdullah, T , C Fu , Gagliardi, C A , McCleskey, M , Mukhamedzhanov, A M , Tabacaru, G , Trache, L , Tribble, R E , Zhai, Y , Carstoiu, F , Burjan, V and Kroha, V
Publisher
Ithaca: Cornell University Library, arXiv.org
Journal title
Language
English
Formats
Publication information
Publisher
Ithaca: Cornell University Library, arXiv.org
Subjects
More information
Scope and Contents
Contents
The cross section of the radiative proton capture reaction on the drip line nucleus 12N was investigated using the Asymptotic Normalization Coefficient (ANC) method. We have used the 14N(12N,13O)13C proton transfer reaction at 12 MeV/nucleon to extract the ANC for 13O -> 12N + p and calculate from it the direct component of the astrophysical S fact...
Alternative Titles
Full title
Astrophysical S factor for the radiative capture 12N(p,gamma)13O determined from the 14N(12N,13O)13C proton transfer reaction
Authors, Artists and Contributors
Identifiers
Primary Identifiers
Record Identifier
TN_cdi_proquest_journals_2087813228
Permalink
https://devfeature-collection.sl.nsw.gov.au/record/TN_cdi_proquest_journals_2087813228
Other Identifiers
E-ISSN
2331-8422
DOI
10.48550/arxiv.0811.0014
