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Nuclear astrophysics studiesat dragon: The...

Nuclear astrophysics studiesat dragon: The 21Na(p,γ)22Mg reaction and oxygen-neon novae

Abstract

The rate of the 21Na(p,γ)22Mg reaction is expected to play a major role in the nucleosynthesis of 22Na in Oxygen-Neon novae, leading to the emission of a characteristic 1.28 MeV gamma-line. This paper reports on preliminary results of the first direct measurements of this reaction and its astrophysical implications.

Authors

Bishop S; Azuma R; Buchmann L; Chen AA; Chatterjee ML; D'Auria JM; Engel S; Gigliotti D; Greife U; Hunter D

Volume

718

Pagination

pp. 263-266

Publisher

Elsevier

Publication Date

July 28, 2003

DOI

10.1016/s0375-9474(03)00726-7

Conference proceedings

Nuclear Physics A

ISSN

0375-9474

Associated Experts

Alan Chen

Professor, Faculty of Science

Labels

Fields of Research (FoR)

5106 Nuclear and plasma physics 5110 Synchrotrons and Accelerators 51 Physical Sciences 5101 Astronomical sciences 5107 Particle and high energy physics

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