Publikationsdatum:
2018-06-15
Beschreibung:
Author(s): M. B. Bennett, C. Wrede, S. N. Liddick, D. Pérez-Loureiro, D. W. Bardayan, B. A. Brown, A. A. Chen, K. A. Chipps, C. Fry, B. E. Glassman, C. Langer, N. R. Larson, E. I. McNeice, Z. Meisel, W. Ong, P. D. O'Malley, S. D. Pain, C. J. Prokop, H. Schatz, S. B. Schwartz, S. Suchyta, P. Thompson, M. Walters, and X. Xu Background: Cl 31 is a neutron-deficient isotope with a half-life of T 1 / 2 = 190 ( 1 ) ms. The nuclear structure of its daughter, S 31 , is important for the determination of the thermonuclear P 30 ( p , γ ) S 31 reaction rate, which affects the final isotopic abundances of the ejecta from classical oxygen-neon nova... [Phys. Rev. C 97, 065803] Published Thu Jun 14, 2018
Schlagwort(e):
Nuclear Astrophysics
Print ISSN:
0556-2813
Digitale ISSN:
1089-490X
Thema:
Physik
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