Mohr, Peter
Angulo, C.
[UCL]
Descouvemont, P.
Utsunomiya, H.
(eng)
The astrophysical reaction rates of the 16O(a,g)20Ne capture reaction and its
inverse 20Ne(g,a)16O photodisintegration reaction are given by the sum of
several narrow resonances and a small direct capture contribution at low
temperatures. Although the thermal population of low lying excited states in
16O and 20Ne is extremely small, the first excited state in 20Ne plays a
non-negligible role for the photodisintegration rate. Consequences for
experiments with so-called quasi-thermal photon energy distributions are
discussed.
Comment: 4 pages, 2 figures, Proceedings Nuclear Physics in Astrophysics-II,
Debrecen, Hungary, 2005
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- Mohr Peter, Photon-induced Reactions in Stars and in the Laboratory: A Critical Comparison, 10.1063/1.1737151
- Vogt K., Mohr P., Babilon M., Enders J., Hartmann T., Hutter C., Rauscher T., Volz S., Zilges A., Measurement of the(γ,n)reaction rates of the nuclides190Pt,192Pt,and198Ptin the astrophysicalγprocess, 10.1103/physrevc.63.055802
- Vogt K., Mohr P., Babilon M., Bayer W., Galaviz D., Hartmann T., Hutter C., Rauscher T., Sonnabend K., Volz S., Zilges A., Measurement of the (γ, n) cross section of the nucleus 197Au close above the reaction threshold, 10.1016/s0375-9474(02)00922-3
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Bibliographic reference |
Mohr, Peter ; Angulo, C. ; Descouvemont, P. ; Utsunomiya, H.. Relation between the O-16 (alpha,gamma) Ne-20 reaction and its reverse Ne-20 (gamma,alpha) O-16 reaction in stars and in the laboratory. In: European Physical Journal A. Hadrons and Nuclei, Vol. 27, p. 75-78 (2006) |
Permanent URL |
http://hdl.handle.net/2078/30996 |