O16(α,γ) | Zendy

H. Costantini | Zendy; R. J. deBoer | Zendy; R.E. Azuma | Zendy; M. Couder | Zendy; J. Görres | Zendy; J. W. Hammer | Zendy; P. J. LeBlanc | Zendy; Hye Young Lee | Zendy; S. O’Brien | Zendy; A. Palumbo | Zendy; E. C. Simpson | Zendy; E. Stech | Zendy; Wanpeng Tan | Zendy; E. Uberseder | Zendy; M. Wiescher | Zendy

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O16(α,γ)

Author(s) -

H. Costantini,

R. J. deBoer,

R.E. Azuma,

M. Couder,

J. Görres,

J. W. Hammer,

P. J. LeBlanc,

Hye Young Lee,

S. O’Brien,

A. Palumbo,

E. C. Simpson,

E. Stech,

Wanpeng Tan,

E. Uberseder,

M. Wiescher

Publication year - 2010

Publication title -

physical review c

Language(s) - English

Resource type - Journals

eISSN - 1089-490X

pISSN - 0556-2813

DOI - 10.1103/physrevc.82.035802

Subject(s) - physics , energy (signal processing) , helium , algorithm , atomic physics , computer science , quantum mechanics

The article presents new measurements of low-energy resonances in the O-16(alpha,gamma)Ne-20 reaction, which represents the endpoint for the reaction sequence responsible for energy production in stellar helium burning in massive red giant stars. The present data and previous unpublished data are analyzed in the framework of R-matrix theory to derive a reaction rate for the temperature regime of stellar helium burning.

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