First Experimental Constraint on theFe59(n,γ)Fe | Zendy

E. Uberseder | Zendy; T. Adachi | Zendy; T. Aumann | Zendy; S. Beceiro-Novo | Zendy; K. Boretzky | Zendy; C. Caesar | Zendy; I. Dillmann | Zendy; O. Ershova | Zendy; A. Estradé | Zendy; F. Fari | Zendy; J. Hagdahl | Zendy; T. Heftrich | Zendy; M. Heil | Zendy; M. Heine | Zendy; M. Holl | Zendy; A. Ignatov | Zendy; H. Johansson | Zendy; N. Kalantar | Zendy; C. Langer | Zendy; T. Le Bleis | Zendy; Yu. A. Litvinov | Zendy; J. Marganiec | Zendy; A. Movsesyan | Zendy; M. A. Najafi | Zendy; T. Nilsson | Zendy; C. Nociforo | Zendy; V. Panin | Zendy; S. Piétri | Zendy; R. Plag | Zendy; A. Prochazka | Zendy; G. Rastrepina | Zendy; R. Reifarth | Zendy; V. Ricciardi | Zendy; C. Rigollet | Zendy; D. M. Rossi | Zendy; D. Savran | Zendy; H. Simon | Zendy; K. Sonnabend | Zendy; B. Štreicher | Zendy; S. Terashima | Zendy; R. Thies | Zendy; Y. Togano | Zendy; V. Volkov | Zendy; F. Wamers | Zendy; H. Weick | Zendy; M. Weigand | Zendy; M. Wiescher | Zendy; K. Wimmer | Zendy; N. Winckler | Zendy; P. J. Woods | Zendy

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First Experimental Constraint on theFe59(n,γ)Fe

Author(s) -

E. Uberseder,

T. Adachi,

T. Aumann,

S. Beceiro-Novo,

K. Boretzky,

C. Caesar,

I. Dillmann,

O. Ershova,

A. Estradé,

F. Fari,

J. Hagdahl,

T. Heftrich,

M. Heil,

M. Heine,

M. Holl,

A. Ignatov,

H. Johansson,

N. Kalantar,

C. Langer,

T. Le Bleis,

Yu. A. Litvinov,

J. Marganiec,

A. Movsesyan,

M. A. Najafi,

T. Nilsson,

C. Nociforo,

V. Panin,

S. Piétri,

R. Plag,

A. Prochazka,

G. Rastrepina,

R. Reifarth,

V. Ricciardi,

C. Rigollet,

D. M. Rossi,

D. Savran,

H. Simon,

K. Sonnabend,

B. Štreicher,

S. Terashima,

R. Thies,

Y. Togano,

V. Volkov,

F. Wamers,

H. Weick,

M. Weigand,

M. Wiescher,

K. Wimmer,

N. Winckler,

P. J. Woods

Publication year - 2014

Publication title -

physical review letters

Language(s) - English

Resource type - Journals

SCImago Journal Rank - 3.688

H-Index - 673

eISSN - 1079-7114

pISSN - 0031-9007

DOI - 10.1103/physrevlett.112.211101

Subject(s) - nucleosynthesis , physics , dissociation (chemistry) , nuclear reaction , nuclear physics , chemistry

The radionuclide Fe-60 has been of great interest to the nuclear astrophysics community for over a decade. An initial discrepancy between the observed and modeled Galactic Fe-60/Al-26 ratio motivated numerous studies focused on the nucleosynthesis of these two isotopes, though the cross section of the primary astrophysical production reaction, Fe-59(n,gamma)Fe-60, has remained purely theoretical. The present work offers a first experimental constraint on the Fe-59(n,gamma)Fe-60 cross section at astrophysical energies, obtained indirectly via Coulomb dissociation, and demonstrates that the theoretical reaction rates used in present stellar models are not highly erroneous

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