First Experimental Constraint on the Fe-59(n, gamma)Fe-60 Reaction Cross Section at Astrophysical Energies via the Coulomb Dissociation of Fe-60
Journal article, 2014

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.

Author

E. Uberseder

T. Adachi

T. Aumann

S. Beceiro-Novo

K. Boretzky

C. Caesar

I. Dillmann

O. Ershova

A. Estrade

F. Farinon

Julius Hagdahl

Chalmers, Fundamental Physics

T. Heftrich

M. Heil

M. Heine

M. Holl

A. Ignatov

Håkan T Johansson

Chalmers, Fundamental Physics

N. Kalantar

C. Langer

T. Le Bleis

Y. A. Litvinov

J. Marganiec

A. Movsesyan

M. A. Najafi

Thomas Nilsson

Chalmers, Fundamental Physics

C. Nociforo

V. Panin

S. Pietri

R. Plag

A. Prochazka

G. Rastrepina

R. Reifarth

V. Ricciardi

C. Rigollet

D. M. Rossi

D. Savran

H. Simon

K. Sonnabend

B. Streicher

S. Terashima

Ronja Thies

Chalmers, Fundamental Physics

Y. Togano

V. Volkov

F. Wamers

H. Weick

M. Weigand

M. Wiescher

C. Wimmer

N. Winckler

P. J. Woods

Physical Review Letters

0031-9007 (ISSN) 1079-7114 (eISSN)

Vol. 112 21

Subject Categories

Subatomic Physics

Physical Sciences

Astronomy, Astrophysics and Cosmology

Roots

Basic sciences

DOI

10.1103/PhysRevLett.112.211101

More information

Created

10/7/2017