Author/Authors :
Peter K. Vogt، نويسنده , , P. Mohr، نويسنده , , M. Babilon، نويسنده , , W. Bayer، نويسنده , , D. Galaviz، نويسنده , , T. Hartmann، نويسنده , , C. Hutter، نويسنده , , T. RAUSCHER، نويسنده , , K. Sonnabend، نويسنده , , S. Volz، نويسنده , , A. Zilges، نويسنده ,
Abstract :
The cross section and the astrophysical reaction rate of the reaction 197Au(γ, n)196Au have been measured close above the reaction threshold at Ethr=8.071 MeV using the method of photoactivation. The results are compared to those of several previous measurements as well as to theoretical calculations. The relevance of the reaction 197Au(γ, n)196Au as a standard for photoactivation experiments is discussed.
Keywords :
Photoactivation technique , measured ? , Comparison with previous result . , model predictions , Nuclear reactions bremsstrahbung , 197Au(? , N) , E=8325–9900 keV , deduced astrophysical reaction rates
