Title of article
Determination of the (n, γ) reaction rate of unstable 185W in the astrophysical s-process via its inverse reaction Original Research Article
Author/Authors
K. Sonnabend، نويسنده , , A. Mengoni، نويسنده , , P. Mohr، نويسنده , , T. RAUSCHER، نويسنده , , Peter K. Vogt، نويسنده , , A. Zilges، نويسنده ,
Issue Information
هفته نامه با شماره پیاپی سال 2003
Pages
3
From page
533
To page
535
Abstract
The (γ, n) reaction rate of 186W was measured in order to deduce the (n, γ) reaction rate of 185W, an important branching point in the astrophysical s-process. The theoretical predictions have been confirmed and the error range was slightly decreased. The derived Maxwellian averaged cross section (MACS) at 30 keV is (687±110) mb.
Journal title
Nuclear physics A
Serial Year
2003
Journal title
Nuclear physics A
Record number
1199305
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