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Determination of the (n,gamma) reaction rate of unstable W-185 in the astrophysical s-process via its inverse reaction

Sonnabend, K. and Mengoni, A. and Mohr, P. and Rauscher, T. and Vogt, K. and Zilges, A.. (2003) Determination of the (n,gamma) reaction rate of unstable W-185 in the astrophysical s-process via its inverse reaction. Nuclear physics. A, Nuclear and hadronic physics, Vol. 718 , S. 533C-535C.

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Official URL: http://edoc.unibas.ch/dok/A5839283

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Abstract

The (gamma,n) reaction rate of W-186 was measured in order to deduce the (n,gamma) reaction rate of 185 W, 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.
Faculties and Departments:05 Faculty of Science > Departement Physik > Physik > Theoretische Physik Astrophysik (Thielemann)
UniBasel Contributors:Rauscher, Thomas
Item Type:Article, refereed
Article Subtype:Research Article
Bibsysno:Link to catalogue
Publisher:North Holland
ISSN:0375-9474
Note:Publication type according to Uni Basel Research Database: Journal article
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Last Modified:14 Sep 2012 07:18
Deposited On:14 Sep 2012 06:44

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