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.
Full text not available from this repository.
Official URL: http://edoc.unibas.ch/dok/A5839283
Downloads: Statistics Overview
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 > Former Organization Units Physics > Theoretische Physik Astrophysik (Thielemann) |
|---|---|
| UniBasel Contributors: | Rauscher, Thomas |
| Item Type: | Article, refereed |
| Article Subtype: | Research Article |
| Publisher: | North Holland |
| ISSN: | 0375-9474 |
| Note: | Publication type according to Uni Basel Research Database: Journal article |
| Related URLs: | |
| Identification Number: | |
| Last Modified: | 14 Sep 2012 07:18 |
| Deposited On: | 14 Sep 2012 06:44 |
Repository Staff Only: item control page