Original paper
Thermal (n , γ ) cross section and resonance integral ofTm 171
Abstract
Background: About 50% of the heavy elements are produced in stars during the slow neutron capture process. The analysis of branching points allows us to set constraints on the temperature and the neutron density in the interior of stars.Purpose: The temperature dependence of the branch point ^{171}\mathrm{Tm}is weak. Hence, the ^{171}\mathrm{Tm}neutron capture cross section can be used to constrain the neutron density during the main...
Paper Details
Title
Thermal (n , γ ) cross section and resonance integral ofTm 171
Published Date
Jun 27, 2019
Journal
Volume
99
Issue
6
Citation AnalysisPro
You’ll need to upgrade your plan to Pro
Looking to understand the true influence of a researcher’s work across journals & affiliations?
- Scinapse’s Top 10 Citation Journals & Affiliations graph reveals the quality and authenticity of citations received by a paper.
- Discover whether citations have been inflated due to self-citations, or if citations include institutional bias.
Notes
History