The 139La(n,gamma) cross section: key for the onset of the s process
arXiv:nucl-ex/0610034 · doi:10.1103/PhysRevC.75.035807
Abstract
The nuclear resonance parameters and the capture cross section of the neutron magic isotope 139La has been measured n_TOF. The description of the experimental apparata is followed by the data analysis procedures. We extracted the resonance parameters, the main nuclear quantities such as the resonance integral, the average gamma widths for s- and p-waves, the nuclear level densities and the neutron strength functions. These results represent a signifcant improvement over previous data. The deduced Maxwellian-averaged capture cross sections are important for the interpretation of the most recent spectroscopic observations in low metallicity stars.
50 pages and 9 Figures
References in corpus (25)
- Neutron capture in low mass Asymptotic Giant Branch stars: cross sections and abundance signatures
- Galactic Evolution of Sr, Y, Zr: A Multiplicity of Nucleosynthetic Processes
- Neutron-Capture Elements in the Early Galaxy: Insights from a Large Sample of Metal-Poor Giants
- The Extremely Metal-Poor, Neutron-Capture-Rich Star CS 22892-052: A Comprehensive Abundance Analysis
- The Hamburg/ESO R-process Enhanced Star survey (HERES) II. Spectroscopic analysis of the survey sample
- The Rise of the s-Process in the Galaxy
- Spectroscopic Studies of Extremly Metal-Poor Stars with Subaru/HDS:II.The r-process Elements, Including Thorium
- Galactic chemical evolution of heavy elements: from Barium to Europium
- A Subaru/HDS study of Lead (Pb) abundances in eight s-process-element-rich, metal-poor stars
- Probing the Neutron-Capture Nucleosynthesis History of Galactic Matter
- Neutron Capture Elements in s-Process-Rich, Very Metal-Poor Stars
- Enrichment of the r-process Element Europium in the Galactic Halo
- Abundance Analysis of HE2148-1247, A Star With Extremely Enhanced Neutron Capture Elements
- Stellar Archaeology: a Keck Pilot Program on Extremely Metal- Poor Stars From the Hamburg/ESO Survey. III. The Lead (Pb) Star HE 0024-2523
- Lead: Asymptotic Giant Branch production and Galactic Chemical Evolution
- Th Ages for Metal-Poor Stars
- New analysis of the two carbon-rich stars CS 22948-27 and CS 29497-34 : binarity and neutron-capture elements
- Near-UV Observations of CS29497-030: New Constraints on Neutron-Capture Nucleosynthesis Processes
- Stellar Sources for Heavy r-Process Nuclei
- Detection of low Eu abundances in extremely metal-poor stars and the origin of r-process elements
- Europium Isotope Ratios in s-Process-Element-Enhanced, Metal-Poor Stars: A New Probe of the 151Sm Branching
- Binary Blue Metal-Poor Stars: Evidence for AGB Mass Transfer
- Inhomogeneous Chemical Evolution of the Galactic Halo: Abundance of r-process Elements
- A Simple Model for r-Process Scatter and Halo Evolution
- Combinatorial Level Densities from a Microscopic Relativistic Structure Model
Cited by in corpus (9)
- The s Process: Nuclear Physics, Stellar Models, Observations
- Neutron Reactions in Astrophysics
- Databases and tools for nuclear astrophysics applications BRUSsels Nuclear LIBrary (BRUSLIB), Nuclear Astrophysics Compilation of REactions II (NACRE II) and Nuclear NETwork GENerator (NETGEN)
- Angular Distribution of -rays from Neutron-Induced Compound States of La
- La(, ) cross sections constrained with statistical decay properties of La nuclei
- Transverse asymmetry of rays from neutron-induced compound states of
- Energy dependent angular distribution of individual -rays in the La(, )La* reaction
- Neutron Capture Reactions near N=82 Shell-Closure
- Measurements of neutron total and capture cross sections of La and evaluation of resonance parameters