(n,γ) cross-sections of light p nuclei

@article{Dillmann2006nCO,
  title={(n,$\gamma$) cross-sections of light p nuclei},
  author={Iris Dillmann and Martin Heil and Franz Käppeler and Ralf Plag and Thomas Rauscher and F. Thielemann},
  journal={The European Physical Journal A - Hadrons and Nuclei},
  year={2006},
  volume={27},
  pages={129-134}
}
Abstract.The nucleosynthesis of elements beyond iron is dominated by the s and r processes. However, a small amount of stable isotopes on the proton-rich side cannot be made by neutron capture and is thought to be produced by photodisintegration reactions on existing seed nuclei in the so-called “p process”. So far most of the p-process reactions are not yet accessible by experimental techniques and have to be inferred from statistical Hauser-Feshbach model calculations. The parametrization of… 

(n,$\gamma$) Cross Sections of Light p Nuclei -- Towards an Updated Database for the p Process

The nucleosynthesis of elements beyond iron is dominated by the s and r processes. However, a small amount of stable isotopes on the proton-rich side cannot be made by neutron capture and are thought

References

SHOWING 1-10 OF 52 REFERENCES

NEUTRON CROSS SECTIONS FOR NUCLEOSYNTHESIS STUDIES

Previous compilations of (n, gamma) cross sections of relevance for neutron capture nucleosynthesis in the big bang and in the slow neutron capture process (s process) have been updated to encompass

Measurement of the(γ,n)reaction rates of the nuclides190Pt,192Pt,and198Ptin the astrophysicalγprocess

The nucleosynthesis of heavy neutron-deficient nuclei in a stellar photon bath at the temperatures relevant for the astrophysical gamma process was investigated. In order to derive (gamma,n) cross

P-process in supernovae

The nucleosynthetic origin of the rare proton-rich isotopes, usually called ''p-process'' isotopes, is examined. A particularly interesting context for this synthesis is found to be explosive events

Tables of nuclear cross sections and reaction rates : An addendum to the paper "Astrophysical reaction rates from statistical model calculations"

In a previous publication (ATOMIC DATA AND NUCLEAR DATA TABLES 75, 1 (2000)), we gave seven-parameter analytical fits to theoretical reaction rates derived from nuclear cross sections calculated in

Astrophysical reaction rates from statistical model calculations

Theoretical reaction rates in the temperature range 0.01 x 10(9) less than or equal to T(K) less than or equal to 10.0 x 10(9) are calculated in the statistical model (Hauser-Feshbach formalism) for

Nucleosynthesis in Massive Stars with Improved Nuclear and Stellar Physics

We present the first calculations to follow the evolution of all stable nuclei and their radioactive progenitors in stellar models computed from the onset of central hydrogen burning through

Nucleosynthesis and Neutron-Capture Cross Sections

The role of neutron capture reactions in the nucleosynthesis of heavy elements in stars is reviewed. Maxwellian-averaged capture cross sections at 30 keV are presented for most isotopes across the

Neutron capture cross section of Au-197: A standard for stellar nucleosynthesis

We have measured the neutron capture cross section of gold using the $^{7}\mathrm{Li}$(p,n${)}^{7}$Be reaction for neutron production. This reaction not only provides the integrated neutron flux via
...