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- W2266848649 abstract "The majority of the light elements up to iron (Fe) are formed by successive rounds of thermonuclear fusion burning in the stellar interiors. The nuclei heavier than iron (Z>26) are being synthesized mainly by neutron-capture reactions the astrophysical r-and s-processes. There are 35 neutron deficient stable isotopes between Se and Hg which are shielded from the rapid neutron capture by stable isobars. These so-called p-nuclei are produced in explosive stellar environments via photodisintegration reactions like (γ,n), (γ,p) and (γ,α) on ror sseed nuclei. The reaction rates of the p-nuclei are mostly based on theoretical parameterizations using statistical model calculations. At the bremsstrahlung facility of the superconducting electron accelerator ELBE, photon-induced reactions of the p-nuclei are being studied. In the scope of this thesis work, photodisintegration measurements of the p-nuclei Mo and Sm have been performed via the photoactivation technique. The residual nuclei resulting from photoactivation were studied via γ-ray spectroscopy. For the decay measurements of short-lived nuclei, a pneumatic delivery system has been used. In the case of Sm(γ,p) and Sm(γ,α) reactions, the activated samarium samples with very low counting statistics were measured at the underground laboratory ”Felsenkeller” in Dresden. The experimental activation yields for the Sm (γ,n), (γ,p) and (γ, α) and the Mo(γ, α) reactions were determined. It is to be emphasized that the (γ,p) and (γ, α) reactions were measured for the first time in a laboratory at astrophysically relevant energies. In all the mentioned experiments, special care was taken to determine the endpoint energy of the bremsstrahlung spectra by using the photodisintegration of deuteron. The Au(γ,n)Au reaction has been established as an activation standard. The photoactivation yields for the Au(γ,n) and Sm(γ, n) reactions have been compared to the yield calculated using cross sections from previous photoneutron experiments. A comparison of the two data sets leads to a conclusion on the inaccuracies in previous data. The statistical uncertainties involved in the activation experiments are very small except for the case of decay spectra with weak counting statistics. The systematic uncertainties are mostly from the experimental determination of photon flux. A detailed discussion of the overall uncertainty is provided. Hauser-Feshbach statistical model calculations using TALYS and NON-SMOKER codes have been performed for all the concerned reactions. The experimental activation yields, in general, agree within a factor of 2 to the simulated yields using statistical model predictions. The sensitivity of the model codes to the nuclear physics inputs like optical-model potentials, nuclear level densities and γ-ray strength functions has been tested." @default.
- W2266848649 created "2016-06-24" @default.
- W2266848649 creator A5085575095 @default.
- W2266848649 date "2009-06-03" @default.
- W2266848649 modified "2023-09-23" @default.
- W2266848649 title "Photodisintegration studies ofastrophysically relevant p-nuclei" @default.
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