Sauerwein, A., Endres, J., Netterdon, L., Zilges, A., Foteinou, V., Provatas, G., Konstantinopoulos, T., Axiotis, M., Ashley, S. F., Harissopulos, S. and Rauscher, T. (2012). Investigation of the reaction Ge-74(p,gamma)As-75 using the in-beam method to improve reaction network predictions for p nuclei. Phys. Rev. C, 86 (3). COLLEGE PK: AMER PHYSICAL SOC. ISSN 1089-490X

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Abstract

Background: Astrophysical models studying the origin of the neutron-deficient p nuclides require knowledge of proton capture cross sections at low energy. The production site of the p nuclei is still under discussion but a firm basis of nuclear reaction rates is required to address the astrophysical uncertainties. Data at astrophysically relevant interaction energies are scarce. Problems with the prediction of charged particle capture cross sections at low energy were found in the comparisons between previous data and calculations in the Hauser-Feshbach statistical model of compound reactions. Purpose: A measurement of Ge-74(p,gamma)As-75 at low proton energies, inside the astrophysically relevant energy region, is important in several respects. The reaction is directly important because it is a bottleneck in the reaction flow which produces the lightest p nucleus Se-74. It is also an important addition to the data set required to test reaction-rate predictions and to allow an improvement in the global p + nucleus optical potential required in such calculations. Method: An in-beam experiment was performed, making it possible to measure in the range 2.1 <= E-p <= 3.7 MeV, which is for the most part inside the astrophysically relevant energy window. Angular distributions of the gamma-ray transitions were measured with high-purity germanium detectors at eight angles relative to the beam axis. In addition to the total cross sections, partial cross sections for the direct population of 12 levels were determined. Results: The resulting cross sections were compared to Hauser-Feshbach calculations using the code SMARAGD. Only a constant renormalization factor of the calculated proton widths allowed a good reproduction of both total and partial cross sections. The accuracy of the calculation made it possible to check the spin assignment of some states in As-75. In the case of the 1075-keV state, a double state with spins and parities of 3/2- and 5/2- is needed to explain the experimental partial cross sections. A change in parity from 5/2(+) to 5/2(-) is required for the state at 401 keV. Furthermore, in the case of Ge-74, studying the combination of total and partial cross sections made it possible to test the gamma width, which is essential in the calculation of the astrophysical As-74(n,gamma)As-75 rate. Conclusions: Between data and statistical model prediction a factor of about two was found. Nevertheless, the improved astrophysical reaction rate of Ge-74(p,gamma) (and its reverse reaction) is only 28% larger than the previous standard rate. The prediction of the As-74(n,gamma)As-75 rate (and its reverse) was confirmed, the newly calculated rate differs only by a few percent from the previous prediction. The in-beam method with high-efficiency detectors proved to be a powerful tool for studies in nuclear astrophysics and nuclear structure.

Item Type: Journal Article
Creators:
CreatorsEmailORCIDORCID Put Code
Sauerwein, A.UNSPECIFIEDUNSPECIFIEDUNSPECIFIED
Endres, J.UNSPECIFIEDUNSPECIFIEDUNSPECIFIED
Netterdon, L.UNSPECIFIEDUNSPECIFIEDUNSPECIFIED
Zilges, A.UNSPECIFIEDUNSPECIFIEDUNSPECIFIED
Foteinou, V.UNSPECIFIEDUNSPECIFIEDUNSPECIFIED
Provatas, G.UNSPECIFIEDUNSPECIFIEDUNSPECIFIED
Konstantinopoulos, T.UNSPECIFIEDUNSPECIFIEDUNSPECIFIED
Axiotis, M.UNSPECIFIEDUNSPECIFIEDUNSPECIFIED
Ashley, S. F.UNSPECIFIEDUNSPECIFIEDUNSPECIFIED
Harissopulos, S.UNSPECIFIEDUNSPECIFIEDUNSPECIFIED
Rauscher, T.UNSPECIFIEDUNSPECIFIEDUNSPECIFIED
URN: urn:nbn:de:hbz:38-483032
DOI: 10.1103/PhysRevC.86.035802
Journal or Publication Title: Phys. Rev. C
Volume: 86
Number: 3
Date: 2012
Publisher: AMER PHYSICAL SOC
Place of Publication: COLLEGE PK
ISSN: 1089-490X
Language: English
Faculty: Unspecified
Divisions: Unspecified
Subjects: no entry
Uncontrolled Keywords:
KeywordsLanguage
ASTROPHYSICAL REACTION-RATES; OPTICAL-MODEL; PROCESS NUCLEOSYNTHESIS; CROSS-SECTIONS; MASSIVE STARS; FINITE NUCLEI; RP-PROCESS; S-PROCESS; TEMPERATURE; SENSITIVITYMultiple languages
Physics, NuclearMultiple languages
URI: http://kups.ub.uni-koeln.de/id/eprint/48303

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