Primary $$\gamma$$-ray intensities and $$\gamma$$-strength functions from discrete two-step $$\gamma$$-ray cascades in radiative proton-capture experiments
Abstract
Background: Reaction rates of radiative capture reactions can play a crucial role in the nucleosynthesis of heavy nuclei in explosive stellar environments. These reaction rates depend strongly on $$\gamma$$-ray decay widths in the reaction products, which are, for nonresonant capture reactions at high excitation energies, derived from the $$\gamma$$-ray strength function and the nuclear level density. Recently, the ratio method was applied to primary $$\gamma$$ rays observed from ($$\textit{d, p}$$) reactions and nuclear resonance fluorescence measurements to extract the dipole strength in atomic nuclei and to test the generalized Brink-Axel hypothesis. Purpose: The purpose of this work is to apply the ratio method to primary $$\gamma$$-ray intensities of the 63,65Cu($$\textit{p},\gamma$$) reactions to extract $$\gamma$$-ray strength information on the nuclei 64,66Zn. Here, the impact of spin distribution, total $$\gamma$$-ray decay widths, level densities, and width fluctuations on the application of the ratio method will be discussed. Additionally, by comparing the relative $$\gamma$$-ray strength at different excitation energies, conclusions on the validity of the generalized Brink-Axel hypothesis can be made. Method: The radiative proton capture reaction measurements have been performed at the HORUS $$\gamma$$-ray spectrometer of the University of Cologne at one excitation energy for each reaction. Primary $$\gamma$$-ray intensities have been determined by normalizing secondary $$\gamma$$-ray transitions in two-step cascades using their absolute branching ratio. The ratio method was applied to the measured primary $$\gamma$$-ray intensities as well as to previous measurements by Erlandsson et al. at different excitation energies. Results: The relative strength function curve for 64Zn from our measurement shows no significant deviation from the previous measurement at a different excitation energy. The same is true for 66Zn where both measurements were at almost the same excitation energy. Absolute $$\gamma$$-strength function values have been obtained by normalizing the relative curves to quasiparticle random phase approximation calculations because of the absence of experimental data in the respective energy region. Conclusion: The generalized Brink-Axel hypothesis, i.e., the independence of the strength function on the excitation energy, seems to hold in the studied energy region and nuclei. The method to obtain primary $$\gamma$$-ray intensities from two-step cascade spectra was shown to be a valuable and sensitive tool although its uncertainties are connected to the knowledge of the low-energy level scheme of the investigated nucleus. The scaling in the ratio method should be taken with care, because the relative strength is not a simple sum of $$f_{E1}$$ and $$f_{M1}$$ but a somewhat complex linear combination dependent on the excitation energy of the nucleus.
- Authors:
-
- Univ. of Cologne (Germany)
- Univ. of Oslo (Norway)
- GSI Helmholtzzentrum für Schwerionenforschung GmbH, Darmstadt (Germany)
- Ohio Univ., Athens, OH (United States)
- Publication Date:
- Research Org.:
- Ohio Univ., Athens, OH (United States)
- Sponsoring Org.:
- USDOE National Nuclear Security Administration (NNSA); German Research Foundation (DFG); European Research Council (ERC)
- OSTI Identifier:
- 1801134
- Grant/Contract Number:
- NA0002905; ZI 510/8-1; 637686
- Resource Type:
- Accepted Manuscript
- Journal Name:
- Physical Review C
- Additional Journal Information:
- Journal Volume: 101; Journal Issue: 4; Journal ID: ISSN 2469-9985
- Publisher:
- American Physical Society (APS)
- Country of Publication:
- United States
- Language:
- English
- Subject:
- 73 NUCLEAR PHYSICS AND RADIATION PHYSICS; Physics
Citation Formats
Scholz, P., Guttormsen, M., Heim, F., Larsen, A. C., Mayer, J., Savran, D., Spieker, M., Tveten, G. M., Voinov, A. V., Wilhelmy, J., Zeiser, F., and Zilges, A. Primary $\gamma$-ray intensities and $\gamma$-strength functions from discrete two-step $\gamma$-ray cascades in radiative proton-capture experiments. United States: N. p., 2020.
Web. doi:10.1103/physrevc.101.045806.
Scholz, P., Guttormsen, M., Heim, F., Larsen, A. C., Mayer, J., Savran, D., Spieker, M., Tveten, G. M., Voinov, A. V., Wilhelmy, J., Zeiser, F., & Zilges, A. Primary $\gamma$-ray intensities and $\gamma$-strength functions from discrete two-step $\gamma$-ray cascades in radiative proton-capture experiments. United States. https://doi.org/10.1103/physrevc.101.045806
Scholz, P., Guttormsen, M., Heim, F., Larsen, A. C., Mayer, J., Savran, D., Spieker, M., Tveten, G. M., Voinov, A. V., Wilhelmy, J., Zeiser, F., and Zilges, A. Mon .
"Primary $\gamma$-ray intensities and $\gamma$-strength functions from discrete two-step $\gamma$-ray cascades in radiative proton-capture experiments". United States. https://doi.org/10.1103/physrevc.101.045806. https://www.osti.gov/servlets/purl/1801134.
@article{osti_1801134,
title = {Primary $\gamma$-ray intensities and $\gamma$-strength functions from discrete two-step $\gamma$-ray cascades in radiative proton-capture experiments},
author = {Scholz, P. and Guttormsen, M. and Heim, F. and Larsen, A. C. and Mayer, J. and Savran, D. and Spieker, M. and Tveten, G. M. and Voinov, A. V. and Wilhelmy, J. and Zeiser, F. and Zilges, A.},
abstractNote = {Background: Reaction rates of radiative capture reactions can play a crucial role in the nucleosynthesis of heavy nuclei in explosive stellar environments. These reaction rates depend strongly on $\gamma$-ray decay widths in the reaction products, which are, for nonresonant capture reactions at high excitation energies, derived from the $\gamma$-ray strength function and the nuclear level density. Recently, the ratio method was applied to primary $\gamma$ rays observed from ($\textit{d, p}$) reactions and nuclear resonance fluorescence measurements to extract the dipole strength in atomic nuclei and to test the generalized Brink-Axel hypothesis. Purpose: The purpose of this work is to apply the ratio method to primary $\gamma$-ray intensities of the 63,65Cu($\textit{p},\gamma$) reactions to extract $\gamma$-ray strength information on the nuclei 64,66Zn. Here, the impact of spin distribution, total $\gamma$-ray decay widths, level densities, and width fluctuations on the application of the ratio method will be discussed. Additionally, by comparing the relative $\gamma$-ray strength at different excitation energies, conclusions on the validity of the generalized Brink-Axel hypothesis can be made. Method: The radiative proton capture reaction measurements have been performed at the HORUS $\gamma$-ray spectrometer of the University of Cologne at one excitation energy for each reaction. Primary $\gamma$-ray intensities have been determined by normalizing secondary $\gamma$-ray transitions in two-step cascades using their absolute branching ratio. The ratio method was applied to the measured primary $\gamma$-ray intensities as well as to previous measurements by Erlandsson et al. at different excitation energies. Results: The relative strength function curve for 64Zn from our measurement shows no significant deviation from the previous measurement at a different excitation energy. The same is true for 66Zn where both measurements were at almost the same excitation energy. Absolute $\gamma$-strength function values have been obtained by normalizing the relative curves to quasiparticle random phase approximation calculations because of the absence of experimental data in the respective energy region. Conclusion: The generalized Brink-Axel hypothesis, i.e., the independence of the strength function on the excitation energy, seems to hold in the studied energy region and nuclei. The method to obtain primary $\gamma$-ray intensities from two-step cascade spectra was shown to be a valuable and sensitive tool although its uncertainties are connected to the knowledge of the low-energy level scheme of the investigated nucleus. The scaling in the ratio method should be taken with care, because the relative strength is not a simple sum of $f_{E1}$ and $f_{M1}$ but a somewhat complex linear combination dependent on the excitation energy of the nucleus.},
doi = {10.1103/physrevc.101.045806},
journal = {Physical Review C},
number = 4,
volume = 101,
place = {United States},
year = {Mon Apr 27 00:00:00 EDT 2020},
month = {Mon Apr 27 00:00:00 EDT 2020}
}
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