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Extraction of neutron-capture cross sections on 92^{92}Zr using the charge-exchange Oslo method

Published 11 Sep 2025 in nucl-ex, astro-ph.SR, and nucl-th | (2509.09776v1)

Abstract: The <sup>93<sup>{93}Nb(tt,<sup>3<sup>{3}He) reaction at 115 MeV/u was studied to demonstrate that nuclear level densities and γ\gamma-ray strength functions can be extracted from charge-exchange reactions at intermediate energies using the Oslo technique. The matrix of excitation energy in <sup>93<sup>{93}Zr, reconstructed from the (tt,<sup>3<sup>{3}He) reaction, versus the energy of γ\gamma rays emitted by the excited <sup>93<sup>{93}Zr nuclei, was obtained in an experiment with the S800 Spectrograph operated in coincidence with the GRETINA γ\gamma-ray detector. The extracted level density and γ\gamma-ray strength function obtained by applying the Oslo method to this matrix were used to estimate the <sup>92<sup>{92}Zr(nn,γ\gamma)<sup>93<sup>{93}Zr cross section by combining the new results with other experimental data and theoretical calculations for EE1 and MM1 strength functions at higher energies. Good agreement with direct measurements of the <sup>92<sup>{92}Zr(nn,γ\gamma)<sup>93<sup>{93}Zr cross section was found. The contribution from the upbend in the extracted γ\gamma-ray strength function was important to achieve the consistency as the neutron-capture cross section without this contribution is significantly below the direct measurements otherwise. Since charge-exchange reactions at intermediate energies have long been used for extracting Gamow-Teller strengths, the successful demonstration of the charge-exchange Oslo method enables experiments in which (nn,γ\gamma) cross sections and Gamow-Teller strengths can be measured simultaneously, which is of benefit for astrophysical studies.

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