18–22 May 2026
Helga Engs Hus
Europe/Oslo timezone

PHOTON STRENGTH FUNCTION OF $^{61}$Cu USING RADIATIVE PROTON CAPTURE

Not scheduled
20m
Auditorium 1 (Helga Engs Hus)

Auditorium 1

Helga Engs Hus

Sem Sælands vei 7, 0371 OSLO Norway
Oral

Speaker

Tshegofatso Modise (University of Botswana)

Description

Radiative proton capture is among the reaction mechanisms used for investigating nuclear structure in the quasi-continuum region. The nuclear level density (NLD) is high in the quasi-continuum region and the study of decays from individual states is not feasible. Instead, information on the decay is obtained through the statistical treatment of decay probabilities such as the photon strength function (PSF) [1]. In the current study, we utilize the $^{60}\mathrm{Ni}(p,\gamma)^{61}\mathrm{Cu}$ reaction to investigate the PSF for $^{61}\mathrm{Cu}$ below the neutron separation threshold. The experiment was conducted using the low-energy nuclear physics beam line at the 3 MV Tandetron facility of the iThemba Laboratory for Accelerator Based Sciences (iThemba LABS) with incident proton beam energies in the range of 2.3-4.3 MeV. This populated excited states in the $^{61}\mathrm{Cu}$ compound nucleus between 7.03 and 9.01 MeV. The emitted gamma rays were detected using Compton suppressed hyper pure germanium (HPGe) and large volume lanthanum bromide (LaBr3) detectors.

The study focuses on the extraction of the shape of PSF through the use of the Shape Method [2]. The results will provide more insight into the $^{61}\mathrm{Cu}$ PSF via direct decays to the ground state and low-lying excited levels.

Preliminary results on the PSF from partial decays to the ground state will be presented.

References
1. S. Goriely et al., Eur. Phys. J. A 55, 172 (2019).
2. M. Wiedeking et al. Phys. Rev.C 104, 014311 (2021).

This research work is supported in part by the National Research Foundation of South Africa (Grant No:118846, 92600, 90741, 92789 and REP-SARC180529336567). It is also based upon work supported by the U.S. Department of Energy, Office of Science, Office of Nuclear Physics under Contract No. DE-AC02-05CH11231.

Authors

Tshegofatso Modise (University of Botswana) Dr Kgashane Malatji (University of California Berkeley) N Palalani (Department of Physics, University of Botswana) Mathis Wiedeking (Lawrence Berkeley National Laboratory) Lindsay Donaldson (iThemba LABS) F Ogundare (Department of Physics, University of Botswana) Philip Adsley (Texas A&M University) Armand Bahini (Université de Caen Normandie, France) Jacob Bekker (University of the Witwatersrand, iThemba LABS, South Africa) Sifundo Binda (University of the Witwatersrand and iThemba LABS) Tshegofatso Bokhutlo (BIUST) Shanyn-Dee Hart (iThemba LABS, National Research Foundation (ZA)) LESEDI JAFTA (iThemba LABS) Dr Pete Jones (iThemba LABS, National Research Foundation (ZA)) Vincent. B Kheswa (University of Johannesburg) Thuthukile Khumalo Sebenzile Magagula (University of the Witwatersrand and iThemba LABS) Refilwe Molaeng (School of Physics, University of the Witwatersrand) R.E. Molaeng (iThemba LABS) Retief Neveling (iThemba LABS, South Africa) Luna Pellegri

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