https://doi.org/10.1140/epja/s10050-025-01647-w
Regular Article - Experimental Physics
Photo-response of the
nucleus 28Si below 13.0 MeV
1
School of Computing, Engineering, and Physical Sciences, University of the West of Scotland, PA1 2BE, Paisley, UK
2
SUPA, Scottish Universities Physics Alliance, Glasgow, UK
3
Helmholtz-Zentrum Dresden-Rossendorf, 01328, Dresden, Germany
4
Department of Physics, Karamanoglu Mehmetbey University, Karaman, Turkey
5
Faculty of Physics, St. Kliment Ohridski University of Sofia, 1164, Sofia, Bulgaria
6
Department of Physics, Oliver Lodge Laboratory, University of Liverpool, L69 7ZE, Liverpool, UK
7
Technische Universität Dresden, Institut für Kern- und Teilchenphysik, 01062, Dresden, Germany
8
GSI Helmholtzzentrum für Schwerionenforschung GmbH, 64291, Darmstadt, Germany
9
Ludwig–Maximilians–Universität München, 85748, Garching, Germany
10
INFN, Sezione di Milano, 20133, Milan, Italy
Received:
11
April
2025
Accepted:
10
July
2025
Published online:
12
August
2025
The electric E1 and magnetic M1 dipole responses of the
nucleus 28Si were investigated in a nuclear resonance fluorescence experiment at the ELBE accelerator of the Helmholtz Zentrum Dresden-Rossendorf. The investigated energy range extends to 13.0 MeV, which corresponds to the kinetic energy of the electrons that were used to produce the unpolarised bremsstrahlung in the entrance channel of the 28Si(
) reaction. The bremsstrahlung photons excited three
, seven
, and several
states. De-excitation
rays were detected using the four high-purity germanium detectors of the
ELBE setup. The excellent background conditions allowed to identify nine previously unobserved
-ray transitions. In the investigated energy region of up to 13.0 MeV a total
strength is firmly observed with a possible addition of
from levels for which the data allows to establish only an upper limit. Furthermore, below 13 MeV this
nucleus exhibits a marginal isoscalar E1 strength of
, which exhausts only 0.026(2) % of the energy-weighted sum rule.
© The Author(s) 2025
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