Abstract
The neutron binding energy in93Sr has been determined to (5230±6) keV from energy correspondences between levels defined by γ-ray transitions and β-delayed neutron emission.
Similar content being viewed by others
References
C.M. Jensen et al., Phys. Rev.C15, 1972 (1977)
S.G. Prussin et al., Phys. Rev.C16, 1001 (1977)
T. Borello-Lewin and O. Dietzsch, Z. Naturforsch.34a, 1536 (1979)
F. Münnich Proc. Int. Workshop on Nuclear Spectroscopy of Fission Products, Institut Laue-Langevin, Grenoble (1979), Inst. of Physics Conf. Ser. No. 51, in press
F.M. Nuh et al., Nucl. Phys.A293, 410 (1977)
C.J. Bischof and W.L. Talbert, Phys. Rev.C15, 1047 (1977)
K.-L. Kratz et al., Proc. Int. Workshop on Gross Properties of Nuclei and Nuclear Excitations V, TH Darmstadt (1977), AED-Conf-77-017-035
Author information
Authors and Affiliations
Additional information
The authors would like to acknowledge fruitful discussions with G. Herrmann and S.G. Prussin.
This work was supported by the German Bundesministerium für Forschung und Technologie.
Rights and permissions
About this article
Cite this article
Kratz, K.L., Ohm, H. The neutron binding energy in the neutron-rich nucleus93Sr. Z Physik A 295, 199–200 (1980). https://doi.org/10.1007/BF01413078
Received:
Issue Date:
DOI: https://doi.org/10.1007/BF01413078