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Microscopic calculations of beta decay far from stability

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Zeitschrift für Physik A Atomic Nuclei

Abstract

Beta decay properties of nuclei far from stability are of decisive importance for the understanding of the element synthesis in the universe and the determination of the age of the universe by means of cosmochronometers. A new large scale microscopic calculation ofβ −-decay half-lives up to the neutron drip line is presented. This new approach uses the proton-neutron quasiparticle random phase approximation with a Gamow-Teller residual interaction.

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Author notes

  1. K. Muto

    Present address: Department of Physics, Tokyo Institute of Technology, Tokyo, Japan

Authors and Affiliations

  1. Max-Planck-Institut für Kernphysik, Heidelberg, Federal Republic of Germany

    A. Staudt, E. Bender, K. Muto & H. V. Klapdor

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  1. A. Staudt
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  2. E. Bender
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Additional information

The authors express their gratitude towards Dr. J. Metzinger for advice and discussions. Furthermore we would like to thank Dr. A.C. Mueller for unpublished data and very fruitful discussions.

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Staudt, A., Bender, E., Muto, K. et al. Microscopic calculations of beta decay far from stability. Z. Physik A - Atomic Nuclei 334, 47–57 (1989). https://doi.org/10.1007/BF01294386

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