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Structure of β-decay Strength Function Sβ(E) in Halo Nuclei

  • Physics of Elementary Particles and Atomic Nuclei. Experiment
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Abstract

It is shown that when the parent nucleus has nn Borromean halo structure, then after Gamow–Teller (GT) β–-decay of parent state or after M1 γ-decay of Isobar Analogue Resonance (IAR) the states with np tango halo structure or mixed np tango + nn Borromean halo structure can be populated. Resonances in the GT β-decay strength function Sβ(E) of halo nuclei, may have np tango halo structure or mixed np tango + nn Borromean halo structure. Correct interpretation of halo structure is important in experiments on β-decay study, interpretation of M1 γ-decay of IAR, and charge-exchange nuclear reactions analysis.

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  1. Joint Institute for Nuclear Research, Dubna, 141980, Russia

    I. N. Izosimov

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  1. I. N. Izosimov
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Correspondence to I. N. Izosimov.

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Izosimov, I.N. Structure of β-decay Strength Function Sβ(E) in Halo Nuclei. Phys. Part. Nuclei Lett. 15, 621–626 (2018). https://doi.org/10.1134/S1547477118060092

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  • DOI: https://doi.org/10.1134/S1547477118060092

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