Effective two-body ΛNNN weak potentials deduced from three-body ΛNNNNN interactions and hypernuclear non-mesonic weak decay rates

Author:

Itonaga Kazunori12,Motoba Toshio345,Rijken Thomas A6

Affiliation:

1. Faculty of Medicine, University of Miyazaki , Miyazaki 889-1692, Japan

2. Physics Department, Gifu University, 1-1 Yanagido , Gifu 501-1193, Japan

3. Research Center for Nuclear Physics, Osaka University , Ibaraki, Osaka 567-0047, Japan

4. Laboratory of Physics, Osaka Electro-Communication University , Neyagawa 572-8530, Japan

5. Yukawa Institute for Theoretical Physics, Kyoto University , Kyoto 606-8502, Japan

6. Institute of Mathematics, Astrophysics, and Particle Physics, Radboud University , NL-6525 ED Nijmegen, The Netherlands

Abstract

Abstract We intend to study the role of the three-body weak ΛNN → NNN interaction in two-nucleon induced hypernuclear non-mesonic weak decay. The three-body weak interactions are constructed on the basis of the meson-pair exchange (MPE) model and then we derive the effective two-body ΛN → NN weak potentials from the three-body interactions based on the Loiseau–Nogami–Ross approximation. The strong coupling constants of MPE are taken from the Nijmegen ESC and GESC models and the weak ones of MPE are evaluated in the weak Λ–n mixing model by Dalitz and Von Hippel [Phys. Lett. 10, 153 (1964)]. The effective two-body ΛN → NN weak potentials are applied to evaluate hypernuclear non-mesonic decay rates, which should give a certain additional contribution to the two-nucleon induced decay rate Γ2N. Calculations of $\Gamma ^{({\text{eff.2B}})}_{nm}$ are done for $^5_\Lambda {\rm He}$, $^{11}_\Lambda {\rm B}$, and $^{12}_\Lambda {\rm C}$ and the results are compared with experimental data $\Gamma ^\mathrm{exp}_{2N}$. We have demonstrated the possibility of accounting for the two-nucleon induced non-mesonic decays of light and p-shell hypernuclei by introducing the effective two-body potentials deduced from the three-body weak interactions, though the calculated $\Gamma ^{(\text{eff.2B})}_{nm}$ still includes uncertainties. Discussions and limitations of our “effective two-body ΛN → NN model” are given.

Funder

Gifu University

Publisher

Oxford University Press (OUP)

Subject

General Physics and Astronomy

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