Electron wave functions in beta-decay formulas revisited (I): Gamow–Teller and spin-dipole contributions to allowed and first-forbidden transitions

Author:

Horiuchi Wataru1ORCID,Sato Toru23ORCID,Uesaka Yuichi4ORCID,Yoshida Kenichi5ORCID

Affiliation:

1. Department of Physics, Hokkaido University, Sapporo 060-0810, Japan

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

3. J-PARC Branch, KEK Theory Center, Institute of Particle and Nuclear Studies (KEK) and Theory Group, Particle and Nuclear Physics Division, J-PARC Center, Tokai, Ibaraki, 319-1106, Japan

4. Faculty of Science and Engineering, Kyushu Sangyo University, Fukuoka 813-8503, Japan

5. Department of Physics, Kyoto University, Kyoto 606-8502, Japan

Abstract

Abstract We propose formulas of the nuclear beta-decay rate that are useful in a practical calculation. The decay rate is determined by the product of the lepton and hadron current densities. A widely used formula relies upon the fact that the low-energy lepton wave functions in a nucleus can be well approximated by a constant and are linear to the radius for the $s$-wave and $p$-wave wave functions, respectively. We find, however, that the deviation from such a simple approximation is evident for heavy nuclei with large $Z$ by numerically solving the Dirac equation. In our proposed formulas, the neutrino wave function is treated exactly as a plane wave, while the electron wave function is obtained by iteratively solving the integral equation, thus we can control the uncertainty of the approximate wave function. The leading-order approximation gives a formula equivalent to the conventional one and overestimates the decay rate. We demonstrate that the next-to-leading-order formula reproduces well the exact result for a schematic transition density as well as a microscopic one obtained by a nuclear energy-density functional method.

Publisher

Oxford University Press (OUP)

Subject

General Physics and Astronomy

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