Gamow–Teller beta decays of the odd-mass neighbors of the solar-neutrino detector 127I Original Research Article

Calculations of the energy spectra and the View the MathML source values of Gamow–Teller beta transitions of neutron-odd and proton-odd nuclei close to the solar-neutrino detector 127I are performed using the microscopic quasiparticle–phonon model. The information obtained from the beta transition strengths is valuable in solar-neutrino detection and dark matter search both in present and future large-scale experiments. Realistic interactions within a realistic single-particle valence space were used in the calculations. The overall correspondence in terms of the excitation spectra and the View the MathML source values between theory and experiments can be regarded as quite good when considering the completely microscopic origin of the model.