6533b7d3fe1ef96bd1261266

RESEARCH PRODUCT

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

Jouni SuhonenE. Holmlund

subject

Nuclear physicsPhysicsNuclear and High Energy PhysicsParticle physicsValence (chemistry)Solar neutrinoDetectorExcitation spectraDark matterSpectral line

description

Abstract Calculations of the energy spectra and the log ft 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 log ft values between theory and experiments can be regarded as quite good when considering the completely microscopic origin of the model.

https://doi.org/10.1016/s0375-9474(02)00758-3