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Abstract: The up–down element V ud of the Cabibbo–Kobayashi–Maskawa (CKM) quark mixing matrix is derived from superallowed Fermi decays between isospin T = 1 states using the semi-empirical techniques pioneered by D.H. Wilkinson. Rather than relying directly on the absolute magnitude of theoretical nuclear structure calculations to correct each decay for isospin symmetry breaking effects, these methods extrapolate the experimental ft values to the charge independent limit at where isospin-dependent effects are negligible. The value V ud = 0.97430(29) derived in this work agrees with the value V ud = 0.97425(22) obtained from the most recent shell-model calculations of isospin symmetry breaking that have expanded the shell-model spaces by including select core orbitals. These values are not in agreement with previous shell-model calculations in more restrictive model spaces or the values obtained from recent self-consistent relativistic Hartree and Hartree–Fock calculations based on the random-phase approximation that all underestimate the magnitude of isospin symmetry breaking. [Copyright &y& Elsevier]

Gamma-Ray Infrastructure For Fundamental Investigations of Nuclei, GRIFFIN, is a new experimental facility for radioactive decay studies at the TRIUMF-ISAC laboratory. This article describes the details of the custom designed GRIFFIN digital data acquisition system. The features of the system that will enable high-precision half-life and branching ratio measurements with levels of uncertainty better than 0.05% are described. The system has demonstrated the ability to effectively collect signals from High-purity germanium crystals at counting rates up to 50 kHz while maintaining good energy resolution, detection efficiency and spectral quality. [ABSTRACT FROM AUTHOR]

The Gamma-Ray Infrastructure For Fundamental Investigations of Nuclei, GRIFFIN, is a new experimental facility for radioactive decay studies at the TRIUMF-ISAC laboratory. The performance of the 16 high-purity germanium (HPGe) clover detectors that will make up the GRIFFIN spectrometer is reported. The energy resolution, efficiency, timing resolution, crosstalk and preamplifier properties of each crystal were measured using a combination of analog and digital data acquisition techniques. The absolute efficiency and add-back factors are determined for the energy range of 80–3450 keV. The detectors show excellent performance with an average over all 64 crystals of a FWHM energy resolution of 1.89(6) keV and relative efficiency with respect to a 3 in . × 3 in . NaI detector of 41(1)% at 1.3 MeV. [ABSTRACT FROM AUTHOR]