Abstract
The g-factor of the 3 − (298 keV) state in 16N has been measured by observing the hyperfine modulation of the γ-ray anisotropy in one-electron ions recoiling in vacuum following the 2H( 15N, p) 16N reaction. From the observed spatial frequency the g-factor was deduced to be | g| = 0.532±0.020. Simultaneous lifetime determinations for this state and the 1 − (397 keV) state in 16N gave values of τm = 131.7±1.9 ps and τ m = 5.63±0.05 ps, respectively. These and other electromagnetic observables associated with the lowest four levels in 16N are compared to shell-model calculations.
Sign-in/Register to access full text options 
Talk to us
Join us for a 30 min session where you can share your feedback and ask us any queries you have
Schedule a callDisclaimer: All third-party content on this website/platform is and will remain the property of their respective owners and is provided on "as is" basis without any warranties, express or implied. Use of third-party content does not indicate any affiliation, sponsorship with or endorsement by them. Any references to third-party content is to identify the corresponding services and shall be considered fair use under The CopyrightLaw.
