Abstract
Modern numerical methods have made it possible calculate, with remarkably satisfactory results, the spectra nuclei up to A = 10 on the basis of realistic phenomenological models for the nucleon-nucleon interaction, which have been fitted to nucleon-nucleon scattering data and with inclusion of a weak three-nucleon interaction [1]. Employment of the corresponding wavefunctions to calculate the electromagnetic and weak observables and transition strengths of these nuclei calls for correspondingly realistic models for the electromagnetic and axial current density operators, which are consistent with the interaction Hamiltonian.
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.
