Phys. Rev. Lett. 78, 4347–4350 (1997)Application of the Kerman-Klein Method to the Solution of a Spherical Shell Model for a Deformed Rare-Earth NucleusReceived 6 February 1997; published in the issue dated 9 June 1997 Put forward more than three decades ago as an alternative to conventional shell-model calculations, the Kerman-Klein method has proved feasible previously only when applied to unrealistically small configuration spaces or when phenomenological simplifications have been superposed. Starting from a spherical shell-model Hamiltonian, we describe a fully microscopic calculation, free of the above limitations, of the properties of the ground-state band of a typical deformed rare-earth nucleus, 158Gd. © 1997 The American Physical Society URL:
http://link.aps.org/doi/10.1103/PhysRevLett.78.4347
DOI:
10.1103/PhysRevLett.78.4347
PACS:
21.60.Ev, 21.10.Re, 21.60.Cs, 27.70.+q
|
|
About | Terms and Conditions | Subscriptions | Search | Help
Use of the American Physical Society websites and journals implies that the user has read and agrees to our Terms and Conditions and any applicable Subscription Agreement. Physical Review®, Physical Review Letters®, Reviews of Modern Physics®, and Physical Review Special Topics® are trademarks of the American Physical Society.