The nature of the superband in backbending for the nucleus /sup 156 /Dy
(1977) Nuclear Physics, Section A — Vol. A279, n° 2, p. 223-236 (1977)
Files
No attached file found for this publication.
Details
- Authors
- Abstract
- In two recent publications by Broglia et al. (see Phys. Lett., vol.57B, p.113 (1975)), it has been shown that backbending can be understood by mixing the ground (g) and a /b K/=1 (super)band (s1). It has also been claimed that a /b K/=0 superband (s0) is not able to reproduce the data. The authors show that, in /sup 156/Dy, and with the inclusion of the gamma -band, a /b K/=0 or a /b K/=1 superband can explain the data equally well. The parameters of the band-mixing model may be reduced by using, for the g-, gamma - and beta -bands, a generalization of the rotational-vibrational model. The g, gamma , beta - and s/b K/ band mixing fits are greatly improved if the moment of inertia of the g-, gamma - and beta -bands are described by the VMI model. Inclusion of the low spin members of the superband in the fit indicates a slight preference for an s0 band.
- Affiliations
Citations
El Masri, Y., Vervier, J., & Faessler, A. (1977). The nature of the superband in backbending for the nucleus /sup 156 /Dy. Nuclear Physics, Section A, A279(2), 223-236. https://hdl.handle.net/2078.5/149204 (Original work published 1977)