Microscopic description of collective motion in pf shell nuclei
✍ Scribed by H. Müther; K. Allaart; K. Goeke; A. Faessler
- Publisher
- Elsevier Science
- Year
- 1975
- Tongue
- English
- Weight
- 659 KB
- Volume
- 248
- Category
- Article
- ISSN
- 0375-9474
No coin nor oath required. For personal study only.
📜 SIMILAR VOLUMES
The weak interaction rates in stellar environments are computed for p f -shell nuclei in the mass range A = 45-65 using large-scale shell-model calculations. The calculated capture and decay rates take into consideration the latest experimental energy levels and log f t-values. The rates are tabulat
From the assumption that the collective Hamiltonian be invariant under the orthogonal group O(A -1, iR) it is concluded that classical collective dynamics can be formulated on a symplectic manifold. This manifold is shown to be a coset space of the symplectic group Y/2(6, [R) of dimension 12, 16 or