Astronomy and Astrophysics – Astrophysics
Scientific paper
Aug 2006
adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2006ennp.conf..411b&link_type=abstract
"EXOTIC NUCLEI AND NUCLEAR/PARTICLE ASTROPHYSICS . Proceedings of the Carpathian Summer School of Physics 2005 . Held 13-24 June
Astronomy and Astrophysics
Astrophysics
Scientific paper
A γ-rigid solution of the Bohr Hamiltonian for γ = 30° is derived, its β-part being related to the second order Casimir operator of the Euclidean algebra E(4). The solution is called Z(4), since it corresponds to the Z(5) model with the γ variable "frozen". Parameter-free (up to overall scale factors) predictions for spectra and B(E2) transition rates are in close agreement to the E(5) critical point symmetry, as well as to experimental data in the Xe region around A = 130.
Bonatsos Dennis
Lenis D.
Petrellis D.
Terziev P. A.
Yigitoglu I.
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