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dc.contributor.authorLenis, D.
dc.contributor.authorYigitoglu, I.
dc.contributor.authorPetrellis, D.
dc.contributor.authorTerziev, P. A.
dc.contributor.authorBonatsos, D.
dc.date.accessioned2021-03-05T08:35:38Z
dc.date.available2021-03-05T08:35:38Z
dc.identifier.citationBonatsos D., Lenis D., Petrellis D., Terziev P. A. , Yigitoglu I., "Z(4): gamma-rigid solution of the Bohr Hamiltonian for gamma=30 degrees compared to the E(5) critical point symmetry", International Conference on Frontiers in Nuclear Structure, Astrophysics and Reactions (FINUSTAR), Kos, Yunanistan, 12 - 17 Eylül 2005, cilt.831, ss.415-416
dc.identifier.othervv_1032021
dc.identifier.otherav_99b53e71-ad43-47b0-9bd0-c4a764296f1d
dc.identifier.urihttp://hdl.handle.net/20.500.12627/103360
dc.description.abstractA gamma-rigid solution of the Bohr Hamiltonian for gamma = 30 degrees is derived, its beta-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 gamma 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.
dc.language.isoeng
dc.subjectFİZİK, NÜKLEER
dc.subjectAstronomi ve Astrofizik
dc.subjectDisiplinlerarası Fizik ve İlgili Bilim ve Teknoloji Alanları
dc.subjectTemel Bilimler
dc.subjectFİZİK, MULTİDİSİPLİNER
dc.subjectFizik
dc.subjectTemel Bilimler (SCI)
dc.subjectUzay bilimi
dc.subjectASTRONOMİ VE ASTROFİZİK
dc.titleZ(4): gamma-rigid solution of the Bohr Hamiltonian for gamma=30 degrees compared to the E(5) critical point symmetry
dc.typeBildiri
dc.contributor.departmentNational Centre of Scientific Research "Demokritos" , ,
dc.identifier.volume831
dc.contributor.firstauthorID131661


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