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dc.contributor.authorLenis, D
dc.contributor.authorYigitoglu, I
dc.contributor.authorPetrellis, D
dc.contributor.authorTerziev, PA
dc.contributor.authorBonatsos, D
dc.date.accessioned2021-03-03T09:40:42Z
dc.date.available2021-03-03T09:40:42Z
dc.identifier.citationBonatsos D., Lenis D., Petrellis D., Terziev P., Yigitoglu I., "X(3): an exactly separable gamma-rigid version of the X(5) critical point symmetry", PHYSICS LETTERS B, cilt.632, ss.238-242, 2006
dc.identifier.issn0370-2693
dc.identifier.othervv_1032021
dc.identifier.otherav_1e48067d-8a9d-4859-b57f-1706c9a3391b
dc.identifier.urihttp://hdl.handle.net/20.500.12627/25519
dc.identifier.urihttps://doi.org/10.1016/j.physletb.2005.10.060
dc.description.abstractA gamma-rigid version (with gamma = 0) of the X(5) critical point symmetry is constructed. The model, to be called X(3) since it is proved to contain three degrees of freedom, utilizes an infinite well potential, is based on exact separation of variables, and leads to parameter free (up to overall scale factors) predictions for spectra and B(E2) transition rates, which are in good agreement with existing experimental data for Os-172 and Pt-186. An unexpected similarity of the beta(1)-bands of the X(5) nuclei Nd-150, Sm-152, Gd-154, and Dy-156 to the X(3) predictions is observed. (c) 2005 Elsevier B.V. All rights reserved.
dc.language.isoeng
dc.subjectTemel Parçacıklar ve Alanlar
dc.subjectTemel Bilimler
dc.subjectFİZİK, NÜKLEER
dc.subjectFizik
dc.subjectFİZİK, PARTİKLER VE ALANLAR
dc.subjectAstronomi ve Astrofizik
dc.subjectTemel Bilimler (SCI)
dc.subjectUzay bilimi
dc.subjectASTRONOMİ VE ASTROFİZİK
dc.titleX(3): an exactly separable gamma-rigid version of the X(5) critical point symmetry
dc.typeMakale
dc.relation.journalPHYSICS LETTERS B
dc.contributor.department, ,
dc.identifier.volume632
dc.identifier.startpage238
dc.identifier.endpage242
dc.contributor.firstauthorID177386


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