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dc.contributor.authorMINKOV, N.
dc.contributor.authorPetrellis, Dımıtrıos
dc.contributor.authorQuesne, C.
dc.contributor.authorBONATSOS, Dennis
dc.date.accessioned2021-03-02T23:18:16Z
dc.date.available2021-03-02T23:18:16Z
dc.identifier.citationBONATSOS D., MINKOV N., Petrellis D., Quesne C., "Bohr Hamiltonian with deformation-dependent mass", 1st NUBA International Conference on Nuclear Physics and Astrophysics, Antalya, Türkiye, 14 - 21 Eylül 2014, cilt.590
dc.identifier.othervv_1032021
dc.identifier.otherav_11ad1f68-2b0e-492d-8327-a50eba933030
dc.identifier.urihttp://hdl.handle.net/20.500.12627/17349
dc.identifier.urihttps://doi.org/10.1088/1742-6596/590/1/012004
dc.description.abstractThe Bohr Hamiltonian with a mass depending on the nuclear deformation is solved using the techniques of supersymmetric quantum mechanics (SUSYQM). Analytical expressions for spectra and wave functions are obtained. Spectra and B(E2) transition rates are calculated for more than 50 gamma-unstable nuclei and more than 60 prolate deformed nuclei using the Davidson potential and the Kratzer potential. In addition to solving the long standing problem of the too rapid increase of the moment of inertia with deformation, the method reveals a conformal factor in the Bohr Hamiltonian, embedding the Bohr space in six dimensions.
dc.language.isoeng
dc.subjectAstronomi ve Astrofizik
dc.subjectDisiplinlerarası Fizik ve İlgili Bilim ve Teknoloji Alanları
dc.subjectTemel Bilimler
dc.subjectFizik
dc.subjectFİZİK, NÜKLEER
dc.subjectFİZİK, MULTİDİSİPLİNER
dc.subjectTemel Bilimler (SCI)
dc.subjectUzay bilimi
dc.subjectASTRONOMİ VE ASTROFİZİK
dc.titleBohr Hamiltonian with deformation-dependent mass
dc.typeBildiri
dc.contributor.departmentNational Centre of Scientific Research "Demokritos" , ,
dc.identifier.volume590
dc.contributor.firstauthorID100277


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