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Abstract:

The low-lying positive-parity states of doubly even titanium isotopes are analyzed with the classical semimicroscopic model which involves the coupling of a two-proton cluster to the corresponding vibrational cores. The calculated energy-level sequence and electromagnetic properties compare favorably with experiment although no attempt to the best fit to individual properties was pursued. Comparison with calculated values with other models is also performed. NUCLEAR STRUCTURE Ti44, Ti46, Ti48, and Ti52; calculated levels, J, , B(E2), B(M1), q, , , , b. Classical semimicroscopic model. © 1979 The American Physical Society.

Registro:

Documento: Artículo
Título:Classical semimicroscopic model applied to doubly even titanium isotopes
Autor:Abecasis, S.M.; Carcione, J.M.
Filiación:Laboratorio de Radiaciones, Departamento de Fisica, Universidad de Buenos Aires, Nunez, 1428 Buenos Aires, Argentina
Año:1979
Volumen:19
Número:4
Página de inicio:1535
Página de fin:1543
DOI: http://dx.doi.org/10.1103/PhysRevC.19.1535
Título revista:Physical Review C
ISSN:05562813
Registro:https://bibliotecadigital.exactas.uba.ar/collection/paper/document/paper_05562813_v19_n4_p1535_Abecasis

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Citas:

---------- APA ----------
Abecasis, S.M. & Carcione, J.M. (1979) . Classical semimicroscopic model applied to doubly even titanium isotopes. Physical Review C, 19(4), 1535-1543.
http://dx.doi.org/10.1103/PhysRevC.19.1535
---------- CHICAGO ----------
Abecasis, S.M., Carcione, J.M. "Classical semimicroscopic model applied to doubly even titanium isotopes" . Physical Review C 19, no. 4 (1979) : 1535-1543.
http://dx.doi.org/10.1103/PhysRevC.19.1535
---------- MLA ----------
Abecasis, S.M., Carcione, J.M. "Classical semimicroscopic model applied to doubly even titanium isotopes" . Physical Review C, vol. 19, no. 4, 1979, pp. 1535-1543.
http://dx.doi.org/10.1103/PhysRevC.19.1535
---------- VANCOUVER ----------
Abecasis, S.M., Carcione, J.M. Classical semimicroscopic model applied to doubly even titanium isotopes. 1979;19(4):1535-1543.
http://dx.doi.org/10.1103/PhysRevC.19.1535