Nuclear curvature energy in relativistic models

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dc.contributor	Universitat de Barcelona
dc.contributor.author	Centelles Aixalà, Mario
dc.contributor.author	Viñas Gausí, Xavier
dc.contributor.author	Schuck, Peter
dc.date	2010-01-28T16:28:42Z
dc.date	2010-01-28T16:28:42Z
dc.date	1996
dc.identifier.citation	0556-2813
dc.identifier.citation	112677
dc.identifier.uri	http://hdl.handle.net/2445/10967
dc.format	4 p.
dc.format	application/pdf
dc.language.iso	eng
dc.publisher	The American Physical Society
dc.relation	Reproducció digital del document publicat en format paper, proporcionada per PROLA i http://dx.doi.org/
dc.relation	Physical Review C, 1996, vol. 53, núm. 2, p. 1018-1021
dc.rights	(c) The American Physical Society, 1996
dc.rights	info:eu-repo/semantics/openAccess
dc.subject	Estructura nuclear
dc.subject	Relativitat (Física)
dc.subject	Models nuclears
dc.subject	Nuclear structure
dc.subject	Relativity (Physics)
dc.subject	Nuclear models
dc.title	Nuclear curvature energy in relativistic models
dc.type	info:eu-repo/semantics/article
dc.type	info:eu-repo/semantics/publishedVersion
dc.description.abstract	The difficulties arising in the calculation of the nuclear curvature energy are analyzed in detail, especially with reference to relativistic models. It is underlined that the implicit dependence on curvature of the quantal wave functions is directly accessible only in a semiclassical framework. It is shown that also in the relativistic models quantal and semiclassical calculations of the curvature energy are in good agreement.

Bhagwat, A.; Viñas Gausí, Xavier; Centelles Aixalà, Mario; Schuck, Peter; Wyss, R.

Bhagwat, A.; Viñas Gausí, Xavier; Centelles Aixalà, Mario; Schuck, Peter; Wyss, R.

Centelles Aixalà, Mario; Schuck, Peter; Viñas Gausí, Xavier

Viñas Gausí, Xavier; Schuck, Peter; Centelles Aixalà, Mario; Farine, M.

Centelles Aixalà, Mario; Leboeuf, P.; Monastra, A. G.; Roccia, J.; Schuck, Peter; Viñas Gausí, Xavier

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