Variational Wigner-Kirkwood approach to relativistic mean field theory

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dc.contributor	Universitat de Barcelona
dc.contributor.author	Estal, Manuel del
dc.contributor.author	Centelles Aixalà, Mario
dc.contributor.author	Viñas Gausí, Xavier
dc.date	2010-01-28T16:31:18Z
dc.date	2010-01-28T16:31:18Z
dc.date	1997
dc.identifier.citation	0556-2813
dc.identifier.citation	121799
dc.identifier.uri	http://hdl.handle.net/2445/10969
dc.format	8 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/10.1103/PhysRevC.56.1774
dc.relation	Physical Review C, 1997, vol. 56, núm. 4, p. 1774-1781
dc.relation	http://dx.doi.org/10.1103/PhysRevC.56.1774
dc.rights	(c) The American Physical Society, 1997
dc.rights	info:eu-repo/semantics/openAccess
dc.subject	Estructura nuclear
dc.subject	Física nuclear
dc.subject	Nuclear structure
dc.subject	Nuclear physics
dc.title	Variational Wigner-Kirkwood approach to relativistic mean field theory
dc.type	info:eu-repo/semantics/article
dc.type	info:eu-repo/semantics/publishedVersion
dc.description.abstract	The recently developed variational Wigner-Kirkwood approach is extended to the relativistic mean field theory for finite nuclei. A numerical application to the calculation of the surface energy coefficient in semi-infinite nuclear matter is presented. The new method is contrasted with the standard density functional theory and the fully quantal approach.