Please use this identifier to cite or link to this item: http://hdl.handle.net/10261/15533
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dc.contributor.authorAntonov, A. N.-
dc.contributor.authorKadrev, D. N.-
dc.contributor.authorGaidarov, M. K.-
dc.contributor.authorMoya de Guerra, Elvira-
dc.contributor.authorSarriguren, Pedro-
dc.contributor.authorUdias, J. M.-
dc.contributor.authorLukyanov, V. K.-
dc.contributor.authorZemlyanaya, E. V.-
dc.contributor.authorKrumova, G. Z.-
dc.date.accessioned2009-07-30T11:10:52Z-
dc.date.available2009-07-30T11:10:52Z-
dc.date.issued2005-10-20-
dc.identifier.citationPhysical Review C 72(4): 044307 (2005)en_US
dc.identifier.issn0556-2813-
dc.identifier.urihttp://hdl.handle.net/10261/15533-
dc.description11 pages, 3 tables, 11 figures.-- PACS nrs.: 21.10.Ft; 21.10.Gv; 25.30.Bf; 21.60.−n.-- ArXiv pre-print available at: http://arxiv.org/abs/nucl-th/0506056v2en_US
dc.description.abstractResults of charge form factors calculations for several unstable neutron-rich isotopes of light, medium, and heavy nuclei (He, Li, Ni, Kr, Sn) are presented and compared to those of stable isotopes in the same isotopic chain. For the lighter isotopes (He and Li) the proton and neutron densities are obtained within a microscopic large-scale shell-model, while for heavier ones Ni, Kr, and Sn the densities are calculated in deformed self-consistent mean-field Skyrme HF+BCS method. We also compare proton densities to matter densities together with their rms radii and diffuseness parameter values. Whenever possible comparison of form factors, densities and rms radii with available experimental data is also performed. Calculations of form factors are carried out both in plane wave Born approximation (PWBA) and in distorted wave Born approximation (DWBA). These form factors are suggested as predictions for the future experiments on the electron-radioactive beam colliders where the effect of the neutron halo or skin on the proton distributions in exotic nuclei is planned to be studied and thereby the various theoretical models of exotic nuclei will be tested.en_US
dc.description.sponsorshipThis work was partly supported by the Agreement (2004 BG2004) between the CSIC (Spain) and the Bulgarian Academy of Sciences, by the Agreement between JINR (Dubna) and INRNE (Sofia), and by funds provided by MEC (Spain) under Contract Nos. BFM 2002-03562 and 2003-04147-C02-01.en_US
dc.format.extent658973 bytes-
dc.format.mimetypeapplication/pdf-
dc.language.isoengen_US
dc.publisherAmerican Physical Societyen_US
dc.rightsopenAccessen_US
dc.subject[PACS] Charge distributionen_US
dc.subject[PACS] Nucleon distributions and halo featuresen_US
dc.subject[PACS] Elastic electron scatteringen_US
dc.subject[PACS] Nuclear structure models and methodsen_US
dc.titleCharge and matter distributions and form factors of light, medium, and heavy neutron-rich nucleien_US
dc.typeartículoen_US
dc.identifier.doi10.1103/PhysRevC.72.044307-
dc.description.peerreviewedPeer revieweden_US
dc.relation.publisherversionhttp://link.aps.org/doi/10.1103/PhysRevC.72.044307en_US
dc.identifier.e-issn1089-490X-
dc.type.coarhttp://purl.org/coar/resource_type/c_6501es_ES
item.openairecristypehttp://purl.org/coar/resource_type/c_18cf-
item.grantfulltextopen-
item.openairetypeartículo-
item.fulltextWith Fulltext-
item.languageiso639-1en-
item.cerifentitytypePublications-
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