Charge and matter distributions and form factors of light, medium, and heavy neutron-rich nuclei
| Autor: | V. K. Lukyanov, E. V. Zemlyanaya, Anton Nikolaev Antonov, Pedro Sarriguren, M. K. Gaidarov, D. N. Kadrev, E. Moya de Guerra, G. Z. Krumova, J. M. Udías |
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| Rok vydání: | 2005 |
| Předmět: |
Physics
Nuclear and High Energy Physics [PACS] Elastic electron scattering Nuclear Theory Proton Stable isotope ratio Isotopes of lithium FOS: Physical sciences Charge density [PACS] Nucleon distributions and halo features Nuclear Theory (nucl-th) Nuclear physics [PACS] Nuclear structure models and methods Isotopes of tin [PACS] Charge distribution Neutron Born approximation Atomic physics Nuclear Experiment Isotopes of helium |
| Zdroj: | Digital.CSIC. Repositorio Institucional del CSIC instname |
| ISSN: | 1089-490X 0556-2813 |
| DOI: | 10.1103/physrevc.72.044307 |
| Popis: | 11 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/0506056v2 Results 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. This 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. |
| Databáze: | OpenAIRE |
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