Please use this identifier to cite or link to this item: http://hdl.handle.net/2445/45426
Title: Origin of the neutron skin thickness of 208Pb in nuclear mean-field models
Author: Centelles Aixalà, Mario
Roca-Maza, X.
Viñas Gausí, Xavier
Warda, M.
Keywords: Física nuclear
Astrofísica
Estructura nuclear
Partícules (Física nuclear)
Nuclear physics
Astrophysics
Nuclear structure
Particles (Nuclear physics)
Issue Date: 2010
Publisher: American Physical Society
Abstract: We study whether the neutron skin thickness Δrnp of 208Pb originates from the bulk or from the surface of the nucleon density distributions, according to the mean-field models of nuclear structure, and find that it depends on the stiffness of the nuclear symmetry energy. The bulk contribution to Δrnp arises from an extended sharp radius of neutrons, whereas the surface contribution arises from different widths of the neutron and proton surfaces. Nuclear models where the symmetry energy is stiff, as typical of relativistic models, predict a bulk contribution in Δrnp of 208Pb about twice as large as the surface contribution. In contrast, models with a soft symmetry energy like common nonrelativistic models predict that Δrnp of 208Pb is divided similarly into bulk and surface parts. Indeed, if the symmetry energy is supersoft, the surface contribution becomes dominant. We note that the linear correlation of Δrnp of 208Pb with the density derivative of the nuclear symmetry energy arises from the bulk part of Δrnp. We also note that most models predict a mixed-type (between halo and skin) neutron distribution for 208Pb. Although the halo-type limit is actually found in the models with a supersoft symmetry energy, the skin-type limit is not supported by any mean-field model. Finally, we compute parity-violating electron scattering in the conditions of the 208Pb parity radius experiment (PREX) and obtain a pocket formula for the parity-violating asymmetry in terms of the parameters that characterize the shape of the 208Pb nucleon densities.
Note: Reproducció del document publicat a: http://dx.doi.org/10.1103/PhysRevC.82.054314
It is part of: Physical Review C, 2010, vol. 82, num. 5, p. 054314-1-054314-10
Related resource: http://dx.doi.org/10.1103/PhysRevC.82.054314
URI: http://hdl.handle.net/2445/45426
ISSN: 0556-2813
Appears in Collections:Articles publicats en revistes (Física Quàntica i Astrofísica)

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