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NSR database version of May 10, 2024.

Search: Author = S.Sewailem

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2019RA09      Phys.Rev. C 99, 034604 (2019)

M.Rashdan, Sh.Sewailem

Effects of in-medium NN cross section and density distribution on the reaction cross sections of Ne, Mg, and O isotopes with 12C at 1 GeV

NUCLEAR STRUCTURE 16,17,18,19,20,21,22,23,24O, 18,19,20,21,22,23,24,25,26,27,28,29,30,31,32Ne, 20,21,22,23,24,25,26,27,28,29,30,31,32,33,34,36Mg; calculated rms neutron, proton and matter radii, and neutron, proton and matter β2 deformation parameters for Mg nuclei using relativistic mean-field theory in an axially symmetric deformed basis, with the relativistic mean-field Lagrangian density, and NL3* force parameter.

NUCLEAR REACTIONS 12C(16O, X), (17O, X), (18O, X), (19O, X), (20O, X), (21O, X), (22O, X), (23O, X), (24O, X), (18Ne, X), (19Ne, X), (20Ne, X), (21Ne, X), (22Ne, X), (23Ne, X), (24Ne, X), (25Ne, X), (26Ne, X), (27Ne, X), (28Ne, X), (29Ne, X), (30Ne, X), (31Ne, X), (32Ne, X), (20Mg, X), (21Mg, X), (22Mg, X), (23Mg, X), (24Mg, X), (25Mg, X), (26Mg, X), (27Mg, X), (28Mg, X), (29Mg, X), (30Mg, X), (31Mg, X), (32Mg, X), (33Mg, X), (34Mg, X), (36Mg, X), E AP 1 GeV/nucleon; calculated reaction σ using Glauber theory with different nucleon-nucleon cross section models and nuclear densities. Comparison with experimental data, and with other theoretical calculations.

doi: 10.1103/PhysRevC.99.034604
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