NSR Query Results
Output year order : Descending NSR database version of May 6, 2024. Search: Author = S.Antic Found 4 matches. 2021BO13 Phys.Rev. C 103, 055804 (2021) O.Boukari, H.Pais, S.Antic, C.Providencia Critical properties of calibrated relativistic mean-field models for the transition to warm, nonhomogeneous nuclear and stellar matter
doi: 10.1103/PhysRevC.103.055804
2020AN18 Phys.Rev. C 102, 065801 (2020) S.Antic, J.R.Stone, J.C.Miller, K.L.Martinez, P.A.M.Guichon, A.W.Thomas Outer crust of a cold, nonaccreting neutron star within the quark-meson-coupling model NUCLEAR STRUCTURE Z=26-50, N=20-90; calculated nuclear binding energies, two-neutron drip line using the QMCπ-III mass model, and compared with experimental data. 56Fe, 62,64,66,78Ni, 80Zn, 82Ge, 84Se, 86,118,120Kr, 120,122,124Sr, 121Y, 122Zr, 124Mo, 126Ru; calculated numerical results of the equation of state (EOSs) in the outer crust of cold nonaccreting, nonrotating neutron stars, such as baryon number densities at the bottom and top of each layer, and neutron and electron chemical potentials, and properties of individual layers in the outer crust. Comparison with results from FRDM, HFB24, and NL3 mass models.
doi: 10.1103/PhysRevC.102.065801
2020BA15 Acta Phys.Pol. B51, 611 (2020) P.Baczyk, M.Konieczka, K.M.L.Martinez, S.Antic, P.A.M.Guichon, W.Satula, J.R.Stone, A.W.Thomas On Introducing Charge-Symmetry-Breaking Terms to Nuclear Energy Density Functionals
doi: 10.5506/APhysPolB.51.611
2015AN02 Nucl.Phys. A938, 92 (2015) Neutron star equations of state with optical potential constraint
doi: 10.1016/j.nuclphysa.2015.03.004
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