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NSR database version of April 26, 2024.

Search: Author = S.Antic

Found 4 matches.

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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
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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
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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
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2015AN02      Nucl.Phys. A938, 92 (2015)

S.Antic, S.Typel

Neutron star equations of state with optical potential constraint

doi: 10.1016/j.nuclphysa.2015.03.004
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