NSR Query Results
Output year order : Descending NSR database version of April 27, 2024. Search: Author = A.Sulaksono Found 34 matches. 2024LI01 Nucl.Phys. A1042, 122812 (2024) N.Liliani, A.M.Nugraha, J.P.Diningrum, A.Sulaksono Tensor and isovector–isoscalar terms of relativistic mean field model: Impacts on neutron-skin thickness, charge radius, and nuclear matter NUCLEAR STRUCTURE 208Pb, 40,48Ca, 132Sn; calculated neutron skin thickness; deduced parameters using the combination of tensor and nonlinear isovector–isoscalar couplings in the RMF model. Comparison with the CREX and PREX collaborations data.
doi: 10.1016/j.nuclphysa.2023.122812
2024RI02 Phys.Rev. C 109, 025803 (2024) Impact of Fermi-surface distortion in a relativistic mean-field model on the moment of inertia and tidal deformability of neutron stars
doi: 10.1103/PhysRevC.109.025803
2022HU01 Nucl.Phys. A1017, 122356 (2022) P.T.P.Hutauruk, A.Sulaksono, K.Tsushima Effects of neutrino magnetic moment and charge radius constraints and medium modifications of the nucleon form factors on the neutrino mean free path in dense matter
doi: 10.1016/j.nuclphysa.2021.122356
2022HU02 Nucl.Phys. A1017, 122356 (2022) P.T.P.Hutauruk, A.Sulaksono, K.Tsushima Effects of neutrino magnetic moment and charge radius constraints and medium modifications of the nucleon form factors on the neutrino mean free path in dense matter
doi: 10.1016/j.nuclphysa.2021.122356
2021LI34 Phys.Rev. C 104, 015804 (2021) N.Liliani, J.P.Diningrum, A.Sulaksono Tensor and Coulomb-exchange terms in the relativistic mean-field model with δ-meson and isoscalar-isovector coupling NUCLEAR STRUCTURE A=10-220; 40Ca, 112,132Sn, 208Pb; calculated binding energies and rms radii, and deduced relative errors between the theoretical and experimental values. 202,204,206,208,210,212,214,216,218,220,222Pb; calculated S(2n). 40Ca, 132Sn, 208Pb; calculated neutron and proton single-particle energies. 208Pb; calculated rms radius as function of symmetry energy, neutron skin thickness in neutron star (NS). Relativistic mean-field (RMF) model with tensor couplings and Coulomb-exchange terms. Comparison with available experimental data.
doi: 10.1103/PhysRevC.104.015804
2021RA32 Phys.Rev. C 104, 065805 (2021) Recent multimessenger constraints and the anisotropic neutron star
doi: 10.1103/PhysRevC.104.065805
2019RI04 Phys.Rev. C 100, 055804 (2019) R.Rizaldy, A.R.Alfarasyi, A.Sulaksono, T.Sumaryada Neutron-star deformation due to anisotropic momentum distribution of neutron-star matter
doi: 10.1103/PhysRevC.100.055804
2017SU14 Phys.Rev. C 95, 045806 (2017) Influence of the nucleon radius on the properties of slowly rotating neutron stars
doi: 10.1103/PhysRevC.95.045806
2016AL25 Phys.Rev. C 94, 052801 (2016) N.Alam, B.K.Agrawal, M.Fortin, H.Pais, C.Providencia, Ad.R.Raduta, A.Sulaksono Strong correlations of neutron star radii with the slopes of nuclear matter incompressibility and symmetry energy at saturation
doi: 10.1103/PhysRevC.94.052801
2016LI28 Phys.Rev. C 93, 054322 (2016) N.Liliani, A.M.Nugraha, J.P.Diningrum, A.Sulaksono Impacts of the tensor couplings of ω and ρ mesons and Coulomb-exchange terms on superheavy nuclei and their relation to the symmetry energy NUCLEAR STRUCTURE A=8-210; 40Ca, 122Sn, 208Pb; calculated effects of the tensor couplings of ω and ρ meson terms, the Coulomb-exchange term, and the isoscalar-isovector couplings on relative errors of binding energies, rms radii, surface thicknesses, and diffraction radii. 208Pb; calculated correlation between the neutron skin thicknesses and symmetry energy. Z=82, N=118-138; N=126, Z=76-100; Z=120, N=160-190; N=172, Z=112-130; calculated binding energies, two-neutron and two-proton gaps, effects of tensor couplings, the Coulomb-exchange term and isoscalar-isovector couplings on two-neutron and two-proton gaps. 208Pb, 292120; calculated single-proton and single-neutron states, nucleon density distributions, neutron skin thicknesses and mean square charge radii and effects of tensor couplings and the Coulomb-exchange term with isoscalar-isovector couplings. Relativistic mean-field model calculations for the properties of nuclear matter, finite nuclei, and superheavy nuclei.
doi: 10.1103/PhysRevC.93.054322
2016MA21 Phys.Rev. C 93, 039802 (2016) Reply to "Comment on 'Nonidentical protons'"
doi: 10.1103/PhysRevC.93.039802
2016PA15 Phys.Rev. C 93, 045802 (2016) H.Pais, A.Sulaksono, B.K.Agrawal, C.Providencia Correlation of the neutron star crust-core properties with the slope of the symmetry energy and the lead skin thickness NUCLEAR STRUCTURE 48Ca, 132Sn, 208Pb; calculated total binding energies, charge and neutron radii for selected parametrizations, skin thickness for 208Pb; investigated correlations of crust-core transition density and pressure in neutron stars with the slope of the symmetry energy and neutron skin thickness using different families of mean-field parametrization in relativistic nonlinear Walecka model (NLWM). Asymmetric nuclear and stellar matter at zero temperature.
doi: 10.1103/PhysRevC.93.045802
2015AL17 Phys.Rev. C 92, 015804 (2015) N.Alam, A.Sulaksono, B.K.Agrawal Diversity of neutron star properties at the fixed neutron-skin thickness of 208Pb NUCLEAR STRUCTURE 48Ca, 132Sn, 208Pb; calculated binding energy, charge and neutron radii, neutron-skin thickness. 208Pb; calculated density dependence of symmetry energy, variations of symmetry energy slope parameter, core-crust transition density and pressure with neutron-skin thickness, mass-radius relationship, plots for the radius of the neutron stars and red shift, tidal polarizability parameter as function of neutron-star mass. Extended relativistic mean-field (RMF) model using different sets of parameters.
doi: 10.1103/PhysRevC.92.015804
2013AG06 Phys.Rev. C 87, 051306 (2013) B.K.Agrawal, J.N.De, S.K.Samaddar, G.Colo, A.Sulaksono Constraining the density dependence of the symmetry energy from nuclear masses NUCLEAR STRUCTURE 208Pb, 238U; calculated symmetry slope parameter L, neutron skin thickness for spherical and deformed nuclei, symmetry energy using a microscopic framework with different energy density functionals.
doi: 10.1103/PhysRevC.87.051306
2013MA11 Phys.Rev. C 87, 025807 (2013) Nonidentical protons
doi: 10.1103/PhysRevC.87.025807
2013MA85 Phys.Rev. C 88, 059802 (2013) Reply to "Comment on 'Nonidentical protons'"
doi: 10.1103/PhysRevC.88.059802
2013SU16 Phys.Rev. C 87, 065802 (2013) Effects of density-dependent lepton fraction on the properties of protoneutron stars
doi: 10.1103/PhysRevC.87.065802
2013SU21 Int.J.Mod.Phys. E22, 1350061 (2013) Cold fusion reactions using neutron-rich projectiles NUCLEAR REACTIONS 208Pb(58Fe, X)266Hs, 208Pb(64Fe, X)272Hs, 208Pb(64Ni, X)272Ds, 208Pb(72Ni, X)280Ds, 208Pb(70Zn, X)278Cn, 208Pb(78Zn, X)286Cn, 208Pb(76Ge, X)284Fl, 208Pb(84Ge, X)292Fl, 208Pb(88Se, X)296Lv, 208Pb(96Kr, X)304Og, E<40 MeV; calculated capture, fission and evaporation residue σ. Comparison with available data.
doi: 10.1142/S0218301313500614
2012AG13 Nucl.Phys. A882, 1 (2012) B.K.Agrawal, A.Sulaksono, P.-G.Reinhard Optimization of relativistic mean field model for finite nuclei to neutron star matter
doi: 10.1016/j.nuclphysa.2012.03.004
2012SU23 Nucl.Phys. A895, 44 (2012) Existence of hyperons in the pulsar PSRJ1614-2230
doi: 10.1016/j.nuclphysa.2012.09.006
2011SU21 Int.J.Mod.Phys. E20, 1983 (2011) Electromagnetic and isovector terms in standard relativistic mean field model NUCLEAR STRUCTURE 40,48Ca, 90Zr, 132Sn, 208Pb; calculated binding energy, rms radii, surface thickness, level energies, J, π. Relativistic mean field model.
doi: 10.1142/S0218301311019775
2009SU06 Phys.Rev. C 79, 044306 (2009) A.Sulaksono, T.J.Burvenich, P.-G.Reinhard, J.A.Maruhn Criteria for nonlinear parameters of relativistic mean field models
doi: 10.1103/PhysRevC.79.044306
2009SU21 Phys.Rev. C 80, 054317 (2009) Fine tuning in an effective field based relativistic mean field model, and properties of neutron-rich matter
doi: 10.1103/PhysRevC.80.054317
2008MA37 Phys.Rev. C 78, 025808 (2008) Low-density instability of multicomponent matter with trapped neutrinos
doi: 10.1103/PhysRevC.78.025808
2007HU05 Nucl.Phys. A782, 400c (2007) P.T.P.Hutauruk, A.Sulaksono, T.Mart Effects of the neutrino electromagnetic form factors on the neutrino and antineutrino mean free paths difference in dense matter
doi: 10.1016/j.nuclphysa.2006.10.034
2007SU21 Phys.Rev. C 76, 041301 (2007) A.Sulaksono, T.Mart, T.J.Burvenich, J.A.Maruhn Instabilities of relativistic mean field models and the role of nonlinear terms
doi: 10.1103/PhysRevC.76.041301
2006MA76 Phys.Rev. C 74, 055203 (2006) Kaon photoproduction in a multipole approach NUCLEAR REACTIONS 1H(γ, K+X), E ≈ 1.5-2.5 GeV; analyzed hyperon production data; deduced resonance contributions.
doi: 10.1103/PhysRevC.74.055203
2006SU03 Phys.Rev. C 73, 025803 (2006) A.Sulaksono, C.K.Williams, P.T.P.Hutauruk, T.Mart Effect of neutrino electromagnetic form factors on the neutrino cross section in dense matter
doi: 10.1103/PhysRevC.73.025803
2006SU17 Phys.Rev. C 74, 045806 (2006) Low density instability in relativistic mean field models
doi: 10.1103/PhysRevC.74.045806
2005SU05 Phys.Rev. C 71, 034312 (2005) Nilsson parameters κ and μ in relativistic mean field models NUCLEAR STRUCTURE 208Pb, 132Sn, 40Ca; calculated single-particle energies, spin-orbit splitting, Nilsson parameters; deduced role of effective mass. Relativistic mean-field models, comparison with data.
doi: 10.1103/PhysRevC.71.034312
2005SU26 Phys.Rev. C 72, 065801 (2005) A.Sulaksono, P.T.P.Hutauruk, T.Mart Isovector-channel role of relativistic mean field models in the neutrino mean free path
doi: 10.1103/PhysRevC.72.065801
2004BU18 Acta Phys.Hung.N.S. 19, 149 (2004) T.Burvenich, T.Cornelius, A.Sulaksono, J.A.Maruhn, W.Greiner, D.G.Madland, P.-G.Reinhard, S.Schramm Application and Extrapolation of Mean-Field Models in the Heavy and Superheavy Regions NUCLEAR STRUCTURE 292120; calculated neutron and proton density distributions. Relativistic point-coupling models.
doi: 10.1556/APH.19.2004.1-2.23
2004HU22 Phys.Rev. C 70, 068801 (2004) P.T.P.Hutauruk, C.K.Williams, A.Sulaksono, T.Mart Neutron fraction and neutrino mean free path predictions in relativistic mean field models
doi: 10.1103/PhysRevC.70.068801
2002BU35 Prog.Theor.Phys.(Kyoto), Suppl. 146, 130 (2002) T.Burvenich, D.G.Madland, A.Sulaksono, J.Maruhn, P.-G.Reinhard A Relativistic Point Coupling Model for Nuclear Structure Calculations NUCLEAR STRUCTURE 16O, 40,48Ca, 56,58Ni, 88Sr, 90Zr, 100,112,120,124,132Sn, 136Xe, 144Sm, 202,204,208Pb; calculated binding energies, radii. Relativistic point coupling model.
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