NSR Query Results
Output year order : Descending NSR database version of April 27, 2024. Search: Author = E.N.van Dalen Found 21 matches. 2020SU07 Phys.Rev. C 101, 034302 (2020) X.Sun, R.Xu, Y.Tian, Z.Ma, Z.Zhang, Z.Ge, H.Zhang, E.N.E.van Dalen, H.Muther Relativistic mean-field approach in nuclear systems NUCLEAR STRUCTURE 16O, 40,48Ca, 90Zr, 116,132Sn, 208Pb; calculated binding energy per nucleon, charge radii, charge density distribution, single particle energies, spin-orbit splitting in 16O, scalar and vector potentials for neutrons and protons as a function of isospin asymmetry using both local density approximation (LDA) and improved LDA, based on Dirac-Brueckner-Hartree-Fock (DBHF) approach starting from a realistic nucleon-nucleon interaction. Comparison with experimental data.
doi: 10.1103/PhysRevC.101.034302
2016XU07 Phys.Rev. C 94, 034606 (2016) R.Xu, Z.Ma, Y.Zhang, Y.Tian, E.N.E.van Dalen, H.Muther Global analysis of isospin dependent microscopic nucleon-nucleus optical potentials in a Dirac-Brueckner-Hartree-Fock approach NUCLEAR REACTIONS 40Ca(n, n), E=2.06-185.0 MeV; 208Pb(n, n), E=1.8-155.0 MeV; 12C(n, n), E=1.04-225.0 MeV; 56Fe(n, n), E=1.8-75.0 MeV; 98Mo(n, n), E=1.5-26.0 MeV; 103Rh(n, n), E=4.51-10.0 MeV; 28Si, 90Zr, 120Sn(n, n), E=65 MeV; 27Al(n, n), E=3.2-26.0 MeV; 40Ca, 56Fe(p, p), E=61.5, 65 MeV; 28Si(p, p), E=14.26-250.0 MeV; 58Ni(p, p), E=7.0-250.0 MeV; 90Zr(p, p), E=9.7-185.0 MeV; 208Pb(p, p), E=16.0-201.0 MeV; calculated σ(θ, E). 12C, 40Ca(polarized n, n), E=10.9 MeV; 58Ni(polarized n, n), E=9.92 MeV; 208Pb(polarized n, n), E=9.97 MeV; 56Fe(polarized p, p), E=16.0-65.0 MeV; 58Ni(polarized p, p), E=16.0-250.0 MeV; 208Pb(polarized p, p), E=80, 200 MeV; calculated analyzing powers Ay(θ, E). 12C, 56Fe, 208Pb(n, X), 40Ca, 120Sn, 208Pb(p, X), E<200 MeV; calculated reaction σ(E). Global analysis of the isospin dependent nucleon-nucleus microscopic optical potential (MOP) based on the DBHF calculation in symmetric and asymmetric nuclear matter; deduced relativistic MOP for nucleon-nucleus scattering. Comparisons with experimental data, and with results from phenomenological Koning-Delaroche global potential. Compiled bibliographic information for experimental (n, n) data for 12C, 14N, 16O, 23Na, 24Mg, 27Al, 28Si, 31P, 32S, 39K, 40Ca, 48Ti, 52Cr, 55Mn, 56Fe, 59Co, 58Ni, 63Cu, 80Se, 88Sr, 89Y, 90Zr, 93Nb, 98Mo, 103Rh, 115In, 120Sn, 197Au, 208Pb, 209Bi targets, and experimental (p, p) data for 12C, 27Al, 28Si, 40Ca, 56Fe, 58Ni, 90Zr, 120Sn, 208Pb targets.
doi: 10.1103/PhysRevC.94.034606
2014VA13 Phys.Rev. C 90, 034312 (2014) Triaxial deformation in nuclei with realistic NN interactions NUCLEAR STRUCTURE 18,20,22,24,26,28,30,32,34Ne; calculated binding energies, neutron and proton single-particle energies, Fermi energies and rms radii, energy gaps, deformations, S(2n). Transition to pasta phase. 24,42Ne; calculated neutron and proton density distribution contours. Realistic NN interaction and Hartree-Fock approach. Comparison with experimental results.
doi: 10.1103/PhysRevC.90.034312
2013VA04 Phys.Rev. C 87, 024317 (2013) Spinodal instabilities in asymmetric nuclear matter based on realistic NN interactions
doi: 10.1103/PhysRevC.87.024317
2012XU03 Phys.Rev. C 85, 034613 (2012) R.Xu, Z.Ma, E.N.E.van Dalen, H.Muther Relativistic nucleon optical potentials with isospin dependence in a Dirac-Brueckner-Hartree-Fock approach NUCLEAR REACTIONS 27Al(n, n), (p, p), E=0.1-250 MeV; calculated Schrodinger equivalent central potential, spin-orbit, and Darwin potentials as function of incident energy and deformation parameter, σ(θ, E), vector analyzing powers. Relativistic microscopical optical potential (RMOP) method in the framework of Dirac-Brueckner-Hartree-Fock (DBHF). Comparison with experimental data.
doi: 10.1103/PhysRevC.85.034613
2011VA10 Phys.Rev. C 84, 024320 (2011) Relativistic description of finite nuclei based on realistic NN interactions NUCLEAR STRUCTURE 16O, 40,48Ca, 90Zr; calculated binding energies per nucleon, charge radii, spin-orbit splittings, proton density distribution for 16O. Density-dependent relativistic Hartree (DDRH), and density-dependent relativistic HF (DDRHF) theories. Comparison with experimental data.
doi: 10.1103/PhysRevC.84.024320
2010GR05 Phys.Rev. C 82, 014315 (2010) P.Grygorov, E.N.E.van Dalen, H.Muther, J.Margueron Separable form of a low-momentum realistic NN interaction
doi: 10.1103/PhysRevC.82.014315
2010VA09 Phys.Rev. C 82, 014319 (2010) Off-shell behavior of nucleon self-energy in asymmetric nuclear matter
doi: 10.1103/PhysRevC.82.014319
2009GO04 Phys.Rev. C 79, 024308 (2009) P.Gogelein, E.N.E.van Dalen, Kh.Gad, Kh.S.A.Hassaneen, H.Muther Properties of asymmetric nuclear matter in different approaches
doi: 10.1103/PhysRevC.79.024308
2009VA11 Phys.Rev. C 80, 037303 (2009) Nuclear saturation with low momentum interactions
doi: 10.1103/PhysRevC.80.037303
2009VA12 Phys.Rev. C 80, 044312 (2009) E.N.E.van Dalen, P.Gogelein, H.Muther Bulk properties of nuclei and realistic NN interactions NUCLEAR STRUCTURE 16O, 40,48,60Ca, 208Pb; calculated density distributions, binding energy, rms radii, single-particle energies, and neutron and proton wave functions using Hartree-Fock approach with realistic nucleon-nucleon interaction, interaction model and unitary-model operator method.
doi: 10.1103/PhysRevC.80.044312
2008GO04 Phys.Rev. C 77, 025802 (2008) P.Gogelein, E.N.E.van Dalen, C.Fuchs, H.Muther Nuclear matter in the crust of neutron stars derived from realistic NN interaction
doi: 10.1103/PhysRevC.77.025802
2007VA02 Eur.Phys.J. A 31, 29 (2007) E.N.E.van Dalen, C.Fuchs, A.Faessler Dirac-Brueckner-Hartree-Fock calculations for isospin asymmetric nuclear matter based on improved approximation schemes
doi: 10.1140/epja/i2006-10165-x
2006KL08 Phys.Rev. C 74, 035802 (2006) T.Klahn, D.Blaschke, S.Typel, E.N.E.van Dalen, A.Faessler, C.Fuchs, T.Gaitanos, H.Grigorian, A.Ho, E.E.Kolomeitsev, M.C.Miller, G.Ropke, J.Trumper, D.N.Voskresensky, F.Weber, H.H.Wolter Constraints on the high-density nuclear equation of state from the phenomenology of compact stars and heavy-ion collisions
doi: 10.1103/PhysRevC.74.035802
2006PL01 Phys.Rev. C 73, 014003 (2006) O.Plohl, C.Fuchs, E.N.E.van Dalen Model-independent study of the Dirac structure of the nucleon-nucleon interaction
doi: 10.1103/PhysRevC.73.014003
2005VA22 Phys.Rev.Lett. 95, 022302 (2005) E.N.E.van Dalen, C.Fuchs, A.Faessler Effective Nucleon Masses in Symmetric and Asymmetric Nuclear Matter
doi: 10.1103/PhysRevLett.95.022302
2005VA35 Phys.Rev. C 72, 065803 (2005) E.N.E.van Dalen, C.Fuchs, A.Faessler Momentum, density, and isospin dependence of symmetric and asymmetric nuclear matter properties
doi: 10.1103/PhysRevC.72.065803
2004VA05 Phys.Rev. C 69, 025802 (2004) E.N.E.van Dalen, A.E.L.Dieperink Bulk viscosity in neutron stars from hyperons
doi: 10.1103/PhysRevC.69.025802
2004VA26 Nucl.Phys. A744, 227 (2004) E.N.E.van Dalen, C.Fuchs, A.Faessler The relativistic Dirac-Brueckner approach to asymmetric nuclear matter
doi: 10.1016/j.nuclphysa.2004.08.019
2003VA06 Phys.Rev. C 67, 065807 (2003) E.N.E.van Dalen, A.E.L.Dieperink, J.A.Tjon Neutrino emission in neutron stars
doi: 10.1103/PhysRevC.67.065807
2002TI04 Phys.Rev. C65, 064007 (2002) R.G.E.Timmermans, A.Yu.Korchin, E.N.E.van Dalen, A.E.L.Dieperink Soft Electroweak Bremsstrahlung: Theorems and astrophysical relevance NUCLEAR REACTIONS 1n, 1H(n, nX), (n, pX), E not given; calculated electroweak bremsstrahlung amplitudes, matrix elements, axial-vector currents. 1n(n, nνν-bar), E at 50-300 MeV/c; calculated σ. Astrophysical implications discussed.
doi: 10.1103/PhysRevC.65.064007
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