NSR Query Results
Output year order : Descending NSR database version of April 27, 2024. Search: Author = W.Poschl Found 11 matches. 1999BA95 J.Phys.(London) G25, L109 (1999) Lattice Gauge Description of Colliding Nuclei
doi: 10.1088/0954-3899/25/11/101
1999PO30 Nucl.Phys. A661, 641c (1999) Real-Time Evolution of Soft QCD in Ultra-Relativistic Heavy-Ion Collisions
doi: 10.1016/S0375-9474(99)85107-0
1999SC35 Phys.Rev. C60, 054309 (1999) R.Schmidt, F.J.Hartmann, B.Ketzer, T.von Egidy, T.Czosnyka, J.Jastrzebski, M.Kisielinski, P.Lubinski, P.Napiorkowski, L.Pienkowski, A.Trzcinska, B.Klos, R.Smolanczuk, S.Wycech, W.Poschl, K.Gulda, W.Kurcewicz, E.Widmann Composition of the Nuclear Periphery from Antiproton Absorption using Short-Lived Residual Nuclei NUCLEAR REACTIONS 48Ca, 100Mo, 104Ru, 112,124Sn, 116Cd(p-bar, X), E at rest; measured Eγ, Iγ(t) following residual nucleus decay; deduced yields, isomeric ratios. 48Ca, 100Mo, 104Ru, 112,124Sn, 116Cd deduced peripheral neutron-to-proton ratios, effective scattering lengths of antiprotons. Comparison with Hartree-Fock-Bogoliubov calculations.
doi: 10.1103/PhysRevC.60.054309
1998LA06 Phys.Lett. 418B, 7 (1998) G.A.Lalazissis, D.Vretenar, W.Poschl, P.Ring Reduction of the Spin-Orbit Potential in Light Drip-Line Nuclei NUCLEAR STRUCTURE Ne, Mg; calculated even isotopes spin-orbit potentials, radii; deduced spin-orbit interaction isospin dependence. Relativistic, nonrelativistic mean-field models.
doi: 10.1016/S0370-2693(97)01473-1
1998LA08 Nucl.Phys. A632, 363 (1998) G.A.Lalazissis, D.Vretenar, W.Poschl, P.Ring Relativistic Hartree-Bogoliubov Description of the Neutron Drip-Line in Light Nuclei NUCLEAR STRUCTURE Z=6-12; calculated level energies, mass radii for neutron-rich nuclei. Relativistic Hartree-Bogoliubov approach.
doi: 10.1016/S0375-9474(98)00009-8
1998VR02 Phys.Rev. C57, R1060 (1998) D.Vretenar, W.Poschl, G.A.Lalazissis, P.Ring Relativistic Mean-Field Description of Light Λ Hypernuclei with Large Neutron Excess NUCLEAR STRUCTURE 28,30,32,34,36,38,40,42Ne; calculated normal, hypernuclei neutron single-particle levels; deduced Λ hyperon effect. Relativistic Hartree Bogoliubov model.
doi: 10.1103/PhysRevC.57.R1060
1997ME11 Z.Phys. A358, 123 (1997) Relativistic Hartree-Bogoliubov Description of the Lithium Isotopes NUCLEAR STRUCTURE 6,7,8,9,10,11Li; calculated binding energies, mass radii; deduced halo structure features. Relativistic Hartree-Bogoliubov theory, Gogny force.
doi: 10.1007/s002180050285
1997PO14 Phys.Rev.Lett. 79, 3841 (1997) W.Poschl, D.Vretenar, G.A.Lalazissis, P.Ring Relativistic Hartree-Bogoliubov Theory with Finite Range Pairing Forcces in Coordinate Space: Neutron halo in light nuclei NUCLEAR STRUCTURE 12,14,16,18,20,22,24,26C, 20,22,24,26,28,30,32,34,36,38,40,42Ne; calculated proton, neutron, mass rms radii, single-particle levels, neutron, proton densities, pairing field for some Ne isotopes; deduced neutron halo features. Relativistic Hartree Bogoliubov model.
doi: 10.1103/PhysRevLett.79.3841
1997VR01 Nucl.Phys. A621, 853 (1997) D.Vretenar, G.A.Lalazissis, R.Behnsch, W.Poschl, P.Ring Monopole Giant Resonances and Nuclear Compressibility in Relativistic Mean Field Theory NUCLEAR STRUCTURE 90Zr, 114Sn, 208Pb, 40,48Ca, 16O; calculated isoscalar monopole states, nuclear compressibilities, isovector monopole moments in some cases. Relativistic mean field theory.
doi: 10.1016/S0375-9474(97)00192-9
1995PO10 Z.Phys. A351, 271 (1995) The Eigenspectrum of the Relativistic Two-Center Hamiltonian in the Diatomic Basis of Bound Hydrogenlike Dirac-Spinors NUCLEAR REACTIONS Hg, U(U, X), I(I, X), Pb(Cl, X), E not given; calculated compound system binding energies, eigenspectra. Two-center Dirac Hamiltonian dynamics description.
1995PO12 Phys.Rev. C52, 1532 (1995) W.Poschl, M.Schaden, K.Dietrich Correlated Pair Conversion in Heavy-Ion Collisions at the Coulomb Barrier NUCLEAR REACTIONS 232Th, 238U(238U, X), 232Th(232Th, X), E ≈ Coulomb barrier; analyzed positron singles, (e+e-)-pair sum energy spectra; deduced emission scenario. Correlated pair formation model.
doi: 10.1103/PhysRevC.52.1532
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