NSR Query Results
Output year order : Descending NSR database version of May 10, 2024. Search: Author = C.Keil Found 7 matches. 2004LE17 Prog.Part.Nucl.Phys. 53, 153 (2004) Correlation dynamics in dripline nuclei
doi: 10.1016/j.ppnp.2004.02.020
2002KE08 J.Phys.(London) G28, 1683 (2002) In-Medium Baryon Interactions and Hypernuclear Structure
doi: 10.1088/0954-3899/28/7/320
2002KE15 Phys.Rev. C 66, 054307 (2002) Hypernuclear Auger effect within density dependent relativistic hadron field theory NUCLEAR STRUCTURE 209Pb; calculated hypernucleus level energies, Auger transition strength distributions. Density-dependent relativistic hadron field theory.
doi: 10.1103/PhysRevC.66.054307
2001HO26 Phys.Rev. C64, 025804 (2001) Application of the Density Dependent Hadron Field Theory to Neutron Star Matter
doi: 10.1103/PhysRevC.64.025804
2001HO28 Phys.Rev. C64, 034314 (2001) Density Dependence Hadron Field Theory for Asymmetric Nuclear Matter and Exotic Nuclei NUCLEAR STRUCTURE 16O, 40,48Ca, 48,56,68Ni, 90Zr, 100,132Sn, 208Pb; calculated charge radii, binding energies. Ni, Sn; calculated binding energies, two-neutron separation energies. Density-dependent hadron field theory.
doi: 10.1103/PhysRevC.64.034314
2001LE21 Prog.Part.Nucl.Phys. 46, 187 (2001) Probing Isospin Dynamics in Halo Nuclei NUCLEAR STRUCTURE 8B, 11Be, 17,19C; calculated ground-state J, π, spectroscopic factors. Many-body theory, core polarization calculations. NUCLEAR REACTIONS 12C(8B, X), (11Be, X), (17C, X), (19C, X), E ≈ 900-1500 MeV; calculated one-nucleon removal σ. Many-body theory, core polarization calculations.
doi: 10.1016/S0146-6410(01)00123-5
2000KE07 Phys.Rev. C61, 064309 (2000) Density Dependent Hadron Field Theory for Hypernuclei NUCLEAR STRUCTURE 9Be, 10B, 13C, 16O, 28Si, 40Ca, 51V, 89Y, 139La, 208Pb; calculated hyperon single-particle energies, spin-orbit splitting. Density dependent hadron field theory. Comparisons with data.
doi: 10.1103/PhysRevC.61.064309
Back to query form Note: The following list of authors and aliases matches the search parameter C.Keil: , C.M.KEIL |