NSR Query Results
Output year order : Descending NSR database version of May 6, 2024. Search: Author = H.M.Ding Found 5 matches. 2001DI19 Nucl.Phys. A692, 549 (2001) Nuclear Transparency in Heavy-Ion Collisions at 14.6 GeV/nucleon NUCLEAR REACTIONS Pb(28Si, X), E=14.6 GeV/nucleon; calculated fragments transverse energy distributions, proton rapidity, multiplicity; deduced transparency features. Glauber theory, quantum molecular dynamics, comparisons with data.
doi: 10.1016/S0375-9474(01)00657-1
1998LU17 Eur.Phys.J. A 3, 377 (1998) X.-F.Lu, B.S.Zou, H.-M.Ding, Y.-X.Liu, E.-G.Zhao Contribution of the σ Meson Exchange to Pionic Double Charge Exchange Reaction NUCLEAR REACTIONS 14C(π+, π-), E < 300 MeV; calculated forward excitation function; deduced sigma-meson exchange contribution.
doi: 10.1007/s100500050192
1996DI01 Phys.Rev. C53, 1985 (1996) Stretched Alignment Due to Pairing Correlation between the Normal and Abnormal Parity Orbits for the γ-Soft Nuclei in the Light Rare-Earth Region NUCLEAR STRUCTURE 118,120,122,124,126,128Xe, 126,128,130,132Ba; calculated level energy vs τ(τ+3), τ is SO(5) group parameter; deduced pairing correlation role between normal, abnormal orbits. Fermion dynamical symmetry model based two-parameter model.
doi: 10.1103/PhysRevC.53.1985
1996WU05 Phys.Rev.Lett. 76, 4132 (1996) L.-A.Wu, H.-M.Ding, Z.-T.Yan, G.Liu Unified Description of Collective Bands of Even-Even Nuclei and Fingerprint of the Nuclear γ Shape NUCLEAR STRUCTURE 156,158,160,162,164Dy; analyzed yrast level data; deduced parameter R. A=80-248; analyzed data; deduced relative root square deviation. 190,192,194Hg; analyzed data; deduced superdeformed bands, parameter R, relative root square deviation.
doi: 10.1103/PhysRevLett.76.4132
1995WU07 Phys.Rev. C52, 1845 (1995) Pairing Correlations between the Normal and Abnormal Parity Orbits and the Mechanism of the Stretching Effect NUCLEAR STRUCTURE 226Ra, 228,230,232Th, 248Cm, 230,232,234,236,238U, 236,238,240,242,244Pu; calculated levels. Fermion dynamical symmetry model.
doi: 10.1103/PhysRevC.52.1845
Back to query form |