SECTION III: NUCLEAR THEORY | |
Astrophysical
Factor for the Neutron Generator 13C(α,n)16O
Reaction in the AGB Stars ................................................................................III-1 The
Trojan Horse Method: an Indirect Technique in Nuclear Astrophysics
......................................................................................................III-3 The
Lowest Excited States pf 13O andAstrophysical Implications
......................................................................................................................III-4 Can We Measure
the Spectroscopic Factors from Nuclear Reaction? ..............................................................................................................III-6 Wide
Resonant States in 15F .................................................................................................................................................................................III-7 Self-Consistency
in Hartree-Fock RPA and Low-Lying States in Nuclei ..........................................................................................................III-9 Self-Consistent
Hartree-Fock RPA and Energy Weighted Sum Rule ...............................................................................................................III-10 Continuous
Phase Transition and Negative Specific Heat in Finite Nuclei
......................................................................................................III-12 Fully
Self-Consistent HF-RPA Calculations with Modern Skyrme Interaction
...............................................................................................III-13 Nuclear
Imcompressibility Coefficient within Fermi Liquid Drop Model
........................................................................................................III-15 Charm
Elliptic Flow at RHIC .............................................................................................................................................................................III-17 Anisotropic
Flows in Cu+Au Collisions at √SNN= 200 GeV
............................................................................................................................III-18 System
Size Dependence of Elliptic Flows in Relativistic Heavy-Ion Collisions
...........................................................................................III-19 Eta
Absorption by Mesons ..............................................................................................................................................................................III-21 Nuclear
Symmetry Energy and the Neutron Skin Thickness of Heavy Nuclei
...........................................................................................III-22 φ
and Ω Production in Relativistic Heavy-Ion Collision in a Dynamical
Coalescence Model ...................................................................III-23 Hadron
Production from Quark Coalescence and Jet Fragmentation
.........................................................................................................III-24 High-Energy
Behavior of the Nuclear Symmetry Potential in Asymmetric Nuclear Matter
.....................................................................III-25 Comprehensive
Interpretation of Thermal Dileptons at the SPS ................................................................................................................III-26 Bottomonium
Production at RHIC and LHC ................................................................................................................................................III-29 Low-Energy
Thermal Photons from Hadronic Matter ................................................................................................................................III-35 Self-Consistent
Approximations to a Model with Spontaneously Broken O(N) Symmetry
.....................................................................III-37 A
New Analysis of 14O Beta Decay: Branching Ratios and CVC
Consistency .................................................................................................III-39
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