The main theme of the workshop is to discuss problems of nucleosynthesis in the Universe, specifically in connections to the unstable atomic nuclei, which would play a crucial role in explosive burning processes. This subject is strongly backed up by an increasing interest in studying unstable nuclei in nuclear physics.The subjects include primordial nucleosynthesis, Hot-CNO cycle and rapid-proton process, neutrino-induced nucleosynthesis, equation of state of neutron-rich matter etc.
目次
The "r"-process in supernovae, B.S. Meyer et al
recent advances in primordial nucleosynthesis, R.N. Boyd
fermion dynamical symmetries, nuclear masses, and their astrophysical implications, D.H. Feng
new generation calculations of beta decay far from stability and astrophysics, H.V. Klapdor-Kleingrothaus
impact of the nuclear equation of state on models of rotating neutron stars, F. Weber and N.K. Glendenning
signatures of inhomogeneous cosmologies
intermediate-mass nucleosynthesis and radioactive nuclear beams, T. Kajino
study of the key reaction 8Li(alpha,n)11B for the primordial nucleosynthesis, S. Kubono et al
the "p"-process in type-II supernovae, M. Arnould et al
the 12C(alpha,gamma)16O cross section at low energies, F.C. Barker and T. Kajino
explosive nucleosynthesis in type II supernovae, K. Nomoto et al
helium burning in some astrophysical scenarios, M. Gai
production of nuclei on the proton drip line for 31</=Z</=37, D.J. Morrissey et al
properties of dense supernovae matter and neutron stars at the birth, T. Takatsuka
the neutrino process and neutrino "r"-process, W.C. Haxton
coulomb dissociation for nuclear astrophysics, G. Baur
some new developments in polarization radioactive beams, S.S. Hanna.