Proceedings of the International Workshop on Unstable Nuclei in Astrophysics, Tokyo, Japan, 7-8 June 1991
著者
書誌事項
Proceedings of the International Workshop on Unstable Nuclei in Astrophysics, Tokyo, Japan, 7-8 June 1991
World Scientific, 1992
- タイトル別名
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Unstable nuclei in astrophysics
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注記
Includes bibliographical reference and index
内容説明・目次
内容説明
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.
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