@inproceedings{0a12664926214dd88bafa98516f63634,
title = "Experimental challenge to nuclear physics problems in the νp-process",
abstract = "Astrophysical stellar reactions at extremely high temperatures involve a variety of problems both in nuclear reactions and nuclear structures. Specifically, the problems in the νpprocess were discussed in this talk based on our recent experimental results with low-energy RI beams and a simulation study. The νp-process is one of the key processes for investigating the mechanism of type II supernovae, and the process could be possibly responsible for {"}the excess production{"} of p-nuclei around mass 90-100. Alpha cluster resonances have been discovered experimentally to play a crucial role for the stellar (α, p) reactions just above the alpha threshold. Neutron induced reactions in the proton-rich nuclear regions in the νp-process are also suggested to play an important role, which involve nuclear structures of high level density at high excitation energies, probably giant resonances. The discussion also covered the p-nuclei production through the νp-process at around mass 100.",
keywords = "The νp-process, breakout of the pp chain, cluster nucleosynthesis, low-energy RI beam, neutron induced reactions, nuclear structure of p-rich nuclei, p-nuclei production, αp-process",
author = "S. Kubono and Binh, {Dam N.} and S. Hayakawa and T. Hashimoto and Kahl, {D. M.} and H. Yamaguchi and Y. Wakabayashi and T. Teranishi and N. Iwasa and T. Komatsubara and S. Kato and A. Chen and S. Cherubini and Choi, {S. H.} and Hahn, {I. S.} and He, {J. J.} and Khiem, {Le H.} and Lee, {C. S.} and Kwon, {Y. K.} and S. Wanajo and Janka, {H. T.}",
year = "2012",
doi = "10.1063/1.4763394",
language = "English",
isbn = "9780735410961",
series = "AIP Conference Proceedings",
pages = "189--196",
booktitle = "Origin of Matter and Evolution of Galaxies 2011",
note = "International Symposium on Origin of Matter and Evolutions of Galaxies 2011, OMEG 2011 ; Conference date: 14-11-2011 Through 17-11-2011",
}