2-6 December 2013
Cape Town
Africa/Johannesburg timezone
Abstract submission is closed. Registration will close on 22 November.

Beta-decay spectroscopy of N=82 nuclei and the path of the r-process:

2 Dec 2013, 16:40
25m

Speaker

Mr Giuseppe Lorusso (RIKEN)

Description

The shell structure at N = 82 plays a crucial role for the rapid neutron capture (r-) process. For example, it determines the shape of the large A∼130 peak in the solar system abundance pattern and affects the timescale of the r-process as well as the amount of neutrons later available for induced fission. However, below Z = 50 the evolution of the N = 82 gap is still unknown and, therefore, the predictions of neutron separation energies, half-lives, and neutron capture cross sections are uncertain making the location and duration of the r-process still an open question. Clearly, more experimental data are needed to provide r-process calculations and nuclear models with experimental inputs. To address this problem we have performed a decay-spectroscopy experiment at the Radioactive Ion Beam Factory (RIBF, RIKEN) in the neutron-rich region below 132Sn. The recent beam development of RIBF, along with the installation of the EURICA γ-ray detector have made this region accessible to decay-spectroscopy experiments. The nuclei of interest were produced by fission of a 345A MeV 238 U primary beam colliding with a 9Be target. Beam purification was provided by the BigRIPS fragment Separator. The fragments of interest were unambiguously identified and their following β decays were recorded by the WAS3ABi silicon stopper in conjunction with the EURICA germanium array. Implantations were correlated with their subsequent decays on an event-by-event basis allowing for the measurement of half-lives, β-delayed γ rays, and γ rays from implanted microsecond isomers. In particular, about 30 new half-lives have been measured, including the r-process waiting point 128Pd. In this contribution we will present the experiment and the preliminary results of the data analysis. The astrophysical implications of these results will also be discussed.

Primary author

Co-authors

Andrea Jungclaus (Istituto de Estructura de la Materia) Daisuke Kameda (RIKEN) Gary Simpson (University Joseph Furier) Hiroshi Suzuki (RIKEN) Hiroshi Watanabe (University of Beihang) Hiroyuki Takeda (RIKEN) Jin Wu (RIKEN) Kenta Yoshinaga (Tokyo University of Science) Naohito Inabe (RIKEN) Naoki Fukuda (RIKEN) Pieter Doornenbal (RIKEN) Shunji nishimura (RIKEN) Soderstorm Par-Anders (RIKEN) Toshiyuki Kubo (RIKEN) Toshiyuki Sumikama (Tohoku University) Yohei Shimizu (RIKEN) Zhengyu Xu (University of Tokyo)

Presentation Materials

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