Dr
Andreea Oprea
(Horia Hulubei National Institute for R&D in Physics and Nuclear Engineering (IFIN-HH))
15/06/2016, 14:00
Short Talk
A.Oprea1, T. Glodariu1,2, D. Filipescu1,2, I. Gheorghe1,2,
I. Cata-Danil1, N. Florea1, D. Bucurescu1, D.G. Ghita1,
N. Marginean1, R. Marginean1, C. Mihai1, A. Negret1, A. Olacel1,
S. Pascu1, R. Suvaila1, L. Stroe1, S. Toma1,3 and N.V. Zamfir1
1 Department of Nuclear Physics, Horia Hulubei National Institute for R&D in Physics and Nuclear Engineering (IFIN-HH)Magurele, Romania
2...
Mr
Tomoyasu Hayakawa
(Kyoto University)
15/06/2016, 14:10
Short Talk
Gamma Ray Bursts (GRBs) are among the most energetic events in the universe. GRBs are divided by the duration time into long GRBs and short GRBs. A popular model of the central engine of long GRBs involves a hyper accreting black hole (BH), created by a core collapse of a massive star (the collapsar model) [1].
Indeed, supernovae (SNe) have been observed to be associated with some GRBs since...
Mr
Fang Ni
(Univ. of Tsukuba)
15/06/2016, 14:20
Short Talk
Nuclei show a variety of collective phenomena. Especially, excited $0^+$ states in even-even nuclei show puzzling properties. Recent experiments reveal anomalous properties of the low-lying $0^+$ states. We presume that the pairing dynamics plays a significant role in these low-lying excited $0^+$ states. For instance, the $0_2^+$ states in $^{152}$Sm and $^{154}$Gd, which were interpreted as...
Mr
Chris Griffin
(University of Edinburgh)
15/06/2016, 14:30
Short Talk
The origin of the heavy elements is one of the most fundamental open questions in modern astrophysics, with a notable difficulty being the lack of a complete description of the rapid neutron-capture process (r-process) [1]. Two key quantities used in r-process calculations are β-decay half-lives and β-delayed neutron emission probabilities. The half-lives determine the timescale for the flow...
Ms
Miyu Masuyama
(University of Tokyo, Research center for the early universe)
15/06/2016, 14:40
Short Talk
Magnetars are neutron stars with strong magnetic fields(B~10^14-10^15G). The mechanism to make such a strong magnetic field and what kind of supernova generates a magnetar have not been well understood. Recent observations of supernova remnants associated with magnetars indicate that magnetar progenitors are massive stars and the typical explosion energy is 10^51 erg (e.g. Kumar et al., 2014,...
Mr
Hideki Shimizu
(CNS, University of Tokyo)
15/06/2016, 14:50
Short Talk
We will present an experimental plan to measure proton resonant elastic scattering with a thick target in inverse kinematics with a novel beam of isomeric Al-26 to be produced with CRIB at RIBF of RIKEN Nishina Center. The steady-state galactic abundance of the Al-26 radionuclide provides a unique window to the ongoing nucleosynthesis in the MIlky Way, as its decay along the galactic plane has...
