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Almudena Arcones
(TU Darmstadt, GSI)
04.08.12, 15:30
I will discuss the origin of lighter heavy elements (Sr, Y, Zr) in neutrino-driven winds.
Dr.
Matthew Mumpower
(North Carolina State University)
04.08.12, 16:00
The potential of an astrophysical environment for making r-process elements has been typically characterized by the neutron-to-seed ratio. We consider the rare earth peak as a new and independent tool for understanding the astrophysical conditions favorable for the main r-process. In the context of a high entropy r-process we discuss rare earth peak formation. We use features of a successful...
Dr.
Shi-Sheng Zhang
(School of Physics and Nuclear Energy Engineering, Beihang University, Beijing 100191, China)
04.08.12, 16:30
Single-particle resonant states embedded in the continuum for Sn, in the vicinity of the neutron capture threshold for Sn(n, ), are calculated by the analytical continuation of the coupling constant (ACCC) approach within the relativistic mean field (RMF) theory framework. Our fully self-consistent RMF calculations using the NL3 effective interaction,
predict...
Prof.
Toshio Suzuki
(Nihon University)
04.08.12, 17:00
β decays of the isotones with N = 126 are studied by shell-model calculations taking into account both the Gamow-Teller (GT) and first-forbidden (FF) transitions [1]. Shell-model interaction of Ref. [2] is adopted and a quenching of g_A^{eff}/g_A =0.7 is used for both the GT and FF transitions except for 0^{-} case. The FF transitions [3] are found to be important to reduce the beta-decay...
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Dr. Shi-Sheng Zhang
Single particle levels in Sn-131 and Sn-133 on the path of r-process nucleosynthesis
The Sebel Hotel
16:30 - 17:00
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