Nuclear Physics in Astrophysics VIII

Session

r-process 1

19 Jun 2017, 11:40

Sala conferenze (Laboratori Nazionali del Sud)

125. Explosive nucleosynthesis of heavy elements: an astrophysical and nuclear physics challenge

Prof. Gabriel Martínez Pinedo (Technische Universität Darmstadt)

19/06/2017, 11:40

Invited talk

Half of the elements heavier than iron are produced by the r process under extreme conditions. To identify its site remains one of the major challenges in nuclear astrophysics. Advances in the description of neutrino-matter interactions and its implementation in core-collapse super- nova modelling have lead to the conclusion that supernova explosions only contribute to the production of...

94. Solving the mystery of r-process: mergers vs. supernovae

Prof. Taka Kajino (NAOJ, The University of Tokyo)

19/06/2017, 12:10

Explosive scenarios in astrophysics: observations, theory, and experiments

Invited talk

Taka Kajino, Shota Shibagaki, Yutaka Hirai, Grant J. Mathews The origin of heavy elements heavier than iron like Au and U are still unknown although sixty years have already passed since the benchmark paper B2FH on the origin of elements in the Universe was published in 1957. GW emitters of both binary neutron-star mergers (NSMs) and core-collapse supernovae (SNe) are viable candidates for...

30. The neutrino process in supernova nucleosynthesis

Mr Andre Sieverding (Technische Universität Darmstadt)

19/06/2017, 12:40

Neutrinos and weak interaction in astrophysics

Oral

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9. Roles of nuclear weak rates on the evolution of degenerate cores in stars

Prof. Toshio Suzuki (Nihon University)

19/06/2017, 13:00

Oral

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