Axel Boeltzig
(GSSI)
23/06/2017, 10:40
Oral
The reaction 23Na(p,γ)24Mg links the NeNa and MgAl cycles in stellar hydrogen burning. For temperatures up to 100MK, typical for RGB and low and intermediate mass AGB stars, the rate of this reaction is predominantly determined by the non-resonant component of the cross section and possibly by a narrow resonance at E(c.m.)=138keV. An upper limit for the strength of this resonance has been...
Dr
Daniele Dell'Aquila
(Univ. Napoli Federico II and INFN - Napoli, Italy)
23/06/2017, 11:00
Oral
Given as .tex file
Dr
Rosanna Depalo
(Università degli Studi di Padova and INFN Padova)
23/06/2017, 11:20
Oral
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Mr
Philipp Scholz
(Institut für Kernphysik, Universität zu Köln, Cologne, Germany)
23/06/2017, 11:40
Oral
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Concetta Parascandolo
(NA)
23/06/2017, 12:00
Oral
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Viviana Mossa
(Università degli Studi di Bari and INFN, sezione di Bari)
23/06/2017, 12:20
Oral
Study of the 2H(p,γ)3He reaction in the Big Bang nucleosynthesis energy range at LUNA
V. Mossa for the LUNA collaboration
Università degli Studi di Bari and INFN, sezione di Bari
Contact email: viviana.mossa@ba.infn.it
The Big Bang Nucleosynthesis (BBN) describes the production of light nuclides in the first minutes of cosmic time. It started with deuterium accumulation when the...
Dr
Tamás Szücs
(MTA Atomki)
23/06/2017, 12:40
Stellar evolution and nucleosynthesis
Oral
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