-
Axel Boeltzig (GSSI)23/06/2017, 10:40OralThe 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...Go to contribution page
-
Dr Daniele Dell'Aquila (Univ. Napoli Federico II and INFN - Napoli, Italy)23/06/2017, 11:00OralGiven as .tex fileGo to contribution page
-
Dr Rosanna Depalo (Università degli Studi di Padova and INFN Padova)23/06/2017, 11:20Oral% % Nuclear Physics in Astrophysics 8 template for abstract % % Format: LaTeX2e. % % Rename this file to name.tex, where `name' is the family name % of the first author, and edit it to produce your abstract. % \documentstyle[11pt]{article} % % PAGE LAYOUT: % \textheight=9.9in \textwidth=6.3in \voffset -0.85in \hoffset ...Go to contribution page
-
Mr Philipp Scholz (Institut für Kernphysik, Universität zu Köln, Cologne, Germany)23/06/2017, 11:40Oral% % Nuclear Physics in Astrophysics 8 template for abstract % % Format: LaTeX2e. % % Rename this file to name.tex, where `name' is the family name % of the first author, and edit it to produce your abstract. % \documentstyle[11pt]{article} % % PAGE LAYOUT: % \textheight=9.9in \textwidth=6.3in \voffset -0.85in \hoffset ...Go to contribution page
-
Concetta Parascandolo (NA)23/06/2017, 12:00Oral% % Nuclear Physics in Astrophysics 8 template for abstract % % Format: LaTeX2e. % % Rename this file to name.tex, where `name' is the family name % of the first author, and edit it to produce your abstract. % \documentstyle[11pt]{article} % % PAGE LAYOUT: % \textheight=9.9in \textwidth=6.3in \voffset -0.85in \hoffset ...Go to contribution page
-
Viviana Mossa (Università degli Studi di Bari and INFN, sezione di Bari)23/06/2017, 12:20OralStudy 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...Go to contribution page
-
Dr Tamás Szücs (MTA Atomki)23/06/2017, 12:40Stellar evolution and nucleosynthesisOral% % Nuclear Physics in Astrophysics 8 template for abstract % % Format: LaTeX2e. % % Rename this file to name.tex, where `name' is the family name % of the first author, and edit it to produce your abstract. % \documentstyle[11pt]{article} % % PAGE LAYOUT: % \textheight=9.9in \textwidth=6.3in \voffset -0.85in \hoffset ...Go to contribution page
Choose timezone
Your profile timezone: