Conveners
Session 4
- Daniele Mengoni (Istituto Nazionale di Fisica Nucleare)
To assess the Universe chemical evolution a crucial ingredient is the cross section of nuclear reactions taking place in stars. Given its low value, pico- to femto-barn, at astrophysical energies, that prevents direct measurements and we still have to rely on extrapolation. The contribution of narrow or of large sub-threshold resonances, which may dominate the reaction rate, cannot be,...
B. Gongora,$^{1}$ P.~Aguilera,$^1$ G.~Andreetta,$^2$ F.~Angelini,$^2$ M.~Balogh,$^2$ J.~Benito,$^2$ G.~Benzoni,$^3$ S.~Bottoni,$^3$ D.~Brugnara,$^{4}$ G.~de Angelis,$^2$ S.~Carollo,$^1$ G.~Corbari,$^3$ A.~Ertoprak,$^{5}$ R.~Escudeiro,$^{6}$ C.~Fransen,$^{7}$ A.~Gadea,$^8$ F.~Galtarossa,$^1$ D.~Genna,$^3$ A.~Giaz,$^3$ A.~Goasduff,$^1$ A.~Gottardo,$^1$ J.~Ha,$^{1}$ S.M.~Lenzi,$^1$...
.
Nuclei in the vicinity of 208Pb are a good testing ground for different models and in particular those differing from the doubly closed shell by a few particles such as 206Hg or 204Pt. This region has been explored in the past using fragmentation reactions [1,2], multi-nucleon transfer [3] allowing to measure lifetimes of isomeric states and perform spectroscopy of states below the isomers. On...
