PI: Alba Formicola, Andreas Best

WG members: M Aliotta, A Best, A Boeltzig, C Broggini, C Bruno, A Caciolli, F Cavanna, GF Ciani, T Davinson, G D'Erasmo, A Di Leva, E Fiore, A Formicola, C Gustavino, G Imbriani, M Junker, I Kochanek, V Mossa, FR Pantaleo, V Paticchio, R Perrino, P Prati, L Schiavulli, O Straniero, A Valentini, S Zavatarelli 

 

Astrophysical Motivation:

  • neutron source in AGB stars 

  • nucleosynthesis of heavy elements

  • s-process neutron capture

 

Documentation