Speaker
Cristian Massimi
(Universita e INFN, Bologna (IT))
Description
We show the impact on AGB stellar nucleosynthesis of the maxwellian averaged capture cross sections determined at n_TOF over the past 20 years. We developed an automated procedure to derive MACSs from evaluated data libraries, which are subsequently used as input to stellar models computed by means of the FUNS code.
In this contribution, we present a number of s-process abundances obtained using different data libraries as input to stellar models, with a focus on the role of n_TOF data.
Primary authors
Alberto Mengoni
(ENEA & INFN, Bologna)
Cristian Massimi
(Universita e INFN, Bologna (IT))
Diego Vescovi
(GSSI e INFN Perugia (IT))
Francesco Giacomini
(INFN CNAF)
Mr
Samuele Lanzi
(University of Bologna)
Sergio Cristallo
(INFN, Perugia (IT), and Osservatorio Astronomico di Teramo, INAF, Teramo (IT))
