Feb 22 – 23, 2024
Centro Congressi Partenope
Europe/Rome timezone

 

 

 

The slow neutron capture process (s-process) is one of the main mechanisms for the production of heavy elements in stars. In the recent years great effort was devoted on improving our knowledge on the nuclear reactions primarily responsible for s-process, i.e.13C(a,n)16O and 22Ne(a,n)25Mg.

 

This conference has the main goal of bringing together the international community of nuclear astrophysicists working on s-process reactions to share the present state of the art and coordinate future efforts which are still necessary for a more accurate understanding of s-process. As main follow up, a review article on this topic is expected to be coordinated by the participants.

 

Starts
Ends
Europe/Rome
Centro Congressi Partenope
Sala B
Via Partenope, 36, 80121 Napoli, Italy
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Local Organising Commitee

 

Chemseddine Ananna - Università degli Studi di Napoli "Federico II"

Daniela Mercogliano - Università degli Studi di Napoli "Federico II"

Daniele Dell'Aquila - Università degli Studi di Napoli "Federico II"

David Rapagnani (chair) - Università degli Studi di Napoli "Federico II" 

Raffaele Buompane - Università degli Studi della Campania "L. Vanvitelli"

 

Scientific Advisory Board

 

Andreas Best  - Università degli Studi di Napoli "Federico II"

Antonino DiLeva  - Università degli Studi di Napoli "Federico II"

David Rapagnani  - Università degli Studi di Napoli "Federico II"

Gianluca Imbriani  - Università degli Studi di Napoli "Federico II"

James DeBoer - University of Notre Dame

Michael Wiescher (chair) - University of Notre Dame