Indirect Methods in Nuclear Astrophysics

Europe/Rome
Meeting room (ECT* - Villa Tambosi - Trento)

Meeting room

ECT* - Villa Tambosi - Trento

Strada delle Tabarelle, 286 38123 - Villazzano (TN) Italy
Livius Trache (IFIN - HH) (“Horia Hulubei” National Institute for Physics and Nuclear), Angela Bonaccorso (INFN Pisa) (INFN Pisa), Carlos Bertulani (Texas A&M) (Texas A&M University-Commerce), Tohru Motobayashi (RIKEN) (RIKEN, Nishina Center for Accelerator based Science, Wako), Zsolt Fulop (MTA ATOMKI ) (MTA ATOMKI Debrecen - Hungary)
Description

Indirect Methods in Nuclear Astrophysics

The workshop intends to identify the most promising indirect methods in nuclear astrophysics, to discuss their particulars and to assess their reliability. We want a broad discussion to: -review the existing indirect methods -assess the problems with their accuracy, in particular those arising from the calculated absolute values -emphasize the need for modern codes -assess the sets of parameters to use in calculations. Physicists working on stellar modeling together with theoreticians and experimentalists working in nuclear physics for astrophysics will meet with the purpose of identifying stellar scenarios needing nuclear reaction data that make sizable difference in stellar evolution and the optimal methods to obtain them. Such discussions are crucial for reliably using indirect methods for nuclear astrophysics and even to validate the very existence of many Rare Isotope Beams facilities which rely on them as one of as their main areas of research.

ECT*                             FBK                                      ENSAR2          

                                  

Secretariat - Ines Campo
  • Monday, 5 November
    • 08:30 09:00
      Registration 30m Rustico Hall (ECT* )

      Rustico Hall

      ECT*

Your browser is out of date!

Update your browser to view this website correctly. Update my browser now

×