GIANTS-X

Programme

Mercoledì 23 Ottobre

 

14:30 Saluto del Direttore – Apertura del workshop

15:00 – 16:15 Nucleosintesi primordiale (F. Cavanna)

1. “⁷Li evolution in the thin and thick discs of the Milky Way” (G. Cescutti) (20’+5’)
2. Search for a resonance in the 6Li(p,gamma)7Be reaction (R. Depalo) (20’+5’)
3. "Influencing 7Be half-life” (C. Santonastaso) (20’+5’)

Coffee break

16:45 – 18:00 Nucleosintesi primordiale e combustione di H (G. Pizzone)

1. The primordial deuterium abundance : a precise measure of ²H(p, g)³He cross section at BBN energies (V. Mossa); (20’+5’)
2. Big Bang Nucleosynthesis investigated via the THM (R. Sparta’) (20’+5’)
3. "Cumulative uncertainty in age determination of old stellar clusters" (S. Degli’Innocenti) (20’+5’)

Visita guidata nel centro storico di Genova

 

Giovedì 24 Ottobre

8:30 – 10:15 Combustione di He e C (G. Imbriani)

1. "¹²C+¹²C reactions measurements: present and future" L. Gallegos Morales (20’+5’ )
2. The ¹²C+¹²C burning explored via the THM (G. Rapisarda) (20’+5’ )
3. The ¹²C+¹²C reaction study at LUNA (A. Guglielmetti) (20’+5’ )
4. "Implication on the new ¹²C+¹²C reaction rate to massive star evolution and nucleosynthesis” (A. Chieffi) (15’+5’ )

Coffee break

10:45 – 13:00 Le sorgenti di neutroni ed oltre (S. Zavatarelli)

1. Neutron induced reactions explored via the THM (Sergi L.) (20’+5’)
2. Low energy resonances in the reactions ²²Ne(a,g)²⁶Mg and ²²Ne(p,g)²³Na (D. Piatti) (20’+5’ )
3. "Everything you always wanted to know about the ¹³C pocket formation but were afraid to ask” (M. Busso) (25’+’5)
4. ¹³C(a,n)¹⁶O cross section in the Gamow peak (Best A.) (25’+5’)
5. The ¹⁹F and ²³Na destruction in stars (D’Agata G.) (20’+5’)

Pranzo

14:30 – 16:30 Sorgenti di neutroni e catture neutroniche (P. Milazzo)

1. Measurement of the ¹⁴⁰Ce(n, g) reaction at energies of astrophysical interest at n-TOF (S. Amaducci) (20’+5’ )
2. Measurement of the neutron capture cross section of the s-only 154Gd isotope (Massimi C.) (20’+5’)
3. The cosmic nucleosynthesis competition between low mass stars and neutron stars mergers (Vescovi D.) (20’+5’)
4. "Modelling of compact binary mergers: connecting nuclei to neutron stars” (A. Perego) (20'+5')

Coffee break

17:00 – 19:10 What’s else… (S. Palmerini)

1. Beta decay rates of highly ionized atoms in stellar environment (Mengoni A.) (20’+5’)
2. "News on Pre-supernova Evolution and Explosive Nucleosynthesis of Massive Stars" (A. Chieffi) (20’+5’ )
3. Fusion reactions in laser-induced plasma (D. Lattuada) (20’+5’)
4. Exploring photodissociation processes at astrophysical energies (G.L. Guardo) (20’+5’)
5. Neutron capture elements in the Galaxy (F. Matteucci) (20’+5’)

Cena Sociale

 

Venerdì 25 ottobre

8:30 – 10:30 What’s next (R. Buompane)

1. LUNA MV (M. Junker) (20’+5’ )
2. Nuclear astrophysics in the era of Multi Messenger Astronomy (La Cognata) (20’+5’ )
3. The new layout of ERNA for the next experiment on 12C(a,g)16O" J. Garcia Duarte(20’+5’)
4. “Application of isotope ratio mass spectrometry to nuclear physics: the contribution of CIRCE centre” (F. Terrasi) (20’+5’ )

Coffee break

11:00 – 13:00 Discussione Generale - Conclusioni (P. Corvisiero-C. Spitaleri)

1. L'astrofisica nucleare nella CSN3 (Nania R.) 
2. ChETEC (Caciolli A.)
3. About the Newsletter.
4. All together!!

Pranzo