Data
Feb
03
2023
Neutron-upscattering enhancement of the triple-alpha process featuring Jack Bishop (Texas A&M University) (Opens in a new window)
Online
Carbon is produced is stars mainly via the triple-alpha process where three helium nuclei fuse to form an excited state of carbon-12 known as the Hoyle state. This is a nuclear resonance (an excited form of a nucleus) that has properties that guide the rate that the triple alpha process takes place. Primarily, the key property is how often the Hoyle state is able to lose energy and end up in the ground state of carbon-12 – known as the radiative width.
Feb
17
2023
Neutron capture for the s-process, with a focus on LANSCE work & new capabilities featuring Aaron Couture (LANL) (Opens in a new window)
Online
IReNA Online Seminar to begin at 2pm ET
Mar
03
2023
Viability of Novae as Sources of Galactic Lithium featuring Alex Kemp (KU Leuven, Belgium) (Opens in a new window)
Online
IReNA Online Seminar to begin at 2pm ET
Mar
17
2023
N-process featuring Marco Pignitari (Konkoly Observatory) (Opens in a new window)
Online
IReNA Online Seminar to begin at 2pm ET
Mar
31
2023
Neutrino detection with BOREXINO experiment featuring Alessandra Carlotta Re (University of Milan, Italy) (Opens in a new window)
Online
IReNA Online Seminar to begin at 2pm
Apr
14
2023
Stellar spectroscopy, galactic archaeology featuring Miho Ishigaki (NAOJ) (Opens in a new window)
Online
IReNA Online Seminar to begin at 2pm ET
Apr
28
2023
Gravitational waves featuring Michèle Heurs (Leibniz Universität Hannover) (Opens in a new window)
Online
IReNA Online Seminar to begin at 2pm ET