Jul
12
2019

Workshop on Nuclear Astrophysics Opportunities at ATLAS 2019 (Opens in a new window)

Argonne National Laboratory

Workshops & Conferences

The aim of the workshop is to bring the nuclear astrophysics community together to discuss opportunities available at the ATLAS facility, to foster new collaborations, and solicit new ideas for future advancement of the facility and experimental program. The ATLAS facility has undergone an expansion in its capabilities to produce and study isotopes of astrophysical interest, both through facility enhancements (CARIBU, RAISOR, the soon-to-be N=126 factory, etc.) and experimental devices/techniques (MUSIC, HELIOS, ion trapping, GRETINA, GAMMASPHERE, etc.).

Aug
12
2019

MICRA 2019 (Opens in a new window)

TPI in Jena, Germany

Workshops & Conferences

MICRA, which stands for Microphysics In Computational Relativistic Astrophysics, is a biennial workshop focused on improving, discussing, and addressing the microphysics needs of relativistic simulations of astrophysical systems, core-collapse supernovae, compact object mergers, and gamma-ray bursts by bringing together nuclear and neutrino theorists and astrophysicists and computational modelers. This year marks the 5th installment and the 10th anniversary of MICRA, and the first since the revolutionary gravitational wave event GW170817.

Sep
09
2019

CEMP Stars as Probes of First-Star Nucleosynthesis, the IMF, and Galactic Assembly (Opens in a new window)

Geneva, Switzerland

Workshops & Conferences

The beginning of the stellar era in the Universe is a singularly fascinating phase in the history of the Cosmos. The baryonic material filling the Universe at that time, having a composition inherited from Big Bang nucleosynthesis, has its physical characteristics modified by the very first stars. Indeed, the first stars will change the degree of ionized material in their vicinity, and, through their winds and/or supernova explosion, will inject energy, momentum, and newly-synthesized elements.

Sep
15
2019

Nuclear Physics in Astrophysics IX (Opens in a new window)

Frankfurt, Germany

Workshops & Conferences

Nuclear physics is the necessary link between astronomical observations, stellar models and galactic chemical evolution. The impressive progress in astrophysics during the last decades explaining and predicting astronomical scenarios was only possible because of the fruitful interplay between all disciplines. New insights in one field triggered new developments in the other fields. New experimental techniques are typically the response to new predictions and observations.

Sep
20
2019

Workshop on β-decay and Charge-exchange Reactions for Nuclear-astrophysics (Opens in a new window)

The University of Hong Kong

Workshops & Conferences

Transitions mediated by the weak interaction play important roles in a wide variety of astrophysical phenomena. The accurate description of beta decays and electron captures are necessary for modelling the evolution of stars, the description of nucleosynthesis upon their cataclysmic demise, for example in neutron-star mergers and core-collapse supernovae, and the interpretation of multi-messenger signals from such events. A wide variety of β-decay and electron-capture (EC) data are needed for use in astrophysical modelling.

Jun
08
2020

Astrophysics with Radioactive Isotopes (AwRI2020) (Opens in a new window)

Budapest, Hungary

Workshops & Conferences

Radioactive nuclei play a significant role in many current astrophysical quests. From the origin of the elements through the driving of the emissions from supernovae (56Ni) and kilonovae (r-process radioactivity), they are crucial for direct studies of galactic enrichment (7Be, 26Al, 44Ti, 60Fe, 99Tc, 244Pu, ...) and for new insights on stellar explosions (56/57Ni, 44Ti).