The goal of this 3-day workshop is to launch the data interpretation phase of the RPA with selected experts in observational, theoretical and experimental r-process work.

The meeting will bring together experts from various fields to discuss the role played by lithium in several astrophysical contexts and to highlight the extraordinary character of this chemical species, as a tracer of the structure and evolution of stars, galaxies and the Universe.

The main topics of the meeting will be:

 * Big Bang nucleosynthesis

 * Nuclear reaction rates involving lithium and beryllium

 * Physical processes in stellar interiors as traced by Li, Be, and B

 * Hot bottom burning in massive AGB stars

Alexander Ji. Carnegie Science Observatories

The lanthanide fraction distribution in r-process metal-poor stars

Abstract:

Join the MSU Science Communication organization (MSU SciComm) with the Facility for Rare Isotope Beams (FRIB) in their first live Science-Art show. There will be live science demos and discussions. This event features guest speaker Patrick Morgan, and Keynote Speaker Dianna Cowern aka Physics Girl. 

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Topics

Beyond iron, a small fraction of the total abundances in the Solar System is made of proton-rich isotopes, the p-nuclei. The clear understanding of their production is a fundamental challenge for nuclear astrophysics but still remains to be clarified.

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.

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.

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.

Currently enrolled high school students participate in a week-long nuclear astrophysics "boot camp" filled with lectures, experiments, and social activities.

Session 2 of the 2019 Art 2 Science Camp for children ages 8-12.

Session Website

Middle and high school physical science teachers from the US and Canada participate in a week-long professional development program to learn techniques for teaching nuclear astrophysics in the classroom. Activities are similar to the student week, but also include lesson plans and materials.

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.).

Session 1 of the 2019 Art 2 Science Camp for children ages 8-12.

Session Website

This workshop will bring together theorists and experimentalists to address the many aspects of nuclear physics and astrophysics that must be considered and properly understood in order to model the r-process

The registration will be open from April 15th. For US participants, there is an opportunity to obtain travel support to ECT* workshops through the EUSTIPEN program.

Currently enrolled high school students participate in a week-long nuclear astrophysics "boot camp" filled with lectures, experiments, and social activities.

We provide training in nuclear detection for this veteran bridge program

An informal meeting to discuss weak interactions in hot and dense matter encountered in supernovae and neutron star mergers will be held at the Institute for Nuclear Theory June 3-6, 2019.

This is the ninth in a series of former JINA and now JINA-CEE meetings that brings together JINA-CEE participants, collaborators, and other interested researchers in nuclear physics, astronomy, and astrophysics to discuss progress and future directions related to the understanding of the origin of the elements and neutron stars.