Wei Jia Ong
Lawrence Livermore National Laboratory
(i) r-process production in GR simulations of the double
neutron stars and CCSNe; the impact of neutrinos.
(ii) The assembly of double neutron stars and r-process
enrichment of the Galaxy and its satellites.
(iii) GW170827; kilonova emission from theoretical perspective.
(iv) GW170817; Modeling and observations of the associated kilonova.
(v) r-process production from the experimental nuclear physics perspective.
(vi) Observations of the r-process enhanced metal poor stars.
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.
Nuclear and astrophysics aspects for the rapid neutron capture process in the era of multimessenger observations (Opens in a new window)
The registration will open form April 15th. For US participants, there is an opportunity to obtain travel support to ECT* workshops through the EUSTIPEN program.
Instructions are available here: http://fribtheoryalliance.org/content/eustipen.php