Outflow from Post-Black Hole-Neutron Star Merger Disks [Poster]
Histograms of mass of a given ratio of electron to baryon number in winds from a post-merger disk for four disks of different masses. This ratio determines how many elements heavier than iron, if any, are produced by a black hole-neutron star merger event. Analysis performed by PhD student Sanjana Curtis (NCSU, now graduated) on Capulin in collaboration with her advisor, Carla Frohlich, and LANL staff Jonah Miller.