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DOE OSTI · 1870607

Outflow from Post-Black Hole-Neutron Star Merger Disks [Poster]

Curtis, Sanjana·Miller, Jonah Maxwell
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Abstract

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.

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BibTeXRIS

Curtis, Sanjana, Miller, Jonah Maxwell. 2022-05-25. Outflow from Post-Black Hole-Neutron Star Merger Disks [Poster]. https://doi.org/10.2172/1870607

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