Shining Light on the Physics of Neutron Star Mergers

In August 2017, the LIGO/Virgo observatory detected gravitational waves for the first time from the merger of two neutron stars. This cataclysmic event was followed (within seconds) by a burst of gamma-rays and (within 11 hours) by a bright but rapidly fading thermal optical/IR glow. The properties of the thermal emission matched remarkably well existing predictions for radiation powered by the radioactive decay of heavy nuclei, which were synthesized in the expanding neutron-rich merger debris via the rapid neutron capture process.  I will describe ongoing efforts to interpret this event from both the electromagnetic and gravitational wave sides, and the resulting implications for the origin of the heaviest elements in the universe and the equation of state of nuclear density matter.  I will place these results in the context of discoveries made during LIGO/Virgo's recently concluded O3 run and, time permitting, preview the diversity in electromagnetic counterpart properties we could expect from future merger events.