Lessons from the light of a neutron star merger

摘要

The discovery by Advanced LIGO/Virgo of gravitational waves from the binary neutron star merger GW170817, and subsequently by astronomers of transient emission across the electromagnetic spectrum, has initiated a new era of multi-messenger gravitational wave astronomy. Here I summarize the electromagnetic discoveries in the context of theoretical counterpart models and present personal views on the major take-away lessons and outstanding new questions from this watershed event, focused on the implications for nuclear physics. The luminosity and colors of the early optical emission discovered within a day of the merger agree well with predictions for "kilonova" emission, powered by the radioactive decay of light r-process nuclei (atomic mass number A less than or similar to 140). The transition of the spectral energy distribution to near-infrared wavelengths on timescales of days indicates that inner portions of the ejecta contain heavy r-process nuclei with high UV/optical opacity due to the presence of at least some lanthanide elements (A greater than or similar to 140). The "blue" and "red" ejecta components likely possess distinct origins (e.g. dynamical ejecta, magnetar-powered wind, or accretion disk outflow), with implications for the merger process (e.g. the lifetime of the remnant prior to black hole formation) and fundamental properties of neutron stars. I outline the predicted diversity in the electromagnetic emission of future mergers-observed with different ingoing binary masses and/or viewing angles-discovered in the years ahead as LIGO/Virgo reach design sensitivity. (C) 2019 Elsevier Inc. All rights reserved.