LIGO Document G1602321-x0
- On September 14, 2015, subtle ripples in the fabric of space-time were detected by the twin LIGO interferometers, heralding the opening of the first observational run (O1) with second generation interferometers and gravitational-wave astronomy itself. By the close of that run, two additional significant events had been collected along with a wealth of scientific return. With observing scheduled to continue through the end of the year, the LIGO and Virgo interferometers are poised to directly measure the properties of a population of binary black holes and their mergers, advancing inquiries into astrophysics and strong-field general relativity which would have been otherwise inaccessible. In this talk, I will highlight many of the important results of the first observing run in the context of current astrophysics as well as explore their implications for models of binary evolution and environments, and finally delve into some of the possibilities for future runs.
DCC Version 3.4.1, contact
Document Database Administrators