Kavli Affiliate: Rana Adhikari | Summary:Improved low-frequency sensitivity of gravitational wave observatories would unlock study of intermediate-mass black hole mergers, binary black hole eccentricity, and provide early warnings for multi-messenger observations of binary neutron star mergers. Today’s mirror stabilization control injects harmful noise, constituting a major obstacle to sensitivity improvements. We eliminated this noise through […]
Continue.. Improving cosmological reach of a gravitational wave observatory using Deep Loop Shaping