We analyze a technique for suppressing laser frequency noise for the laser interferometer space antenna (LISA) gravitational wave detector. We demonstrate that the laser frequency can be stabilized to a LISA arm by high gain feedback. It is shown that the feedback bandwidth is not limited by the 33 second round-trip propagation time and example frequency controller designs are presented
The existence of gravitational waves is the most prominent of Einstein's predictions that has not ye...
The goal with LISA (Laser Interferometer Space Antenna) is to detect and study low-frequency astroph...
The requirement on laser frequency noise in the Laser Interferometer Space Antenna (LISA) depends on...
The Laser Interferometer Space Antenna (LISA) will be the first dedicated space based gravitational ...
Overcoming laser frequency noise is a significant technical challenge for achieving the design sensi...
We have investigated an ytterbium-doped distributed-feedback fiber master oscillator power amplifier...
This research focuses on laser ranging developments for LISA (Laser Interferometer Space Antenna), a...
For the Laser Interferometer Space Antenna (LISA) to reach its design sensitivity, the coupling of t...
The prime focus of LISA technology development efforts at NASA/GSFC has been in LISA interferometry,...
The laser interferometer space antenna will be the first space-based laser interferometric gravitati...
The laser frequency stabilization is one of the most important key technologies for the interferomet...
We present detailed numerical simulations of a laser phase stabilization scheme for LISA, where both...
Stabilization of laser frequency to interferometers with a large time delay in one arm is of signifi...
The Laser Interferometer Space Antenna (LISA) is a future space-based gravitational wave (GW) detect...
Low frequency high precision laser interferometry is subject to excess laser frequency noise couplin...
The existence of gravitational waves is the most prominent of Einstein's predictions that has not ye...
The goal with LISA (Laser Interferometer Space Antenna) is to detect and study low-frequency astroph...
The requirement on laser frequency noise in the Laser Interferometer Space Antenna (LISA) depends on...
The Laser Interferometer Space Antenna (LISA) will be the first dedicated space based gravitational ...
Overcoming laser frequency noise is a significant technical challenge for achieving the design sensi...
We have investigated an ytterbium-doped distributed-feedback fiber master oscillator power amplifier...
This research focuses on laser ranging developments for LISA (Laser Interferometer Space Antenna), a...
For the Laser Interferometer Space Antenna (LISA) to reach its design sensitivity, the coupling of t...
The prime focus of LISA technology development efforts at NASA/GSFC has been in LISA interferometry,...
The laser interferometer space antenna will be the first space-based laser interferometric gravitati...
The laser frequency stabilization is one of the most important key technologies for the interferomet...
We present detailed numerical simulations of a laser phase stabilization scheme for LISA, where both...
Stabilization of laser frequency to interferometers with a large time delay in one arm is of signifi...
The Laser Interferometer Space Antenna (LISA) is a future space-based gravitational wave (GW) detect...
Low frequency high precision laser interferometry is subject to excess laser frequency noise couplin...
The existence of gravitational waves is the most prominent of Einstein's predictions that has not ye...
The goal with LISA (Laser Interferometer Space Antenna) is to detect and study low-frequency astroph...
The requirement on laser frequency noise in the Laser Interferometer Space Antenna (LISA) depends on...