Abstract. LISA relies on several techniques to reduce the initial laser frequency noise in order to achieve an interferometric length measurement with an accuracy of ≈ 10 pm/√Hz. LISA will use ultra-stable reference cavities as a first step to reduce the laser frequency noise. In a second step the frequency will be stabilized to the LISA arms which provide a better reference in the frequency band of interest. We present experimental results demonstrating Arm locking with LISA-like light travel times and Doppler shifts. We also integrated this system with a LISA-like pre-stabilization system using our ultra-stable cavities. The addition of realistic Doppler shifts led to further refinements of the arm locking controllers compared to the cont...
In order to attain the requisite sensitivity for LISA (Laser Interferometric Space Antenna)-a joint ...
Abstract. Recent advances at JPL in experimentation and design for LISA interferometry include the d...
Low frequency high precision laser interferometry is subject to excess laser frequency noise couplin...
For the Laser Interferometer Space Antenna (LISA) to reach its design sensitivity, the coupling of t...
Overcoming laser frequency noise is a significant technical challenge for achieving the design sensi...
The Laser Interferometer Space Antenna (LISA) will be the first dedicated space based gravitational ...
The Laser Interferometer Space Antenna (LISA) is a future space-based gravitational wave (GW) detect...
We present the first experimental confirmation of the so-called 'self-phase-locked delay interferome...
We present detailed numerical simulations of a laser phase stabilization scheme for LISA, where both...
We analyze a technique for suppressing laser frequency noise for the laser interferometer space ante...
A phase-locking configuration for LISA is proposed that provides a significantly simpler mode of ope...
At the University of Florida, we are developing an experimental Laser Interferometer Space Antenna (...
We discuss the baseline optical configuration for the Laser Interferometer Space Antenna (LISA) miss...
Recent advances at JPL in experimentation and design for LISA interferometry include the demonstrati...
The prime focus of LISA technology development efforts at NASA/GSFC has been in LISA interferometry,...
In order to attain the requisite sensitivity for LISA (Laser Interferometric Space Antenna)-a joint ...
Abstract. Recent advances at JPL in experimentation and design for LISA interferometry include the d...
Low frequency high precision laser interferometry is subject to excess laser frequency noise couplin...
For the Laser Interferometer Space Antenna (LISA) to reach its design sensitivity, the coupling of t...
Overcoming laser frequency noise is a significant technical challenge for achieving the design sensi...
The Laser Interferometer Space Antenna (LISA) will be the first dedicated space based gravitational ...
The Laser Interferometer Space Antenna (LISA) is a future space-based gravitational wave (GW) detect...
We present the first experimental confirmation of the so-called 'self-phase-locked delay interferome...
We present detailed numerical simulations of a laser phase stabilization scheme for LISA, where both...
We analyze a technique for suppressing laser frequency noise for the laser interferometer space ante...
A phase-locking configuration for LISA is proposed that provides a significantly simpler mode of ope...
At the University of Florida, we are developing an experimental Laser Interferometer Space Antenna (...
We discuss the baseline optical configuration for the Laser Interferometer Space Antenna (LISA) miss...
Recent advances at JPL in experimentation and design for LISA interferometry include the demonstrati...
The prime focus of LISA technology development efforts at NASA/GSFC has been in LISA interferometry,...
In order to attain the requisite sensitivity for LISA (Laser Interferometric Space Antenna)-a joint ...
Abstract. Recent advances at JPL in experimentation and design for LISA interferometry include the d...
Low frequency high precision laser interferometry is subject to excess laser frequency noise couplin...