Arm locking is one of the key technologies to suppress the laser phase noise in spaced-based gravitational waves observatories. Since arm locking was proposed, phase margin criterion was always used as the fundamental design strategy for the controller development. In this paper, we find that this empirical method from engineering actually cannot guarantee the arm locking stability. Therefore, most of the advanced arm locking controllers reported so far may have instable problems. After comprehensive analysis of the single arm locking's transient responses, strict analytical stability criterions are summarized for the first time. These criterions are then generalized to dual arm locking, modified-dual arm locking and common arm locking, and...
Long baseline laser interferometers used for gravitational wave detection have proven to be very com...
We analyze a technique for suppressing laser frequency noise for the laser interferometer space ante...
Residual motion of the arm cavity mirrors is expected to prove one of the principal impediments to ...
For space gravitational wave (GW) detection, arm locking is a proposal useful in decreasing the freq...
The laser frequency stabilization is one of the most important key technologies for the interferomet...
The Laser Interferometer Space Antenna (LISA) is a future space-based gravitational wave (GW) detect...
The Laser Interferometer Space Antenna (LISA) will be the first dedicated space based gravitational ...
Modern ground-based gravitational wave (GW) detectors require a complex interferometer configuration...
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...
We present the first experimental confirmation of the so-called 'self-phase-locked delay interferome...
Abstract. LISA relies on several techniques to reduce the initial laser frequency noise in order to ...
We present detailed numerical simulations of a laser phase stabilization scheme for LISA, where both...
Residual motion of the arm cavity mirrors is expected to prove one of the principal impediments to s...
Long-baseline laser interferometers used for gravitational-wave detection have proven to be very com...
Long baseline laser interferometers used for gravitational wave detection have proven to be very com...
We analyze a technique for suppressing laser frequency noise for the laser interferometer space ante...
Residual motion of the arm cavity mirrors is expected to prove one of the principal impediments to ...
For space gravitational wave (GW) detection, arm locking is a proposal useful in decreasing the freq...
The laser frequency stabilization is one of the most important key technologies for the interferomet...
The Laser Interferometer Space Antenna (LISA) is a future space-based gravitational wave (GW) detect...
The Laser Interferometer Space Antenna (LISA) will be the first dedicated space based gravitational ...
Modern ground-based gravitational wave (GW) detectors require a complex interferometer configuration...
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...
We present the first experimental confirmation of the so-called 'self-phase-locked delay interferome...
Abstract. LISA relies on several techniques to reduce the initial laser frequency noise in order to ...
We present detailed numerical simulations of a laser phase stabilization scheme for LISA, where both...
Residual motion of the arm cavity mirrors is expected to prove one of the principal impediments to s...
Long-baseline laser interferometers used for gravitational-wave detection have proven to be very com...
Long baseline laser interferometers used for gravitational wave detection have proven to be very com...
We analyze a technique for suppressing laser frequency noise for the laser interferometer space ante...
Residual motion of the arm cavity mirrors is expected to prove one of the principal impediments to ...