On the laser frequency stabilization by locking to a LISA arm
| dc.creator | Tinto, Massimo | |
| dc.creator | Rakhmanov, Malik | |
| dc.date | 2004-08-21 | |
| dc.date.accessioned | 2026-07-07T03:28:56Z | |
| dc.date.available | 2026-07-07T03:28:56Z | |
| dc.description | LISA is an array of three spacecraft flying in an approximately equilateral triangle configuration, which will be used as a low-frequency detector of gravitational waves. Recently a technique has been proposed for suppressing the phase noise of the onboard lasers by locking them to the LISA arms. In this paper we show that the delay-induced effects substantially modify the performance of this technique, making it different from the conventional locking of lasers to optical resonators. We analyze these delay-induced effects in both transient and steady-state regimes and discuss their implications for the implementation of this technique on LISA. | |
| dc.description | 3 pages, 1 figure | |
| dc.identifier | https://arxiv.org/abs/gr-qc/0408076 | |
| dc.identifier | http://arxiv.org/abs/gr-qc/0408076 | |
| dc.identifier.uri | http://salesiana.dossiersoluciones.com/handle/123456789/35023 | |
| dc.subject | General Relativity and Quantum Cosmology | |
| dc.title | On the laser frequency stabilization by locking to a LISA arm | |
| dc.type | text |