DC readout experiment in Enhanced LIGO

Tobin T. Fricke*, Nicolás D. Smith-Lefebvre, Richard Abbott, Rana Adhikari, Katherine L. Dooley, Matthew Evans, Peter Fritschel, Valery V. Frolov, Keita Kawabe, Jeffrey S. Kissel, Bram J.J. Slagmolen, Sam J. Waldman

*Corresponding author for this work

    Research output: Contribution to journalArticlepeer-review

    98 Citations (Scopus)

    Abstract

    The two 4 km long gravitational wave detectors operated by the Laser Interferometer Gravitational-wave Observatory (LIGO) were modified in 2008 to read out the gravitational wave channel using the DC readout form of homodyne detection and to include an optical filter cavity at the output of the detector. As part of the upgrade to Enhanced LIGO, these modifications replaced the radio-frequency (RF) heterodyne system used previously. We describe the motivations for and the implementation of DC readout and the output mode cleaner in Enhanced LIGO. We present characterizations of the system, including measurements and models of the couplings of the noises from the laser source to the gravitational wave readout channel. We show that noise couplings using DC readout are improved over those for RF readout, and we find that the achieved shot-noise-limited sensitivity is consistent with modeled results.

    Original languageEnglish
    Article number065005
    JournalClassical and Quantum Gravity
    Volume29
    Issue number6
    DOIs
    Publication statusPublished - 21 Mar 2012

    Fingerprint

    Dive into the research topics of 'DC readout experiment in Enhanced LIGO'. Together they form a unique fingerprint.

    Cite this