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Advanced LIGO

2015· article· en· 3 389 citations· W4234856688 sur OpenAlex· 10.1088/0264-9381/32/7/074001

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Résumé

The Advanced LIGO gravitational wave detectors are second-generation instruments designed and built for the two LIGO observatories in Hanford, WA and Livingston, LA, USA. The two instruments are identical in design, and are specialized versions of a Michelson interferometer with 4 km long arms. As in Initial LIGO, Fabry–Perot cavities are used in the arms to increase the interaction time with a gravitational wave, and power recycling is used to increase the effective laser power. Signal recycling has been added in Advanced LIGO to improve the frequency response. In the most sensitive frequency region around 100 Hz, the design strain sensitivity is a factor of 10 better than Initial LIGO. In addition, the low frequency end of the sensitivity band is moved from 40 Hz down to 10 Hz. All interferometer components have been replaced with improved technologies to achieve this sensitivity gain. Much better seismic isolation and test mass suspensions are responsible for the gains at lower frequencies. Higher laser power, larger test masses and improved mirror coatings lead to the improved sensitivity at mid and high frequencies. Data collecting runs with these new instruments are planned to begin in mid-2015.

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La notice

Revue
Classical and Quantum Gravity
Thématique
Pulsars and Gravitational Waves Research
Domaine
Physics and Astronomy
Établissements canadiens
Canadian Institute for Theoretical AstrophysicsUniversity of Toronto
Organismes subventionnaires
Govern de les Illes BalearsIstituto Nazionale di Fisica NucleareMinistero dello Sviluppo EconomicoNational Research Foundation of KoreaLeverhulme TrustHungarian Scientific Research FundIndustry CanadaNational Aeronautics and Space AdministrationScottish Funding CouncilScottish Universities Physics AllianceCouncil of Scientific and Industrial Research, IndiaScience and Technology Facilities CouncilNational Research FoundationAlfred P. Sloan FoundationMinisterio de Economía y CompetitividadNational Science Foundation
Mots-clés
LIGOPhysicsInterferometryGravitational waveSensitivity (control systems)Michelson interferometerOpticsGravitational-wave observatoryLaserDetectorFrequency bandAstrophysicsElectronic engineeringTelecommunicationsComputer scienceBandwidth (computing)Engineering
Résumé présent dans OpenAlex
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