LEADER 03712nam 22006495 450 001 9910300535903321 005 20200701050535.0 010 $a3-319-96014-8 024 7 $a10.1007/978-3-319-96014-2 035 $a(CKB)4100000005323171 035 $a(DE-He213)978-3-319-96014-2 035 $a(MiAaPQ)EBC5481460 035 $a(PPN)229503624 035 $a(EXLCZ)994100000005323171 100 $a20180728d2018 u| 0 101 0 $aeng 135 $aurnn|008mamaa 181 $ctxt$2rdacontent 182 $cc$2rdamedia 183 $acr$2rdacarrier 200 10$aControl of the Gravitational Wave Interferometric Detector Advanced Virgo /$fby Julia Casanueva Diaz 205 $a1st ed. 2018. 210 1$aCham :$cSpringer International Publishing :$cImprint: Springer,$d2018. 215 $a1 online resource (XVII, 202 p. 133 illus., 122 illus. in color.) 225 1 $aSpringer Theses, Recognizing Outstanding Ph.D. Research,$x2190-5053 311 $a3-319-96013-X 327 $aGravitational Waves -- Ground Based Gravitational Wave Detectors -- Advanced Virgo -- Fabry-Perot Cavities in Advanced Virgo -- Power Recycled Interferometer -- Advanced Virgo Commissioning -- Conclusion. 330 $aThis book focuses on the development and implementation of the longitudinal, angular and frequency controls of the Advanced Virgo detector, both from the simulation and experimental point of view, which contributed to Virgo reaching a sensitivity that enabled it to join the LIGO-Virgo O2 run in August 2017. This data taking was very successful, with the first direct detection of a binary black hole merger (GW170814) using the full network of three interferometers, and the first detection and localization of a binary neutron star merger (GW170817). The second generation of gravitational wave detector, Advanced Virgo, is capable of detecting differential displacements of the order of 10?21m. This means that it is highly sensitive to any disturbance, including the seismic movement of the Earth. For this reason an active control is necessary to keep the detector in place with sufficient accuracy. 410 0$aSpringer Theses, Recognizing Outstanding Ph.D. Research,$x2190-5053 606 $aAstronomy$vObservations 606 $aAstronomy?Observations 606 $aPhysical measurements 606 $aMeasurement 606 $aGravitation 606 $aLasers 606 $aPhotonics 606 $aAstronomy, Observations and Techniques$3https://scigraph.springernature.com/ontologies/product-market-codes/P22014 606 $aMeasurement Science and Instrumentation$3https://scigraph.springernature.com/ontologies/product-market-codes/P31040 606 $aClassical and Quantum Gravitation, Relativity Theory$3https://scigraph.springernature.com/ontologies/product-market-codes/P19070 606 $aOptics, Lasers, Photonics, Optical Devices$3https://scigraph.springernature.com/ontologies/product-market-codes/P31030 615 0$aAstronomy 615 0$aAstronomy?Observations. 615 0$aPhysical measurements. 615 0$aMeasurement. 615 0$aGravitation. 615 0$aLasers. 615 0$aPhotonics. 615 14$aAstronomy, Observations and Techniques. 615 24$aMeasurement Science and Instrumentation. 615 24$aClassical and Quantum Gravitation, Relativity Theory. 615 24$aOptics, Lasers, Photonics, Optical Devices. 676 $a520 700 $aCasanueva Diaz$b Julia$4aut$4http://id.loc.gov/vocabulary/relators/aut$0833966 906 $aBOOK 912 $a9910300535903321 996 $aControl of the Gravitational Wave Interferometric Detector Advanced Virgo$91864488 997 $aUNINA