Present and Future of Gravitational Wave Astronomy

The first detection on Earth of a gravitational wave signal from the coalescence of a binary black hole system in 2015 established a new era in astronomy, allowing the scientific community to observe the Universe with a new form of radiation for the first time. More than five years later, many more...

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Bibliographic Details
Format:	Online
Language:	English
Published:	MDPI - Multidisciplinary Digital Publishing Institute 2022
Subjects:	LIGO Virgo KAGRA gravitational waves detector characterization data quality noise mitigation seismic noise Newtonian noise seismic isolation system noise subtraction DECIGO thermal noise quantum noise diffraction loss interferometers ground based gravitational-wave detector Advanced Virgo gravitational-wave backgrounds stochastic gravitational-wave backgrounds stochastic searches of gravitational waves gravitational-wave laser interferometers pulsar timing arrays gravitational wave detectors optomechanics low-noise high-power laser interferometry calibration interferometer gravitational wave astrophysics laser metrology squeezed states quantum optics gravitational wave detector laser interferometer cryogenics underground einstein telescope newtonian noise coating noise silicon suspensions payload cryostat core-collapse supernova future detectors continuous gravitational waves neutron stars dark matter gravitational-wave astrophysics stars black holes stellar evolution binary stars stellar dynamics laser interferometers n/a thema EDItEUR::G Reference, Information and Interdisciplinary subjects::GP Research and information: general thema EDItEUR::P Mathematics and Science::PH Physics
Online Access:	ONIX_20221025_9783036552255_24
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Present and Future of Gravitational Wave Astronomy

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