Present and Future of Gravitational Wave Astronomy

• Andere auteurs: Vajente, Gabriele (Redacteur)
• Formaat: Elektronisch Hoofdstuk
• Taal: Engels
• Gepubliceerd in: MDPI - Multidisciplinary Digital Publishing Institute 2022
• Onderwerpen: Research & information: general; Physics; 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
• Online toegang: DOAB: download the publication; DOAB: description of the publication

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...