Present and Future of Gravitational Wave Astronomy

• Autore: Vajente Gabriele
• Pubblicazione: MDPI - Multidisciplinary Digital Publishing Institute, 2022
• Descrizione fisica: 1 online resource (428 p.)
• Soggetto topico: Physics; Research & information: general
• Soggetto non controllato: Advanced Virgo; astrophysics; binary stars; black holes; calibration; coating noise; continuous gravitational waves; core-collapse supernova; cryogenics; cryostat; dark matter; data quality; DECIGO; detector characterization; diffraction loss; einstein telescope; future detectors; gravitational wave; gravitational wave detector; gravitational wave detectors; gravitational waves; gravitational-wave astrophysics; gravitational-wave backgrounds; gravitational-wave laser interferometers; ground based gravitational-wave detector; interferometer; interferometers; KAGRA; laser interferometer; laser interferometers; laser metrology; LIGO; low-noise high-power laser interferometry; n/a; neutron stars; newtonian noise; Newtonian noise; noise mitigation; noise subtraction; optomechanics; payload; pulsar timing arrays; quantum noise; quantum optics; seismic isolation system; seismic noise; silicon; squeezed states; stars; stellar dynamics; stellar evolution; stochastic gravitational-wave backgrounds; stochastic searches of gravitational waves; suspensions; thermal noise; underground; Virgo
• Persona (resp. second.): VajenteGabriele
• Sommario/riassunto: 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 gravitational wave signals have been detected, including the first binary neutron star coalescence in coincidence with a gamma ray burst and a kilonova observation. The field of gravitational wave astronomy is rapidly evolving, making it difficult to keep up with the pace of new detector designs, discoveries, and astrophysical results. This Special Issue is, therefore, intended as a review of the current status and future directions of the field from the perspective of detector technology, data analysis, and the astrophysical implications of these discoveries. Rather than presenting new results, the articles collected in this issue will serve as a reference and an introduction to the field. This Special Issue will include reviews of the basic properties of gravitational wave signals; the detectors that are currently operating and the main sources of noise that limit their sensitivity; planned upgrades of the detectors in the short and long term; spaceborne detectors; a data analysis of the gravitational wave detector output focusing on the main classes of detected and expected signals; and implications of the current and future discoveries on our understanding of astrophysics and cosmology.
• Titolo autorizzato: Present and Future of Gravitational Wave Astronomy
• ISBN: 3-0365-5226-X
• Formato: Materiale a stampa
• Livello bibliografico: Monografia
• Lingua di pubblicazione: Inglese
• Record Nr.: 9910619468803321
• Lo trovi qui: Univ. Federico II