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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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Gardado en:
Formato: Online
Idioma:inglés
Publicado: 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
Acceso en liña:ONIX_20221025_9783036552255_24
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