Large-scale gravitational wave detectors are expected to be operational in the first decade of the 21st century, enabling detection of galactic sources and black hole mergers.

Detection of gravitational waves

This study presents novel methods to detect and measure the polarization of continuous gravitational waves, providing new model-independent constraints on deviations from general relativity.

Probing dynamical gravity with the polarization of continuous gravitational waves

Optical frequency modulation can potentially detect high-frequency gravitational waves, with promising sensitivities across a broad frequency range.

High-frequency gravitational wave detection via optical frequency modulation

Large-scale gravitational wave detectors are expected to be operational in the first decade of the 21st century, enabling the detection of galactic sources and black hole mergers.

Gravitational wave science is poised for a breakthrough in the coming decade, with 2nd-generation LIGO and Virgo interferometers likely to detect the first signals.

Gravitational Waves: Sources, Detectors and Searches

Gravitational wave detectors are expected to achieve secure detections by 2014, offering insights into physics, astrophysics, and cosmology.

Physics, Astrophysics and Cosmology with Gravitational Waves

Deep auto-encoder models using Apache Spark offer competitive accuracy and scalability in detecting gravitational waves from time series data, offering a valuable machine learning tool for astrophysical analysis.

Scalable auto-encoders for gravitational waves detection from time series data

Gravitational waves detection, using Michelson interferometers, offers a new horizon for astronomers to explore the universe and carry more information about black holes and the Big Bang than electromagnetic waves.

The Detection Scheme and Applications of Gravitational Waves

This tunable resonant sensor can detect gravitational waves in the frequency range of 50-300 kHz, extending the search volume for sources by 1 to 3 orders of magnitude.

Detecting high-frequency gravitational waves with optically levitated sensors.

Gravitational-wave astronomy has a bright future, with potential for increased bandwidth and sensitivity, and a brighter understanding of cataclysmic events in the universe.

Gravitational-wave physics and astronomy in the 2020s and 2030s

Gravitational waves may be detected within the next decade using test masses suspended as pendulums and laser interferometry, offering high sensitivities over a wide range of frequencies.

THE DETECTION OF GRAVITATIONAL WAVES

The new instrument designed by researchers can detect gravitational waves at distances 5 times further away than Advanced LIGO, potentially revolutionizing our understanding of the universe.

A cryogenic silicon interferometer for gravitational-wave detection

Gravitational wave detection technology has successfully detected black hole mergers, providing clues for studying the universe's mysteries and potential communication applications.

Application of gravitational wave detection technology in astronomical observations

Gravitational-wave astronomy offers a new era of scientific exploration, potentially reshaping our understanding of the cosmos and the laws of Nature.

Black holes, gravitational waves and fundamental physics: a roadmap

Gravitational waves from early universe phase transitions, such as bubble collisions and inverse-cascade helical magnetohydrodynamic turbulence, may be detectable today using the Laser Interferometer Space Antenna.

Detectability of gravitational waves from phase transitions

Gravitational waves can test gravity and dark energy models, providing a new tool to probe the nature of dark energy and fundamental properties of gravity.

Dark Energy in Light of Multi-Messenger Gravitational-Wave Astronomy

New generation of laser interferometers are expected to revolutionize gravitational-wave detection, leading to precision science using gravitational radiation in the coming decades.

Gravitational Radiation Detection with Laser Interferometry

Gravitational waves can test gravity theories by detecting the gradual activation of dipole radiation due to massive fields, providing new constraints on coupling parameters for masses less than 6 x 10-14 eV.

Testing massive-field modifications of gravity via gravitational waves

The next generation of gravitational wave detectors should be able to observe compact binary sources with high signal-to-noise ratio, maximizing the scientific potential of gravitational-wave astronomy.

Exploring the Sensitivity of Next Generation Gravitational Wave Detectors

The future detection of gravitational waves can test theories of gravity in a model-independent way, providing valuable constraints on model parameters in effective field theories.

Generalized framework for testing gravity with gravitational-wave propagation. III. Future prospect

How do we understand and detect gravitational waves?

These studies suggest that understanding and detecting gravitational waves involve using large-scale detectors, novel measurement methods, optical frequency modulation, machine learning tools, and tunable resonant sensors, with significant advancements expected from 2nd-generation interferometers like LIGO and Virgo.