Mid-Frequency Gravitational Wave Detection and Sources
arXiv:2004.05590 · doi:10.1142/S021827181902005X
Abstract
A brief history and various themes of mid-frequency gravitational wave detection are presented more or less following historical order -- Laser Interferometry, Atom Interferometry (AI), Torsion Bar Antenna (TOBA), and Superconducting Omni-directional Gravitational Radiation Observatory (SOGRO). Both Earth-based and Space-borne concepts are reviewed with outlook on expected astrophysical sources
reference update and minor corrections
References in corpus (50)
- Observation of Gravitational Waves from a Binary Black Hole Merger
- GW170817: Observation of Gravitational Waves from a Binary Neutron Star Inspiral
- GW151226: Observation of Gravitational Waves from a 22-Solar-Mass Binary Black Hole Coalescence
- GW170104: Observation of a 50-Solar-Mass Binary Black Hole Coalescence at Redshift 0.2
- Measurement of the fine-structure constant as a test of the Standard Model
- Precision Measurement of the Newtonian Gravitational Constant Using Cold Atoms
- Beyond LISA: Exploring Future Gravitational Wave Missions
- New determination of the fine structure constant and test of the quantum electrodynamics
- Multi-axis inertial sensing with long-time point source atom interferometry
- Gravitational wave detection with optical lattice atomic clocks
- 6-axis inertial sensor using cold-atom interferometry
- AEDGE: Atomic Experiment for Dark Matter and Gravity Exploration in Space
- An Atomic Gravitational Wave Interferometric Sensor (AGIS)
- Exploring gravity with the MIGA large scale atom interferometer
- Observational evidence for intermediate-mass black holes
- Determination of the Newtonian Gravitational Constant Using Atom Interferometry
- Phase shift in atom interferometry due to spacetime curvature
- Testing Gravity with Cold-Atom Interferometers
- Seismic gravity-gradient noise in interferometric gravitational-wave detectors
- ZAIGA: Zhaoshan Long-baseline Atom Interferometer Gravitation Antenna
- An Atomic Gravitational Wave Interferometric Sensor in Low Earth Orbit (AGIS-LEO)
- Precision atomic gravimeter based on Bragg diffraction
- Cold atom gravimetry with a Bose-Einstein Condensate
- Atom interferometry gravity-gradiometer for the determination of the Newtonian gravitational constant G
- A spaceborne gravity gradiometer concept based on cold atom interferometers for measuring Earth's gravity field
- ASTROD-GW: Overview and Progress
- Low-Frequency Terrestrial Gravitational-Wave Detectors
- Terrestrial Gravity Fluctuations
- Astrophysics and cosmology with a decihertz gravitational-wave detector: TianGO
- Human Gravity-Gradient Noise in Interferometric Gravitational-Wave Detectors
- Is it possible to detect gravitational waves with atom interferometers?
- The astrophysical science case for a decihertz gravitational-wave detector
- Impact of infrasound atmospheric noise on gravity detectors used for astrophysical and geophysical applications
- Gravitational wave detectors based on matter wave interferometers (MIGO) are no better than laser interferometers (LIGO)
- Towards MIGO, the Matter-wave Interferometric Gravitational-wave Observatory, and the Intersection of Quantum Mechanics with General Relativity
- State of the art in the determination of the fine structure constant: test of Quantum Electrodynamics and determination of h/mu
- Upper Limit on Gravitational Wave Backgrounds at 0.2 Hz with Torsion-bar Antenna
- Newtonian-noise cancellation in full-tensor gravitational-wave detectors
- A comparison between matter wave and light wave interferometers for the detection of gravitational waves
- Characterizing Earth gravity field fluctuations with the MIGA antenna for future Gravitational Wave detectors
- Optical frequency standards for gravitational wave detection using satellite Doppler velocimetry
- Atomic Interferometric Gravitational-wave Space Observatory (AIGSO)
- Sensitivity of a small matter-wave interferometer to gravitational waves
- Matter-wave laser Interferometric Gravitation Antenna (MIGA): New perspectives for fundamental physics and geosciences
- Gravitational Wave (GW) Classification, Space GW Detection Sensitivities and AMIGO (Astrodynamical Middle-frequency Interferometric GW Observatory)
- Gravitational-wave Detection With Matter-wave Interferometers Based On Standing Light Waves
- Using Atomic Clocks to Detect Gravitational Waves
- Ground Based Low-Frequency Gravitational-wave Detector With Multiple Outputs
- Seismic Cross-coupling Noise in Torsion Pendulums
- Chang'e 3 lunar mission and upper limit on stochastic background of gravitational wave around the 0.01 Hz band