Atomic Interferometric Gravitational-wave Space Observatory (AIGSO)
arXiv:1711.03690 · doi:10.1088/0253-6102/69/1/37
Abstract
We propose a space-borne gravitational-wave detection scheme, called atom interferometric gravitational-wave space observatory (AIGSO). It is motivated by the progress in the atomic matter-wave interferometry, which solely utilizes the standing light waves to split, deflect and recombine the atomic beam. Our scheme consists of three drag-free satellites orbiting the Earth. The phase shift of AIGSO is dominated by the Sagnac effect of gravitational-waves, which is proportional to the area enclosed by the atom interferometer, the frequency and amplitude of gravitational-waves. The scheme has a strain sensitivity in the 100 mHz-10 Hz frequency range, which fills in the detection gap between space-based and ground-based laser interferometric detectors. Thus, our proposed AIGSO can be a good complementary detection scheme to the space-borne laser interferometric schemes, such as LISA. Considering the current status of relevant technology readiness, we expect our AIGSO to be a promising candidate for the future space-based gravitational-wave detection plan.
9 pages, 3 figures
References in corpus (12)
- GW170817: Observation of Gravitational Waves from a Binary Neutron Star Inspiral
- GW170814: A Three-Detector Observation of Gravitational Waves from a Binary Black Hole Coalescence
- Atom Interferometers
- Precision Measurement of the Newtonian Gravitational Constant Using Cold Atoms
- New determination of the fine structure constant and test of the quantum electrodynamics
- Timing Measurements of the Relativistic Binary Pulsar PSR B1913+16
- An Atomic Gravitational Wave Interferometric Sensor (AGIS)
- Test of Equivalence Principle at Level by a Dual-species Double-diffraction Raman Atom Interferometer
- An Atomic Gravitational Wave Interferometric Sensor in Low Earth Orbit (AGIS-LEO)
- Is it possible to detect gravitational waves with atom interferometers?
- Gravitational-wave Detection With Matter-wave Interferometers Based On Standing Light Waves
- Population Boundaries for Galactic White Dwarf Binaries in LISA's Amplitude-Frequency Domain