ZAIGA: Zhaoshan long-baseline atom interferometer gravitation antenna
By M. Zhan, Jin Wang, W. Ni, D. Gao, Gang Wang, Lingxiang He, Runbing Li, Lin Zhou, Xiangshan Chen, Jiaqi Zhong and 14 more. International Journal of Modern Physics D, 2019
139 citations recorded by the source corpus.
The Zhaoshan long-baseline Atom Interferometer Gravitation Antenna (ZAIGA) is a new type of underground laser-linked interferometer facility, and is currently under construction. It is in the 200-m-on-average underground of a mountain named Zhaoshan which is about 80[Formula: see text]km southeast to Wuhan. ZAIGA will be equipped with long-baseline atom interferometers, high-precision atom clocks, and large-scale gyros. ZAIGA facility will take an equilateral triangle configuration with two 1-km-apart atom interferometers in each arm, a 300-m vertical tunnel with atom fountain and atom clocks mounted, and a tracking-and-ranging 1-km-arm-length prototype with lattice optical clocks linked by locked lasers. The ZAIGA facility will be used for experimental research on gravitation and related problems including gravitational wave detection, high-precision test of the equivalence principle of micro-particles, clock-based gravitational red-shift measurement, rotation measurement and gravitomagnetic effect.
Subfields: Atomic and Molecular Physics, and Optics
View Paper: https://www.semanticscholar.org/paper/0179e1a7abe6944f1095bda56ba3e8d1b08200fe
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Citations in the corpus
- AION: an atom interferometer observatory and network (2019, methodology): “ould observe early inspiral stages of mergers, providing 2We also envisage networking with atom interferometer experiments in Europe, including MIGA [15] and ELGAR [16], and in China, including ZAIGA [17]. { 16 { good angular localization precisions [69] and predictions for the time of the merger th”
- Solar-mass primordial black holes explain NANOGrav hint of gravitational waves (2020, unknown): “We do not show the MPBH 5Though not shown in the figure, see also the following references for related experiments: ALIA [121], ELGAR [122], MAGIS [123, 124], MIGA [125], Taiji [126], and ZAIGA [127]. dependence in the figure, but the spectra shift to the left as MPBH increases.”
- Matter-wave Atomic Gradiometer Interferometric Sensor (MAGIS-100) (2021, unknown): “MAGIS-100 100 1 Vertical Sr Clock AI, Bragg USA AION [10] 100 1 Vertical Sr Clock AI UK MIGA [5] 200 2 Horizontal Rb Bragg France ZAIGA [8] 300 3 Vertical Rb, Sr Raman, Bragg, OLC China”