期刊
QUANTUM SCIENCE AND TECHNOLOGY
卷 6, 期 4, 页码 -出版社
IOP Publishing Ltd
DOI: 10.1088/2058-9565/abf719
关键词
quantum sensor; atom interferometry; gravitational wave detection; ultralight dark matter
资金
- Gordon and Betty Moore Foundation [GBMF7945, GBMF7946]
- Fermi Research Alliance, LLC (FRA) [DE-AC02-07CH11359]
- US Department of Energy, Office of Science, QuantiSED Initiative
- UKRI's Science and Technologies Facilities Council (STFC)
- Engineering and Physical Sciences Research Council (EPSRC)
- Laboratory Directed Research and Development program at SLAC National Accelerator Laboratory [DE-AC02-76SF00515]
- Kavli Foundation
- Department of Defense (DoD)
- NSF Quantum Information Science and Engineering Network (QISE-NET) Graduate Fellowship - NSF [DMR-1747426]
- Universities Research Alliance (URA)
- Royal Society, UK
- Office of Naval Research [N00014-19-1-2181]
- National Institute of Standards and Technology [60NANB19D168]
- Office for Research and Innovation
- University President's Office
- Science and Technology Facilities Council [ST/S000879/1] Funding Source: researchfish
MAGIS-100 is a next-generation quantum sensor being constructed at Fermilab, aiming to explore fundamental physics through atom interferometry over a 100 m baseline. This novel detector will search for ultralight dark matter, test quantum mechanics in new regimes, and pave the way for future gravitational wave detectors.
MAGIS-100 is a next-generation quantum sensor under construction at Fermilab that aims to explore fundamental physics with atom interferometry over a 100 m baseline. This novel detector will search for ultralight dark matter, test quantum mechanics in new regimes, and serve as a technology pathfinder for future gravitational wave detectors in a previously unexplored frequency band. It combines techniques demonstrated in state-of-the-art 10-meter-scale atom interferometers with the latest technological advances of the world's best atomic clocks. MAGIS-100 will provide a development platform for a future kilometer-scale detector that would be sufficiently sensitive to detect gravitational waves from known sources. Here we present the science case for the MAGIS concept, review the operating principles of the detector, describe the instrument design, and study the detector systematics.
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