Simulations project that the Lunar Gravitational Wave Antenna could detect roughly 30 Galactic monochromatic double white dwarf sources and 10 extragalactic mergers in 10 years using population synthesis and Fisher matrix methods.
P., Abbott, R., Abbott, T
2 Pith papers cite this work. Polarity classification is still indexing.
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Multiple independent late-universe measurements of the Hubble constant show 4-5.8 sigma tension with early-universe predictions.
citing papers explorer
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Observing Double White Dwarfs with the Lunar GW Antenna
Simulations project that the Lunar Gravitational Wave Antenna could detect roughly 30 Galactic monochromatic double white dwarf sources and 10 extragalactic mergers in 10 years using population synthesis and Fisher matrix methods.
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Tensions between the Early and the Late Universe
Multiple independent late-universe measurements of the Hubble constant show 4-5.8 sigma tension with early-universe predictions.