The South Pole's low seismic noise, existing infrastructure, and geographic position make it a strong candidate site for a long-baseline atom interferometer to detect decihertz gravitational waves and strengthen global triangulation.
Model binary black hole source parameters used chirp mass of 25M ⊙, luminosity distance 100 Mpc, binary inclination angle of π/4 and polarization angleπ/3
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Opportunities for Gravitational Wave Physics at the South Pole
The South Pole's low seismic noise, existing infrastructure, and geographic position make it a strong candidate site for a long-baseline atom interferometer to detect decihertz gravitational waves and strengthen global triangulation.