Proposes APTA with 6 satellites and 10^{-18} relative clock uncertainty at 1s averaging to achieve sensitivity for observing 10^3-10^4 solar-mass black hole mergers in the decihertz band.
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4 Pith papers cite this work. Polarity classification is still indexing.
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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.
Multiple viable sites on the Moon satisfy isolation, protection, accessibility, and line-of-sight constraints for both LILA-Pioneer and LILA-Horizon gravitational wave detectors.
The paper reviews cosmological tensions including the H0 and S8 discrepancies and explores new physics models that could explain them.
citing papers explorer
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Artificial Precision Timing Array: bridging the decihertz gravitational-wave sensitivity gap with clock satellites
Proposes APTA with 6 satellites and 10^{-18} relative clock uncertainty at 1s averaging to achieve sensitivity for observing 10^3-10^4 solar-mass black hole mergers in the decihertz band.
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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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Site selection constraints and options for LILA-Pioneer and LILA-Horizon
Multiple viable sites on the Moon satisfy isolation, protection, accessibility, and line-of-sight constraints for both LILA-Pioneer and LILA-Horizon gravitational wave detectors.
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Cosmology Intertwined: A Review of the Particle Physics, Astrophysics, and Cosmology Associated with the Cosmological Tensions and Anomalies
The paper reviews cosmological tensions including the H0 and S8 discrepancies and explores new physics models that could explain them.