Super-Eddington accretion boosts predicted LISA detections of high-redshift black hole binaries to ~64 per year while dropping ET detections to ~4 per year, compared to ~32 and ~64 under Eddington-limited growth.
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Setting the cold neutral medium density to 7500 cm^{-3} in a model for MACS0416_Y1 allows UV trapping and reduced supernova destruction, reproducing the UV-to-FIR SED with intermediate-size grains dominating the infrared output.
citing papers explorer
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Gravitational Waves from the Cosmic Dawn: Tracing Cosmic Black Hole Binaries with ET, LGWA and LISA
Super-Eddington accretion boosts predicted LISA detections of high-redshift black hole binaries to ~64 per year while dropping ET detections to ~4 per year, compared to ~32 and ~64 under Eddington-limited growth.
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Resolving the Dust Budget Crisis at $z \sim 8$ with Optically Thick, High-Density Molecular Clumps: MACS0416_Y1
Setting the cold neutral medium density to 7500 cm^{-3} in a model for MACS0416_Y1 allows UV trapping and reduced supernova destruction, reproducing the UV-to-FIR SED with intermediate-size grains dominating the infrared output.