Lenient heavy-seed models in BRAHMA simulations produce black hole merger rates above 100 per year and near-unity occupation fractions down to low-mass galaxies, while strict models yield only about 1 merger per year and occupation fractions below 10 percent for galaxies under 10^8 solar masses.
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A review summarizing established modeling techniques, open questions, and research directions for three classes of LISA gravitational wave sources.
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Astrophysics with the Laser Interferometer Space Antenna
A review summarizing established modeling techniques, open questions, and research directions for three classes of LISA gravitational wave sources.