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Lucio Mayer04/12/2025, 10:00
The typical binaries of massive black holes that the LISA gravitational wave detector will observe
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are in the range 10^4-10^6 solar masses. In the low redshift Universe, observations of active
galactic nuclei and other types of sources suggest that such black holes preferentially reside
in dwarf galaxies. Dwarf galaxies are notoriously dark matter dominated down to their cores. I... -
John Silverman04/12/2025, 10:30
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