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- W2803410694 abstract "Recent numerical simulations reveal that the isothermal collapse of pristine gas in atomic cooling haloes may result in stellar binaries of supermassive stars with |$M_*gtrsim 10^4,mathrm{M}_{odot }$|. For the first time, we compute the in-situ merger rate for such massive black hole remnants by combining their abundance and multiplicity estimates. For black holes with initial masses in the range |$10^{4-6} ,mathrm{M}_{odot }$| merging at redshifts z ≳ 15 our optimistic model predicts that Laser Interferometer Space Antenna (LISA) should be able to detect 0.6 mergers yr−1. This rate of detection can be attributed, without confusion, to the in-situ mergers of seeds from the collapse of very massive stars. Equally, in the case where LISA observes no mergers from heavy seeds at z ≳ 15 we can constrain the combined number density, multiplicity, and coalescence times of these high-redshift systems. This letter proposes gravitational wave signatures as a means to constrain theoretical models and processes that govern the abundance of massive black hole seeds in the early Universe." @default.
- W2803410694 created "2018-06-01" @default.
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- W2803410694 date "2018-05-24" @default.
- W2803410694 modified "2023-10-01" @default.
- W2803410694 title "Gravitational wave signals from the first massive black hole seeds" @default.
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- W2803410694 doi "https://doi.org/10.1093/mnrasl/sly091" @default.
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