Do floating orbits in extreme mass ratio binary black holes exist?
Shasvath J. Kapadia; Daniel Kennefick; Kostas Glampedakis · 2013 · arXiv
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Abstract (excerpt)
This paper examines the possibility of floating or non-decaying orbits for extreme mass ratio binary black holes. In the adiabatic approximation, valid in the extreme mass ratio case, if the orbital flux lost due to gravitational radiation reaction is compensated for by the orbital flux gained from the spins of the black holes via superradiant scattering (or, equivalently, tidal acceleration) the orbital decay would be stalled, causing the binary to "float". We show that this flux balance is not, in practice, possible for extreme mass ratio binary black holes with circular equatorial orbits; f
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Metadata source: arXiv