Time-dependent fluctuations in the gravitational wave background can be large and detectable when the background is dominated by massive, eccentric supermassive black hole binaries or by a single eccentric binary with signal-to-noise ratio near one.
Binary Massive Black Hole Astrophysics
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From eccentric binaries to nonstationary gravitational wave backgrounds
Time-dependent fluctuations in the gravitational wave background can be large and detectable when the background is dominated by massive, eccentric supermassive black hole binaries or by a single eccentric binary with signal-to-noise ratio near one.