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.
Title resolution pending
1 Pith paper cite this work. Polarity classification is still indexing.
1
Pith paper citing it
fields
gr-qc 1years
2024 1verdicts
CONDITIONAL 1representative citing papers
citing papers explorer
-
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.