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Confusion background from compact binaries · Around

2009

Confusion background from compact binaries

Regimbau, T., Hughes, Scott A.

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Double neutron stars are one of the most promizing sources for terrestrial gravitational wave interferometers.

For actual interferometers and their planned upgrades, the probability of having a signal present in the data is small, but as the sensitivity improves, the detection rate increases and the waveforms may start to overlap, creating a confusion background, ultimately limiting the capabilities of future detectors.
The third generation Einstein Telescope, with an horizon of $z > 1$ and very low frequency ``seismic wall'' may be affected by such confusion noise.
At a minimum, careful data analysis will be require to separate signals which will appear confused.

Built on

V. Kalogera et al., Astrophys. J. 614
2004
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D. E. Holz and S. A. Hughes, Astrophys. J. 629
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A. M. Hopkins and J. Beacom, Astrophys. J. 651
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K. Nagamine, J. Ostriker, M. Fukugita, and R. Cen, Astrophys. J. 653
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Earlier work this paper cites.

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Then

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