Statistical properties of astrophysical gravitational-wave backgrounds
  We investigate how a stochastic gravitational wave background, produced from
a discrete set of astrophysical sources, differs from an idealised model
consisting of an isotropic, unpolarised, and Gaussian background. We focus, in
particular, on the different signatures produced from these two cases, as
observed in a cross-correlation search. We show that averaged over many
realisations of an astrophysical background, the cross-correlation measurement
of an astrophysical background is identical to that of an idealised background.
However, any one realisation of an astrophysical background can produce a
different signature. Using a model consisting of an ensemble of binary neutron
star coalescences, we quantify the typical difference between the signal from
individual realisations of the astrophysical background and the idealised case.
For advanced detectors, we find that, using a cross-correlation analysis,
astrophysical backgrounds from many discrete sources are probably
indistinguishable from an idealised background.
