Figure 27: Detection limits of TAMA, first LIGO, advanced LIGO, and Large-scale Cryogenic
Gravitational wave Telescope (LCGT) with the expected GW spectrum obtained from the numerical
simulations. The left panel shows the GW spectrum contributed from neutrinos (solid) and from the
matter (dashed) in a rotating model with imposed initially on a progenitor
model. In the right panel, the open circles and the pluses represent the amplitudes of with
the characteristic frequencies of for the models with the cylindrical and the shell-type rotation
profiles, respectively. Under the frequency of , the GWs from the neutrinos dominate over those
from the matter contributions. From the panel, it is seen that the GWs from neutrinos dominate
over the ones from the matter in a lower frequency ( ). Note that the source is assumed
to be located at the distance of 10 kpc. (Figures from [166]; used with permission.)
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