Me. Tobar et al., Parametric transducers for the advanced cryogenic resonant-mass gravitational wave detectors, GEN RELAT G, 32(9), 2000, pp. 1799-1821
It is shown that a large improvement in liquid helium and ultra-cryogenical
ly cooled resonant-mass gravitational wave detectors can be achieved throug
h improved parametric transducers using either low loss sapphire dielectric
resonators or niobium re-entrant cavities. Performance is analysed in rela
tion to the existing resonant bar antenna Niobe and to massive spherical de
tectors. Applied to Niobe, a millisecond burst sensitivity of order 10(-20)
be achieved, corresponding to a spectral strain sensitivity of 2 x 10(-22)
/root Hz With a 50 Hz bandwidth. Applied to an ultra-cryogenic 117 tonne sp
herical detector made from CuAl, a spectral strain sensitivity of better th
an 10(-23)/root Hz with a bandwidth of order 100 Hz can be achieved, which
is close to the quantum limit. This sensitivity is comparable to that of ad
vanced interferometer detectors at this frequency.