The tiny bar vibration induced by a passing g.w. is
easily masked not only by the thermal noise (thus making necessary to cool
down the bar) but also by the mechanical and acoustical noises. The
acoustical noise coming from the laboratory environment is suppressed by
placing the bar in a vacuum chamber: in AURIGA two vacuum chambers (the
OVC and the IVC that houses the bar) provides for this insulation.
A more difficult task is to reduce the mechanical noise: this is due to
floor vibrations, caused for instance by any nearby moving vehicle or
walking person and by the intrinsic seismic noise. The AURIGA cryostat is
placed on the top of a special 200tons heavy concrete platform, separated from the rest of the
laboratory. The platform sits on a sand layer which reduces by -20dB the
mechanical noise at the floor: on the platform this is measured to be 2x10-14m/Hz½ around the AURIGA
bar resonant frequency (which occurs at 920 Hz). Unfortunately this noise
figure is still too high for a g.w. experiment as AURIGA: other insulation
stages are necessary so to reduce the mechanical noise felt at the bar
input down to a negligible level.
The
fundamental idea for the suspension employed in AURIGA is to take
advantage of the properties of a damped harmonic oscillator: for
frequencies higher than the the oscillator's resonance, the displacement
transfer function decreases with a slope of -6dB/octave. The basic suspension
stage is indeed a spring-mass system, whose resonant frequency is chosen
to be much smaller than the bar resonance (i.e. the frequency of
interest). By the way in a real spring-mass system one must take into
account its internal modes which add structure to the transfer function
and complicate the design of the suspensions for AURIGA. This is further
complicated by the requirement of preserving the bar high mechanical
quality factor and of the detector overall volume being not too
large.
The solution adopted in AURIGA is to take advantage of the thermal
shields that needs to be employed in the cryostat in order to cool down
the bar. For what concerns the suspension, the thermal shields act as the
masses in the spring-mass systems; the cables that support the shields in
cascade constitute the spring. The last suspension stage (i.e. the last
spring-mass system) is provided by the cable that suspend the bar and the
bar itself: the bar is suspended horizontally by a belly copper cable
around the bar middle section. Except for the little cables for the
transducer and the calibrator, the belly cable is the only connection of
the bar with the rest of the world!
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Fig. 1 is a schematic of the suspension
design in AURIGA: suspensions and cryogenics are fully integrated. More
details and suspension performances are listed in the following table (they
refer to room temperature measurements in the frequency range
800Hz÷1000Hz). The total mechanical gain of the overall suspension is -240dB at bar
resonance.
| Mechanical filter |
mass [tons] |
suspension |
mean vertical gain |
| Al5056 bar |
2.3 |
Cu-OF belly cable |
-100 dB |
| Cu inner shield |
0.5 |
4 rods of Ti64 |
-45 dB |
| Cu middle shield |
0.5 |
4 rods of Ti64 |
-40 dB |
| Cu outer shield |
1.6 |
4 rods of Ti64 |
-30 dB |
| Liquid He vessel |
2.0 |
4 rods of Ti64 |
-25 dB |
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