istituto di fisica dello spazio interplanetario a gradiometric measurement of g xciv congresso...
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Istituto di Fisica dello Spazio Interplanetario
A gradiometric measurement of G
XCIV Congresso Nazionale SIFGenova, 22-27 Settembre 2008
V. Iafolla, E. Fiorenza, C. Lefevre, S. Nozzoli,R. Peron, M. Persichini, A. Reale, F. SantoliIstituto di Fisica dello Spazio Interplanetario (IFSI/INAF), Roma, Italy
Istituto di Fisica dello Spazio Interplanetario
Gundlach, J. H. and Merkowitz, S.M. Phys. Rev. Lett. 85, 2869-2872 (2000)
Current knowledge of G
with a relative uncertainty:
Current experimental results for G are characterized by very small errors, but with big discrepancies among the various results:
Gu
nd
lach
et
al.
Last “best” measurement:
However, the values obtained in the various experiments differ one from the other by more than 600 ppm
2131110)000092.0674215.6( sKgmG
ppmG
G14
Istituto di Fisica dello Spazio Interplanetario
Gu
nd
lach
et
al.
The currently recommended value of G by CODATA is:
with a relative uncertainty:
The discrepancies in the results for G of the various experiments are a proof of the presence of significant systematic errors in the experiments, as well as of the difficulty in carrying out the experiment. This also stresses the importance of the use of different techniques in measuring G.
The difficulties of the measurement of G are related with the smallness of the gravitational effects, to the presence of spurious effects (vibrational, thermal, electromagnetic), as well as to the implementation of the required metrological precision.
Current knowledge of G
2131110)00067.067428.6( sKgmG
ppmG
G100
Istituto di Fisica dello Spazio Interplanetario
Torsion balances
2r
MmGF
The test bodies are attached at the opposite ends of a horizontal beam which is suspended with a wire from its midpoint. Any force acting differently on the test masses and perpendicular to the plane formed by the beam and the wire, gives rise to a non zero net torque which will twist the wire by an angle proportional to the differential force itself.
Current knowledge of G
Istituto di Fisica dello Spazio Interplanetario
Current knowledge of G
Istituto di Fisica dello Spazio Interplanetario
Why measuring G ? (the locally measured gravitational constant GL)
G represents a fundamental constant of Nature both in Newton theory as well as in Einstein’s Geometrodynamics
G enters in several mathematical expressions with other fundamental constants (G is a conversion factor …)
One very important problem in modern physics is to know whether the quantities known as constants in Nature (G, c, h, e, …) can vary with time or not
Indeed, nonstandard theories of gravity predicts both a spatial and a time dependency of G
…
No more to say about the importance of G measurements
Current knowledge of G
Istituto di Fisica dello Spazio Interplanetario
• A characteristic of such gradiometer is the detection of the off–diagonal components of the gravity gradient tensor
• At the same time the gradiometer rejects the linear acceleration due to the vibrational noise, the so–called Common Mode Rejection (CMR)
One–axis gravity gradiometer
Al 5056
X
Y
Z
ZX
A preliminary experimental work has been performed in order to measure the gravitational (constant) G using a one axis gravity gradiometer
Istituto di Fisica dello Spazio Interplanetario
• The test mass is connected to an external reference frame by means of two torsional arms
• The torsion axis is also the symmetry axis of the test mass
• The oscillator is sensitive to the rotations of the horizontal plane
• The torque produced by the gravity gradient is balanced by the torsional spring of the oscillator
One–axis gravity gradiometer
Al 5056
X
Y
Z
ZX
Istituto di Fisica dello Spazio Interplanetario
One–axis gravity gradiometerMI
HzI
f 12
1
20
0
M gravitational torque signal deflection
torsion elastic constant I moment of inertia of the test mass coefficient of dissipation1.00
I
Q
The oscillator works in the region where its transfer function is flat, below the resonance frequency f0:
20
I
MM
Al 5056
X
Y
Z
ZX
Istituto di Fisica dello Spazio Interplanetario
One–axis gravity gradiometer
fb
ICZT
Q
T
m
kM on
ntr
obt
2
22 24)(
The pick-up system The signal is detected by means of a capacitive transducer in a bridge configuration
The bridge is driven by a voltage with high frequency fp trough a transformer
The output signal at frequency fr = 10 KHz produced by the unbalancing of the bridge is detected as a modulation of the bias voltage
Total torque noise of the oscillator
Istituto di Fisica dello Spazio Interplanetario
Common mode rejection: CMR• Usually, the rejection is quite difficult with different instruments: we need two
equal transfer functions
• The rejection is very important because of the vertical seismic noise
• Indeed, the limit in the accuracy of measurement is given by the value of the seismic noise on the oscillator around the frequency of the gravitational signal to be detected
• Of course, the seismic noise that does apply a torque on the system is not rejected
Al 5056
X
Y
Z
ZX
Istituto di Fisica dello Spazio Interplanetario
• In order to obtain the CMR we need to take the difference of the two measurements (time span of about 8 days)
• With the one–axis gradiometer the rejection is automatic and the CMR is valid both for the mechanical signal and the thermal one
Common mode rejection: CMRA way to obtain CMR is to take two equal accelerometers (with the same transfer function) with their sensitive axis almost parallel to the horizontal plane
Two equal accelerometers
Istituto di Fisica dello Spazio Interplanetario
System parameters: experimental measurements…
The main parameters to be measured in the laboratory are:
1. The system resonance frequency
2. The mechanical quality factor
3. The system transfer function (ambient conditions)
4. The electrical parameters
5. The transducer factor (calibration)
6. The seismic noise at the frequencies of interest of the gravitational signal
Istituto di Fisica dello Spazio Interplanetario
System parameters: experimental measurements …
• The measurement has been performed under vacuum conditions in order to have a higher Q(=3), but low enough in order to excite the system with an electric signal
• The experimental value for the frequency is 1.01 Hz
Q=3Q=3
Amplitude Phase
Hzf 01.10
Transfer function and resonance frequency
Istituto di Fisica dello Spazio Interplanetario
• At ambient pressure the oscillator is an overdamped system because of the gas between the capacitor plates
• We are interested to measure gravitational signals around 101 Hz, therefore a smaller Q is possible
• Again, the system has been excited with an electric signal
Q=0.1 Q=0.1
Amplitude Phase
System parameters: experimental measurements …
Transfer function in ambient conditions
Istituto di Fisica dello Spazio Interplanetario
System parameters: experimental measurements…
V
mN
V
M
41058.1M
ΔV
Calibration procedure for the transducer factor
The response of the system is linear
Istituto di Fisica dello Spazio Interplanetario
Measurement of the gravitational effect• The rotor is made by suspending a system
of two masses on a wire
• The one–axis gradiometer detector is placed inside a metallic box in order to provide electric isolation of the system
• The sources are two cylinder filled with fused Pb: 29 kg each mass
• The frequency of the gravitational signal is twice the rotation frequency of the rotor: in this way noise effects induced by the rotation of the system are avoided
An electric motor produces the desired rotation
Source masses:
D = 18 cm
H= 11.5 cm
The experimental apparatus
Istituto di Fisica dello Spazio Interplanetario
Measurement of the gravitational effect
In order to maximize the gravitational effect, the two centers-of-mass of the gradiometer (in black) were placed as close as possible to the two sources (in red)
Blue = gravitational signal
Red = noise of the rotor
Spectrum of the signalSignal
The experimental apparatus
Istituto di Fisica dello Spazio Interplanetario
Measurement of the gravitational effect
2 4 6 8 10 12 14 16
0
1
2
3
4
5
6
7
x 10-9
Time [s]
Mom
entu
m N
*m
10-3
10-2
10-1
100
101
10-12
10-11
10-10
10-9
10-8
Frequency [Hz]
Mom
entu
m N
*m
Numerical evaluations with a finite elements method
221110*)22.8( KgmNG
Experimental results
Comparison of the experimental results with the theoretical (numerical) predictions
Metrological errors:
• Masses
• Distances
Istituto di Fisica dello Spazio Interplanetario
Measurement of the gravitational effect
10-5
10-4
10-3
10-2
10-1
100
10-14
10-12
10-10
10-8
10-6
10-4
freq(Hz)
acce
lera
tion(
g/sq
rt(H
z))
Electronic noise
Rotor noise
Rotor + signal noise
Accuracy of the measurement
32 1010 N
S
At IFSI laboratory
5 hours integration time
HzgS 710
HzgN 10105
HzgN 11101
410N
S
At Gran Sasso laboratory: lower differential noise
Istituto di Fisica dello Spazio Interplanetario
Recent results
New design for the gradiometer
Istituto di Fisica dello Spazio Interplanetario
Recent results
Resonance frequency
Istituto di Fisica dello Spazio Interplanetario
Conclusions
1. The one–axis gradiometer is able to measure G with a fractional accuracy of about 104, i.e., 100 ppm
2. This accuracy is competitive with other measurements in the literature
3. However, such a result can be reached if and only if all the other parameters entering in the gravitational law are measured with the same accuracy:
3.1 Homogeneity and density of the masses, their shape
3.2 Center–of–mass positions
3.3 Distances
4. A laboratory with a very low seismic noise and stable temperature is necessary (possibly no variations at the gravitational signal frequency)
5. At first, because of its higher frequency, the one–axis gradiometer seems unfavourable when compared with torsion balances
Istituto di Fisica dello Spazio Interplanetario
Conclusions
6. On the contrary this instrument has several advantages:
6.1 The system is excited at a specific frequency in a frequency band where the seismic noise is very low
6.2 The CMR is high, only differential noise will matter
6.3 A capacitive bridge is used for the detection of the signal
6.4 The system undergoes small displacements and it is not subjected to the hysteresis of the spring
6.5 The system can be calibrated very easily
6.6 With the use of electric fields we are able to lower its resonance frequency
6.7 The system works in free fall conditions, therefore it can be used in space