Gravity Geselleschaft

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Gravity waves passing through a piezo material such as crystalline quartz or tourmaline cause varying charges across the crystal, resolvable to +one ten thousandth of the charge on a single electron+ by a newly invented device, the Quantum Dot Transistor (Elect. Eng. Times, June 24,'96)). A large phased array of such detectors could be correlated to filter out noise to arbitrary levels of sensitivity, and provide directionality. To avoid terrestrial noise, the array could consist of a spread formation of small spacecraft using laser ranging to monitor positions. Such a scheme may be sensitive enough for a practical "gravity telescope".


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Homebrew Gravity Hacking-

To reduce non-gaussian interference, a global network of GPS timebase-correlated cryogenically cooled crystals is proposed to allow computational filtering of signal noise. Local arrays to allow effective filtering of local noise. An array allows wave information such as phase as well as simple periodicity.

This approach had potential advantages over traditional experiments consisting of large metal rods with vibration transducers. One seeming advantage is direct signal pickup by the antenna vs the use of a secondary transducer .

Alignment of the piezo crystal lattice with the gravity wave target-

It may be that a piezo crystal based gravity antenna allows better angular resolution compared to previous designs. Potential off axis noise immunity, combined with alignment at a tangent to the earth's surface, might greatly mitigate gravitational noise from churning of the earth's interior (or even the sun). With regard to angular resolution, a further intuition is that a high aspect ratio is desirable for the crystal rod. It may be that a whisker shape, alone or in an array, is best suited for experimentation. Arbitrarily large antenna elements could be made by stacking piezo elements lengthwise, which may prove necessary to achieve sufficient voltage sensitivity.

Active feedback control of the antenna-

The piezo effect works both ways- stress a crystal and a charge develops, or charge a crystal and it stresses. (Piezo crystal behavior is based on a flexing helical crystal lattice. As a kid I wondered why a little cloud in the shape of a tornado could be faintly seen in a quartz/amethyst. It turns out that minor impurities are sometimes carried along the crystallization front and deposited in a ghostly image of the invisible structure.)

Variable stressing of the piezo antenna, by charging it, could offer a means to tune it to specific resonances.

A key issue was how to deal with noise created by antenna dampening. It would help if the antenna were resonant with the signal, but how does one build a broadband tunable gravity antenna? One might use an array of variably tuned antenna elements. A charge to the piezo crystal that changes its resonant frequency might serve for fine tuning. A switched network of stacked crystals might enable broad tuning.

Unstressing a crystal reduces its temperature and this might be a basis for momentarrily reducing cryogenic temperature beyond what's otherwise practical. Prestressing the crystal might allow more violent voltage and mechanical inputs. A piezo stressed flywheel might hold together at monstrous RPM.


The original brainstorming group started from the premise that giant natural crystals, as monstrous single molecules, may have unique properties otherwise unavailable to science and engineering. Exploiting the fantastic precision of such objects, down to the atomic scale, amounts to a sort of natural nanotechnology.

A basic insight was that feeding a signal into a piezo crystal amounts to a "gravity wave projector", albeit at a very weak level. This effect suggests several cool applications. Communications might be possible between two crystals. Thus the long awaited experimental confirmation of Einstein's prediction might be determined at relatively low cost. An alternative is to just use the crystal as a sensor using something like a big artillery piece to generate a gravity pulse.

Phased arrays of crystal projectors could manipulate standing gravity waves for such purposes as artificial gravity and "tractor beams". Gravity wave emitter arrays could form the basis of future space propulsion systems.

A shaped stack of crystals can be pumped like a rail gun to build up usable gravity pulses.

Date: Wed, 29 Apr 1998 13:57:54 -0700
From: jeremy rutman jeremy_rutman@bigfoot.com
To: gravity@zilker.net
Subject: piezo limits
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Wow-I was just in the dumps 
(http://www.polycosmos.org/gravhack/mail.htm), 
wondering what current limits on piezo sensitivity are
and thinking in any case interferometry is unbeatable.
Then I found:

        RECORD NO.:  5408617 INSPEC Abstract No: A9623-8170C-069
            AUTHOR:  Fortunko, C.M.; Boltz, E.S.
       CORP SOURCE:  Mater. Reliability Div., Nat. Inst. of Stand. &
Technol., 
                     Boulder, CO, USA
             TITLE:  Comparison of absolute sensitivity limits of
various 
                     ultrasonic and vibration transducers
            SOURCE:  Mater. Sci. Forum (Switzerland), Materials Science
Forum, 
                     vol.210-213, pt.1, p. 471-8
              ISSN:  0255-5476

"...of wide-band AE studies in metals. Furthermore, we find that 
a new, conical, piezoelectric transducer, based on a 
refinement of the NIST secondary-standard transducer, 
appears to have sufficient sensitivity for such 
applications. In particular, this new transducer is found to 
exhibit absolute sensitivity that approaches the "thermal 
rattle" limit in aluminum within 10 dB in the 250 kHz to 1 
MHz region. Also, we show that the new transducer's noise 
floor is below the noise floors of optical interferometers, 
air-coupled capacitive transducers and EMATs"





First experiments-

The oldest traditions in fusion, aviation, and gravity wave reasearch, built experimental  
devices with faint immediate hope. These devices were necessary  
contemplation objects toward the detail engineering of true prototypes. 


In this spirit I made crude devices from  
cheap natural crystals, mountings, high voltage  
sources, and commercial grade FETs. There was zero expectation of tangible results. The quick and dirty tests made with the hardware were almost purely ceremonial.  


Machining crystals-

Preliminary work is underway to machine quartz cylinders  
from natural samples. The Aztecs used reeds (!) with sand  
abrasive and bow drills to machine quartz, so we will try brass  
tubes on a machine lathe with a water-borne abrasive. The resulting  
cylinders are to be polished to eliminate micro-flaws that as stress  
concentrators promote violent mechanical failure of the crystal  
under highly charged conditions.




A loose end is a comment at a Japanese gravity science Website (  
http://www.icrr.u-tokyo.ac.jp/gr/English/theory/resonant.html ) that  
piezo transducers on historic metal rod instruments did not work well  
at cryogenic temperatures. I do not yet know if this applies only to  
man-made ceramic piezo materials, or the magnitude of sensitivity  
loss, if any, by supercooled quartz or tourmaline.




====included message=====  


> 2) Please critique the following concept for a gravity wave  
detector
> based on piezo effect-
>
> -Set up globally distributed network (an LBA to filter out local
> seismic and other noise) of machined giant quartz crystals  
(available
> in 3' plus lengths or stack smaller crystals to long lengths) with
> crystal lattice precisely aligned with gravity wave source.
> 

> -Proposed target source would be of a known period from
> electromagnetic evidence.
> 

> -As gravity waves compress and stretch crystals along long axis a  
few
> electrons should pop back and forth from a sensitive end mounted
> electrostatic pick up.
>
> -Use GPS timing signals to correlate the distributed nodes.
>
> -Use noise filtering techniques to sift for gravity wave signal.
>

Your scheme eliminates two major sources of  error, seismic and  
non-gaussian.  Seismic is important at very low frequencies, say  
lower than 100 Hz.  Non-gaussian is the technical name for acts of  
god, like a truck hitting your building, or a high energy cosmic ray  
hitting your detector.  Your scheme of putting multiple detectors at  
different locations and then recombining the signal using timing info  
etc.  handles this nicely (although there could be problems with a  
random event that effects the whole earth, say  a sudden increase in  
the solar wind leading to an increase in particles hitting the earth.   
But still, millisecond timing should be able to eliminate these  
events.)

However, at high frequencies, above 500 Hz or so, the major cause of   
noise is thermal vibrations of the antenna.  Regardless of the  
material, its temperature causes noise.  All operating antennas are  
cooled to at least 4 K with liquid helium but even that is not cool  
enough.  The current goal is to cool a spherical antenna to 50 mK  
using a dilution refrigerator. 


Then you have noise from the damping in the antenna.  The  
dissipation/fluctuation theorem states that you will get noise from  
any source of loss in a system.  Since the antenna will always have  
some loss (if you hit it, it won't ring forever) you will get noise  
from that.  So the goal is to minimize this.  This is the famous "Q"  
factor that we worry about so much.  Using aluminum, current Q values  
are around 10 million at 4 K.  We need to have them up around 50  
million.

That said, the problem with your quartz antennas might be the  
ability, not just to construct them, but to do it in such a way to  
get high Q.  Using their piezoelectric properties to get an  
electrical output, although a neat trick, is not that helpful.  There  
are currently mechanical transducers that can magnify the tiny  
vibrations in an aluminum antenna enough without introducing too much  
noise, that conventional electrical amplifiers can then amplify the  
signal.  Your scheme has the advantage of not requiring a second  
mechanical system, which also needs to have a high Q.  However, it  
requires sophisticated knowledge of the mechanical properties of  
quartz at low temperature.  I don't know of anyone who has made  
macroscopic objects out of quartz that have Qs of 10s of millions at  
liquid helium temperatures.  But if this a solved problem with an  
industry capable of constructing such an antenna, it becomes an  
attractive idea.

Gregg Harry gharry@wam.umd.edu



Active Damping/Exciting of piezo mass to manipulate bandwidth.-ds


http://www.nitehawk.com/Mystical.Crystal/atlcrpw.htm



================

A good background info. link-

http://www.piezo.com/histry.html

===============

http://www.pd.uwa.edu.au/Grav_Wave/AdvResMass.html

ADVANCED RESONANT-MASS GRAVITATIONAL WAVE
DETECTORS APPROACHING  
QUANTUM LIMITED SENSITIVITY

Michael .E. Tobar

Australian International Gravitational Research Centre, Dept. of  
Physics, 

University of Western Australia, Perth, 6907, Australia

A large improvement is envisaged for the University of Western  
Australia's (UWA) resonant-mass Gravitational Wave (GW) detector due  
to a new type of parametric transducer constructed from low-loss  
monocrystalline sapphire. Single pieces of crystals can be used as  
both the resonant microwave transducer and a tuned resonant  
mechanical mass. The sensitivity is determined by the acoustic losses  
in the detector as well as the phase noise of the pump oscillator  
driving the transducer. Newly developed cryogenic microwave  
oscillators are now available with ultra-low noise levels of -165  
dBc/Hz [1]. We project that this can be further reduced to -185  
dBc/Hz with the advent of recent technology. Calculations suggest by  
implementing this technology the noise temperature can be reduced  
from a few mK to the order of micro Kelvin in a liquid helium  
cryostat. This sensitivity can be achieved in the short term with  
very little expense in comparison to the construction of an  
interferometer, and is ideal for correlation experiments with the  
proposed AIGO interferometer. Cryogenic sapphire transducer  
technology presents a viable alternative to SQUID technology.

The quantum limit of a resonant mass at 4 K is of the order of a few  
hundredths of a micro Kelvin. We show it is possible to measure such  
a low noise temperature in a Sapphire Dielectric Bar Transducer  
(SDBT). 


[1] R.A. Woode, M.E. Tobar, E.N. Ivanov, D.G. Blair, An ultra-low  
noise microwave oscillator based on a high-Q liquid nitrogen cooled  
sapphire resonator, to be published in IEEE Trans. on UFFC, 1996.

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