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This Defense Intelligence Reference Document was prepared by the Defense Intelligence Agency under its Advanced Aerospace Weapon System Applications (AAWSA) program, is dated 6 April 2010 and is part of a series of advanced technology reports produced in FY 2009. It reviews proposed laboratory generators and detectors of high-frequency gravitational waves for communications. It favors an infrared-excited molecules transmitter and the Li-Baker detector, estimating about 1.9 million bits per second over 7,000 km through the Earth. It also discusses timing standards and interplanetary navigation uses.
UNCLASSIFIED//P9R: 9PPH!ltlrt 1!181!! 8HLY The figure of merit for a HFGW generator is given explicitly by Baker, Woods and Li (2006). This Figure of merit can be extended by considering other effects since in the laboratory the force change could not even approach those of the celestial sources. It would seem that the magnitude of any laboratory generated GWs could be best increased (1) by utilizing electromagnetic forces rather than gravitational, (2) by increasing the distance between the gravitational radiators, (3) by increasing the GW frequency (that is, reducing ti.t) and especially (4) by developing a large number of in- phase system elements. This last effect enters as the square of the number of elements, N , as proved using General Relativity analyses by Dehnen and Romero- Borja's analyses (Romero and Dehnen, 1981; Dehnen and Romero, 2003). Such N2 dependence also may be the key to successful laboratory generation of GWs, especially HFGWs. In that regard, recent proposal by Woods (Woods and Baker, 2009; Black and Baker, 2009)) propose the use of infrared-energized atomic nuclei, electrons and or molecules, which have a very large N, contained in a stack of N waveguide rings (Patents Pending). The distance between GW radiators may be proportional to the GW wavelength in that it may have a limit that is less than or equal to a GW wavelength. The wavelength is inversely proportional to the GW frequency. Thus given some value for the proportional constant, say unity or the distance between radiators equal to one GW wavelength, the GW frequency cancels out. As already noted it is important to take advantage of square of the number of in phase elements for useful laboratory HFGW generation. If the elements are sliced in one dimension (the dimension along the axis of HFGW generation) in order to increase the number of elements, then the change in force per element will be inversely proportional to the number of elements. For example, if the elements are sliced into one hundred separate pieces, then each piece will have one hundredth of the force of the unsliced element. Essentially, f = ma and it is assumed that the acceleration of the element was the same after the split as before. This result also follows Equation (8), page 17 in Baker, Stephenson and Li (2008b) and if there were 100 splits of an FBAR, then the power to an individual slice, P and its mass, m would be both one hundredth of their un-split value and the square root of their product would again be one hundredth. The frequency of the split elements may be a higher value -- but the attendant increase in GW power proportional to the square of the higher frequency and the decrease in power due to a smaller distance between tracks (assuming that the distance between tracks is one GW wavelength, which would be smaller) would cancel and there would be no net effect on HFGW amplitude. It is concluded, therefore, that in this particular special situation the amplitude of the generated HFGWs is proportional to the number of in-phase elements, N (not the square). In any event a large number of elements for a given HFGW-generator length can be best realized by reducing the size of the individual elements to submicroscopic size (as discussed in U.S. Patent Number 6,784,591). In the case of HFGW generation for communications applications, it is important to relate the amplitude of a GW, A, with the power, P, or more exactly with the GW flux, FGw, in wm- 2 . For a viable communications link, the HFGW amplitude, A, must be large enough to be detected at the HFGW receiver. From Appendix B of Baker, Woods and Li (2006 ), A = 1.28x 10-18 ( FGw/VGw)½ m/m where A has the dimensionless value of spacetime strain or m/m and VGw is the GW frequency s- 1 . Following the proceeding numerical example we will concentrate the HFGW on a diffraction-limited area of 4x 10-3 m 2 or 0.004 m 2 for a HFGW flux of 5 UNCLASSIFIED/ ,'P8"1 8PPll!l"'I! l!l!il! 8111!¥ (2)
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Report, from the dia collection. The PDF is mirrored here; the original link is above. 57 pages are in the text index: search them above, or from the library's search.