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Defense Intelligence Reference Document High-Frequency Gravitational Wave Communications

Defense Intelligence Agency · 57 pages · text from the file's own layer

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.

  • p. 2 …a series of advanced technolo re orts roduced in FY 2009 under the Defense Intelligence Agency…
  • p. 30 …The bandwidth, B, here is arbitrarily taken to be 100 kHz for a future advanced system…
  • p. 38 …It is difficult to predict even ten years in advance to the time when we expect…
  • p. 41 …The most stunning advances in HFGW applications will probably not be in communications, but in the…
  • p. 42 …its wavelength changes based on gravitational red shift and the gravitational wave backscatters off the curvature…
  • p. 44 …M. (2008), "Very High Frequency Gravitational Waves," Gravitational Wave Advanced Detector Workshop (GWADW), Elba Conference, 17…
  • p. 46 …Magnetic Field," in the proceedings of the HFGW2 Workshop, Institute of Advanced Studies at Austin (IASA…
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The most benefit would come from a coordinated effort spread over a number of
different universities. Wherever possible, pre-existing assets should be utilized to
stretch funding as far as possible. For example, if synchrotron light is needed to verify
the Gertsenshtein effect and the Li-effect, a survey of existing national synchrotron
light facilities should be part of the funded effort to find an appropriate host facility. The
funding activity-that is, the National Science Foundation-would have the overall
responsibility to coordinate this activity in an ongoing manner, through proposal review,
contract awards, and progress reviews, and the approach should be flexible enough to
allow the redirection of funding should a particularly promising new technology or
invention move to the forefront.
Assuming that positive laboratory results can be achieved and peer reviewed in a 10 to
12 year timeframe, the next step would call for a period of prototype development, in
which the device physics and engineering needed to support the technology could be
matured. As prototypes show promise they could be transitioned to device
development, the first time that industry would likely enter the field. Once the
individual devices required to support GW communication technology-for example, GW
generators and GW sensors-are in place, at that point it will be possible to begin full-
scale development of systems applications. This is a conservative timeline, based on
scaling from the development of previous technologies. If breakthroughs materialize, or
if the pace of technological development quickens, progress may certainly occur more
quickly than this.
4.2 HFGW COMMUNICATIONS PREDICTIONS TO 2050
In what follows, with an eye to the future, extrapolations are made concerning the
development of a HFGW communications technology into the far future (for example,
2050 and beyond). It is difficult to predict even ten years in advance to the time when
we expect to have the results of the proof-of-concept test (or "Bell-Watson"
experiment) are available and the immediate applications to HFGW communications
completed. Speculation beyond that time will be contingent upon advanced
development of FBAR crystals, new materials within the toroidal waveguides, and so
forth, or even entirely new approaches such as those proposed by G. Fontana, V.
Rudenko, R. Chiao, et al. No doubt the Li-Baker detector performance can also be
greatly improved with stronger magnetic fields, more intense Gaussian beams, and
better baffles as well as new detector designs yet to be developed possibly based upon
theories developed at Birmingham University, INFN Genoa and The National
Astronomical Observatory of Japan. Optimum designs of communication channels,
bands and modulation are also be anticipated. Many of these advanced concepts were
discussed at the 3rd HFGW Workshop in Huntsville in February 2009. Nanotechnology
advances will allow for the fabrication of smaller and smaller HFGW transceivers having
millimeter dimensions and milliwatt power requirements by 2050 and "Radio ID" or
rather "HFGW ID" nanochip tags may be ubiquitous. Gravitational wave transmissions
would also have the advantage of being able to pierce the protective plasma shielding
that may in the future be routinely used to protect the crew aboard manned vessels-
that is, communications through artificial magnetospherics, a technological limit of RF
communications.
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