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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. 3 …the FTS Devices ............................................. 30 3.4.1 Propagating Signals From Optical Lattice Clocks for Timing ................ 31…
  • p. 4 …Omni-Directional Nature of the HFGW Radiation Pattern ....................... 10 Figure 8. Predicted Relic GW Energy Density…
  • p. 5 …The Piezoelectric Approach to HFGW generation is best for the proof-of- concept test and the…
  • p. 6 …Antennas, cables, and phone lines would be things of the past. A timing standard alone, provided…
  • p. 8 …over the time interval !1t, s; that is, the jerk or shake of the two masses…
  • p. 9 …The usual difficulty with HFGWs generated by nuclear reactions is the small dimensions of their nuclear…
  • p. 22 …the initial momentum uncertainty, dt is the time of the future measurement, and m is the…
  • p. 23 …Eis the effective energy contained within the detector cavity summed over the detection averaging time, and…
  • p. 24 …The temporal quality factor in the Li-Baker detector arises from averaging the signal over time…
  • p. 28 …Another way to increase Q is to arbitrary increase sample times of the signal. This technique…
  • p. 29 …There is also a hidden integral here which occurs over the sample time, which is understood…
  • p. 30 …3.3 FREQUENCY AND TIME STANDARD The first application of HFGW to the distribution of frequency…
  • p. 31 …The arrival times of the received PPS signals could be compared via time difference of arrival…
  • p. 32 …The universal nature of the HFGW frequency and time standards are especially helpful. The following telecommunication…
  • p. 33 …the search space is reduced, speeding acquisition. • Ultra-fast acquisition allows more efficient TDMA, or Time…
  • p. 34 …For a 5 μsec acquire test time, the result is Tacq = 150 x 150 x 16…
  • p. 35 …At this precision one could measure the time delay caused by changing once centimeter in height…
  • p. 36 …the problem of mapping the positions of the Lagrangian points, which vary slightly over time. 3…
  • p. 38 …As prototypes show promise they could be transitioned to device development, the first time that industry…
  • p. 39 …For instance, if there were one GW source on Earth, and one GW source on the…
  • p. 41 …Nonlinearity improves the focusing process and h goes to one in finite time, producing a singularity…
  • p. 45 …and Stephenson, G.V. (2007), "The Value Estimation of an HFGW Frequency Time Standard for Telecommunications…
  • p. 46 …Thesis, The University of Birmingham, January. Kippenberg, T. J. and Vahala, K. J. (2008), "Cavity Optomechanics…
  • p. 49 …time of future measurement, s effective energy contained within the detector cavity summed over the detection…
  • p. 50 …The project plan and timing are described below under separate headings for each component of the…
  • p. 51 …coils that superimpose upon the constant applied magnetic field a time-varying component at low frequency…
  • p. 53 …photon events, and has very good time resolution. The disadvantage is its cost and complexity. This…
  • p. 55 …Cryogen-free (more accurately, the cryogen is completely enclosed and re-cycled each time the magnet…
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3.3.4 The Impact of Frequency Noise Improvements on FDMA and
FHSS
The very low noise frequency standard that would be supplied by an HFGW FTS system
would allow for much more efficient use of reserved frequency bandwidth. Frequency
noise limits the type of modulation and manner of encoding that can be performed in
frequency space, such as Frequency Division Multiple Access (FDMA) or Frequency
Hopping Spread Spectrum (FHSS). HFGW can reduce frequency noise by providing a
frequency reference with outstanding stability. For example, guard bands can be shrunk
in FDMA, and frequency slices can be smaller and more stable in FHSS.
A frequency space representation of the FDMA and FHSS noise improvements are
depicted in Figure 22.
High Freq Noise Low Freq Noise
C.t.,e Ca,e High hcq Noise Lo" Freq Noise
Ca,e Ca,c
Larger Guard Bands-, Smaller Guard Bands Fewer Freq
Symbols
- ;-;,,. - - ,- ,- ~,-
t
Frequency~
(a) Frequency Division Multiple Access.
t \.
Frequency+-'
(b) Frequency Hop Spread Spectrum.
Figure 22. The Impact of Frequency Noise Improvements on FDMA and FHSS
Efficiencies in guard-band structure can be defined as in Equation (14).
Guard band BW Efficiency = (Total Bandwidth -{Sum of Guard BW} )/Total Bandwidth
(14)
Guard bands often consume 30 to 50 percent of assigned frequency space. While guard
bands would still be required to allow for the side lobes of signals, the frequency error
component would be eliminated. Similar efficiencies may be gained in the FHSS
approach. A better knowledge of absolute frequency allows better frequency coding
efficiencies, as seen in Equation (13) and depicted in Figure 21.
3.4 POSSIBLE FUTURE UPGRADES TO THE FTS DEVICES
Per the 9 Feb 2009 issue of New Scientist, optical lattice clocks are under development
that will lead to a dramatic improvement over the current standard Cesium atomic
oscillation clocks that now provide frequency time standard references. Optical lattice
clocks vibrate at optical frequencies rather than microwave frequencies, with the
reference frequency mixed down via frequency combs to allow measurements back
down in the microwave regime. Strontium lattice clock are already operating with
measurement precisions of 1 part in 10 16 , and theoretical performance approaches 1
part in 10 18 . At this precision one could measure the time delay caused by changing
once centimeter in height in the Earth's gravitational field.
30
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Report, from the dia collection. The PDF is mirrored here; the original link is under it. 57 pages are in the text index: search them above, or from the library's search.