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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. 4 …Change in Centrifugal Force of Orbiting Masses, .dfct, Replaced by Change in Tangential Force, Aft, to…
  • p. 5 …cannot be shielded or shadowed by planetary masses. Plasma interference seen at planetary entry would be…
  • p. 8 …Change in Centrifugal Force of Orbiting Masses, b.fc1, Replaced by Change in Tangential Force, 4ft…
  • p. 9 …as the particles move through a target mass. The usual difficulty with HFGWs generated by nuclear…
  • p. 10 …to an individual slice, P and its mass, m would be both one hundredth of their…
  • p. 13 …radiation pattern for a pair of orbiting masses. GW l I T GW Figure 4. Radiation…
  • p. 14 …The mass density of pentane is divided by its molecular mass and that gives the density…
  • p. 17 …In 1995 Tobar characterized multi-mode resonant-mass HFGW detectors and three years later in 1998…
  • p. 22 …E/c2 may be substituted for mass in an energy only system. This is depicted in…
  • p. 36 …as strongly affected by the presence of mass. Such a differential propagation delay comparison (between RF…
  • p. 41 …The concept is that the mass essentially "rolls" down a "hill" produced by the static g…
  • p. 47 …V. (2009a), "Lessons for Energy Resonance HFGW Detector Designs Learned from Mass Resonance and Interferometric LFGW…
  • p. 48 …Tobar, M, 1729-1736 E. (1995), "Characterizing multi-mode resonant-mass gravitational wave detectors," Journal of…
  • p. 49 …pairs of oppositely jerking at one-time mass elements, integer power of the generated gravitational waves…
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4.5 2050 and Beyond ....................................................................................... 37
5.0 Acknowledgements ........................................................................................ 37
6.0 References ..................................................................................................... 37
Appendix A: Nomenclature ................................................................................... 44
Appendix B: Li-Baker HFGW Detector ................................................................... 45
Appendix C: Perturbative Photon Fluxes Generated By High-Frequency
Gravitational Waves and Their Physical Effects .................................... 52
Figures
Figure 1. Communication Link Block Diagram ........................................................ 2
Figure 2. Change in Centrifugal Force of Orbiting Masses, .dfct, Replaced by Change
in Tangential Force, Aft, to Achieve HFGW Radiation ............................... 3
Figure 3. Circular Resonator Geometry Using Infrared Excitation .......................... 8
Figure 4. Radiation Pattern Calculated by Landau and Lifshitz (1975) ................... 8
Figure 5. GW Flux Growth Analogous to Stack of N Orbital Planes ......................... 9
Figure 6. Stack of Circular-Wave-Guide Plates With Typical Molecule Jerks, .df's ... 9
Figure 7. Omni-Directional Nature of the HFGW Radiation Pattern ....................... 10
Figure 8. Predicted Relic GW Energy Density as a Function of Frequency ............. 11
Figure 9. Birmingham University HFGW Detector ................................................. 13
Figure 10. INFN Genoa HFGW Detector ................................................................ 13
Figure 11. The National Astronomical Observatory of Japan 100 MHz Detector ... 14
Figure 12. Detection Photons Sent to Locations that are Less Affected by Noise .. 15
Figure 13. Quantum Back Action as a Mechanism for Creating the Standard
Quantum Limit ..................................................................................... 17
Figure 14. Schematic of Ultra-Sensitive HFGW Detector ....................................... 21
Figure 15. Fractal Membrane Component of Li-Baker Detector Exhibited in Planar
Form .................................................................................................... 21
Figure 16. Conceptual SNR Fill Factors: Signal and Noise Components ................ 23
Figure 17. A Block Diagram of a Typical Link Budget ............................................ 24
Figure 18. A Proposed Near Earth Distribution of Frequency Time Standard ........ 26
Figure 19. HFGW Supplemented Remote Terminal Design .................................... 27
Figure 20. Acquisition Search Space Improvement Accruing From HFGW FTS ...... 28
Figure 21. The Impact of Phase Noise Improvements on Phase Shift Encoding ... 29
Figure 22. The Impact of Frequency Noise Improvements on FDMA and FHSS ..... 30
Figure 23. The Earth's Associated Lagrangian Points ........................................... 31
Figure 24. HFGW Com Space Application Development Roadmap, Estimated
Timeline .............................................................................................. 32
Figure 25. A GW Pair on Earth as Used by a Lunar Mission ................................... 34
Figure 26. A GW Pair on Earth and on the Moon, as Used by a Mission to Mars .... 35
Figure 27. A GW Pair on Earth and on Mars for an Outer Planetary Reference
Pair ...................................................................................................... 35
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