Documents / Official release

AAWSAP DIRD, High-Frequency Gravitational Wave Communications, April 2010

U.S. Department of War · 2010-04-06 · 57 pages · text from the file's own layer

This Defense Intelligence Reference Document, DIA-08-1004-005, is dated 6 April 2010. The Defense Intelligence Agency's Defense Warning Office prepared it under the Advanced Aerospace Weapon System Applications program. It reviews proposed laboratory generators and detectors for high-frequency gravitational waves. It favors a piezoelectric approach for proof-of-concept tests, IR-excited molecules for an operational transmitter and the Li-Baker detector as the receiver. It estimates about 1.9 million bits per second over 7,000 km through the Earth and discusses timing standards and interplanetary navigation uses.

From the source: Release of 2026-09-18 Incident: 4/6/10, Las Vegas, Nevada. Released with redactions. This document is a Defense Intelligence Reference Document (DIRD), a technical reference format used by the Defense Intelligence Agency (DIA) to capture baseline knowledge on a specific topic for later analytic use. DIRDs are best understood as reference and synthesis products rather than as original research. It is one of 38 DIRDs produced under the Advanced Aerospace Weapon System Applications Program (AAWSAP) between 2009 and 2011. Because AAWSAP’s scope permitted a broad range of supporting topics, not every DIRD in the series directly concerns aerospace systems or future threat assessment. The following summary reflects the DIRD’s scope and framing at the time of writing and should not be read as implying current validation of the concepts discussed. This DIRD examines whether high-frequency gravitational waves could serve as a communications medium while avoiding the attenuation that limits radio-frequency systems. The report surveys proposed transmitter and detector concepts, argues that gravitational-wave communications could support secure point-to-point links, timing standards, and interplanetary navigation, and gives particular attention to laboratory generator concepts and the Li-Baker detector as possible building blocks for such a system. The document makes clear, however, that the entire concept depends on capabilities that had not been demonstrated in practice, including laboratory-scale generation and reliable detection of usable high-frequency gravitational-wave signals. It is an exploratory systems-oriented review built around a future communications concept.

UNCLASSIFIED//EOR OEEICI0L Llili QI\IL¥
1964), the gaser consists of a long rod of a material and microscopic parts of which can
be excited by a means, such as electromagnetic (EM) radiation, to emit HFGWs. They
utilize linearized theory to treat the interaction of a gravitational field with matter:
"Application is made to the emission ... of gravitons by microscopic systems such as
molecules and nuclei." Grishchuk and Sazhin in early 1974 discussed the emission of
gravitational waves by an electromagnetic cavity. In August of 1974 Chapline, Nuckolls
and Woods suggested the generation of HFGWs by nuclear explosions. In this same
regard Fontana suggested that the problem of efficient generation of HFGWs and pulses
of gravitational radiation might find a reasonably simple solution by employing nuclear
matter (Fontana and Baker, 2006; Fontana and Binder, 2009), especially isomers. A
fissioning isomer not only rotates at extremely high frequency(~ 3.03x10 24 s-1 )
according to the aforementioned references, but is also highly deformed in the first
stages of fission (the nucleus is rotating and made asymmetric "before" fission). Thus
one achieves significant impulsive forces (for example, 3.67x 108 N) acting over
extremely short time spans (for example, 3.3x 10-22 s). Alternatively, a pulsed particle
beam, which could include antimatter, could trigger nuclear reactions and build up a
coherent GW as the particles move through a target mass. The usual difficulty with
HFGWs generated by nuclear reactions is the small dimensions of their nuclear-reaction
volumes-that is, the small moment of inertia and submicroscopic radii of gyration (for
example, 10-16 m) of the nuclear-mass system. Such a difficulty is overcome by utilizing
small clusters of nuclear material, whose nuclear reactions are in synchronization; for
example, through the use of a computer controlled logic system. Such nuclear
energized HFGW generators are currently very theoretical. Braginsky and Rudenko
(1978) discussed the generation of gravitational waves in the laboratory and proposed
a means utilizing small particles In 1981 Romero and Dehnen analyzed the generation
of gravitational radiation in the laboratory also utilizing a linear array of piezoelectric
crystals that will be analyzed in more detail in Section 2.1.3. In 1988 Pinto and Rotoli
presented a paper on the laboratory generation of gravitational waves at the Italian
Conference on General Relativity and Gravitational Physics. Another Italian, Giorgio
Fontana (1998), suggested that the possibil ity of emission of high frequency
gravitational radiation from junction between d-wave and s-wave superconductors.
Kraus (1991) proposed that gravitational-wave communication might be possible in the
IEEE Antennas & Propagation magazine. At the first HFGW Working Group Conference
at the MITRE Corporation in 2003, Grishchuk analyzed electromagnetic generators and
detectors of gravitational waves. At that same Conference Valentin Rudenko presented
a paper on the optimization of parameters of a coupled generator-receiver for a HFGW
Hertz experiment. At the second HFGW Working Group Conference in Austin, Texas, in
2007, Kolosnitsyn and Rudenko presented another paper on the generation and
detection of the high-frequency gravitational radiation in a strong magnetic field. In
2007, and more recently this year, a new type of HFGW generator/detector and mirror
system based on thin, type I superconducting films was proposed by R. Chiao, S.
Minter, and K. Wegter-McNelly (2007; 2009a,b). Therefore it is evident that a number
of devices for the laboratory generation of HFGWs have been proposed including the
aforementioned gaser (as has been mentioned, was first proposed by Halpren and
Laurent in 1964, some 45 years ago) discussed by Fontana and Baker (2003); as well
as an actual laser generator of HFGWs as discussed by Li and Li (2006). Finally a rather
practical laboratory HFGW generator, which may be appropriate for the initial proof-of
concept test, is one utilizing off-the-shelf components such as magnetron energized
piezoelectric crystals or Film Bulk Acoustic Resonators or FBARs has been analyzed in
Woods and Baker, (2005) and Baker, Woods and Li (2006).
UNCLASSIFIED/ /FOR OEEICIJ.b HSI!! Dflti
4

Not linked to a story yet.

About this file

Official release, from the pursue 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.