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AAWSAP DIRD, Traversable Wormholes, Stargates, and Negative Energy, April 2010

U.S. Department of War · 2010-04-06 · 42 pages · text from the file's own layer

This Defense Intelligence Reference Document, DIA-08-1004-004, is dated 6 April 2010. The Acquisition Support Division of the Defense Intelligence Agency's Defense Warning Office prepared it as one in a series of advanced technology reports from FY 2009 under the Advanced Aerospace Weapon System Applications Program. It reviews the physics of traversable wormholes and flat-faced "stargate" solutions, and it covers how negative energy might be generated in the laboratory. It concludes that the key technical challenge is identifying and producing exotic matter.

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 traversable wormholes and “stargates” as hypothetical spacetime structures within general relativity that theoretically offer a means of faster-than-light travel or communication. The report focuses extensively on the requirement for exotic, negative-energy matter to stabilize and keep such geometries open for the passage of macro-scale objects. It reviews standard wormhole models, describes a flat-throated “stargate” variant, and argues that violations of general relativity's standard energy conditions do not physically rule such structures out, citing microscopic, transient negative-energy effects observed in Casimir-type laboratory phenomena. However, the document acknowledges that the transition from microscopic quantum fluctuations to macroscopic engineering is an unresolved barrier. While small-scale negative-energy effects are observable, there is no known mechanism to generate, concentrate, or stabilize the amounts of exotic matter proposed to be required to sustain a traversable macroscopic wormhole. Ultimately, while the paper frames wormhole concepts within accepted relativistic physics, it confirms that the gap between theoretical models and any realizable technology remains enormous.

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matter, and many other fascinating properties (Reference 22-24, 26, 73-76).
Therefore, if the emergent spacetime/gravity approach turns out to be correct, then
there will likely be a direct consequence to the physics of traversable wormholes that
could dramatically alter the mechanism by which they are created and/or mitigate the
requirement for negative energy.
Until such new approaches are established and testable predictions published by their
proponents, one cannot specu late on how the physics of traversable wormholes will be
affected. Therefore, it is beneficial to stick to the outcome of the present study in terms
of quantum field theory and general relativity theory, and outline what needs to be
accomplished going forward in order to demonstrate a traversable wormhole in the lab.
Going forward toward the demonstration of a t raversable wormhole will require the
following:
• Generating Negative Energy in the Lab: Our assessment concludes that we already
make small amounts of negative energy in the lab, but we do not yet know if we can
access larger amounts for extended periods of time over extended spatial
distributions for the purpose of engineering a traversable wormhole . In this regard
we propose the following options for further exploration.
• Squeezed quantum vacuum generators: A dedicated research program to develop
the two negative energy generator concepts described in Section 111-B-2 will need to
be established in order to evolve state-of-the-art quantum optics technology
towards producing higher magnitudes of negative energy as well as special
techn iques required to separate out any positive energy fluxes that accompany the
negative energy fluxes. Specifically, the Rabeau et al. (Reference 48, 49) and Ries
et al. (Reference 50) experimental programs should be followed as a template
toward this goal. Quantum optics technology via high power fiber lasers, resonators,
amplifier stages, beam conditioning stages, etc., are rapidly advancing. So research
should be conducted in parallel to invent add itional ways to produce negative energy
via innovative quantum optics.
• Casimir effect: Even though the standard electromagnetic Casim ir effect is feeble,
and thus not likely to contribute to a traversable wormhole engineering program,
there are still a number of other electromagnetic and non-electromagnetic Casimir
effects described in Section 11I-B-4 that require further study. These other Casimir
effects have not been explored with an eye toward testing them in the lab, and so
there could be important new information yet to be uncovered.
• Moving Mirrors (a.k.a. the dynamical Casimir effect): Even though this concept was
identified (Section I11-B-5) as being too feeble to produce any useful flux of negative
energy, the observable effects due to the change in the boundary conditions (e.g .,
moving mirrors/cavity walls) of quantum fields provide crucial information on the
quantum vacuum at the macroscopic level. Theoretical and laboratory efforts are
underway to understand the dissipative effects of vacuum fluctuations (Reference
77-78). This dissipation mechanism should induce irradiation of photons, a
phenomenon also known as the dynamical Casimir effect. This can be understood
both as the creation of particles under non-adiabatic changes in the boundary
conditions of quantum fields, or as classical parametric amplification with the zero
point energy of a vacuum field mode as an input state. More recent developments
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Official release, from the pursue collection. The PDF is mirrored here; the original link is above. 42 pages are in the text index: search them above, or from the library's search.