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AAWSAP DIRD, Quantum Tomography of Negative Energy States in the Vacuum, January 2011

U.S. Department of War · 2011-01-11 · 51 pages · text from the file's own layer

This Defense Intelligence Reference Document, dated 11 January 2011, was prepared by the Defense Intelligence Agency's Defense Warning Office under the Advanced Aerospace Weapons System Applications program. It reviews negative, or sub-vacuum, energy found in the Casimir effect and squeezed light, and describes quantum optical homodyne tomography for measuring it. It proposes balanced homodyne detector systems to map negative energy. It also suggests that arrays of such sensors could detect anomalous aerospace platforms that use engineered spacetime effects for propulsion.

From the source:Release of 2026-09-18 Incident: 1/11/11, 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 how negative-energy, or “sub-vacuum,” states in quantum fields might be detected and mapped. Its practical scope is limited to the laboratory-scale measurement of minute quantum effects, though it extrapolates from those effects to consider theoretical relevance to concepts such as warp drives, wormholes, or gravitational control. By reviewing previously identified laboratory examples such as the Casimir effect and squeezed light states, the report identifies the core technical challenge as mapping their spatial and temporal structures reliably. To address this, it proposes quantum optical homodyne tomography as a method to reconstruct and quantify the vacuum fluctuations associated with these states. The document acknowledges that only microscopic, transient negative-energy effects have been realized in laboratory settings. It remains unknown whether larger or longer-lived distributions of such effects can be generated or stabilized, particularly given the experimentally unresolved constraints imposed by quantum inequalities. Overall, this DIRD functions as a measurement- and diagnostics-oriented review intended to lay experimental groundwork for a far more ambitious, highly speculative negative-energy research agenda.

UNCLASSIFIED/ /FOR &FFl&IAk l:ISE &HkV
Figure 14. Experimentally Measured Squeezed State. (courtesy of P.
Marecki) This graph of vacuum dB noise vs . relative optical phase angle shows
an experimentally measured squeezed state (plot (I)) and a normal
(undisturbed) vacuum state (plot (II)). The deep valleys with negative dB
values in plot (I) are sub-vacuum regions with sub-vacuum (negative) energy
density (see also, Figure 1 for a comparison) .
When applied to pulsed sources, the frequency-domain BHD techn ique implies that
averaging over many individual laser pulses takes place. However, in time-doma in BHD,
each laser pu lse generates a signal that is observed in real time and yields a single
value of a field quadrature. Repeated measurements of a large number of laser pulses
produce a quantum probability distribution associated with th is quadrature . When
transform-limited LO pulses are used, time-domain BHD gives the complete information
about the quantum state in the spatial-temporal mode that matches that of the LO.
Hansen et al. [4] point out that time-domain BHD is technically challenging, because 1)
the electronics must ensure time resolution of individual laser pu lses and 2) the
measured quadrature values must not be influenced by low-frequency noise. The
detector must provide ultralow noise, high subtraction, and a flat amplification profile in
the entire frequency range from DC to at least the LO pulse repetition rate. See
Reference [4] for a comp lete description of their device as shown in Figure 13.
UNCLASSIFIED/ /EOA OFFIGIAk l:ISE 8HLY
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Official release, from the pursue collection. The PDF is mirrored here; the original link is above. 51 pages are in the text index: search them above, or from the library's search.