Documents / Report
This Defense Intelligence Reference Document from the Defense Intelligence Agency is dated 3 January 2011. It was produced under the Advanced Aerospace Weapon System Applications (AAWSA) Program as part of a series of advanced technology reports. The report asks whether negative mass exists and whether it could be used for propulsion. It concludes that one route might be an ultra-light form of matter that could have gathered at the Moon's center. Reaching it would take a tunnel dug with thermonuclear shape charges.
“The Times”16 pages
UNCLASSIFIED/ ,'P81l 8PPll!lllit tl!II!! t!IHLY The mass density (14) is not fictitious but represents physical reality. According to Einstein's E = mc2 one obtains for an electric field Ethe mass density (15) Replacing f:o with -(1/y), one obtains the energy density of the gravitational field (16) It possesses the (negative) mass density (17) Besides the field g, we have on a "merry-go-round" the Coriolis force field G~2cw (18) By setting G = g and inserting G into (17) with g2 = G2, one obtains the mass density (14). This means the centrifugal force is the gravitational force associated with the mass density of the Coriolis field. But where is this huge negative mass coming from? The obvious answer is by the very large vacuum energy, making itself felt by going to an accelerated frame of reference. In Mach's principle the motion of the distant galaxies as seen in an accelerated frame of reference is responsible for the inertial forces. But this idea is wrong because if by some miracle the distant galaxies were to be set into motion, it would take a long time before their fields propagating with the velocity of light would reach the earth. Adding the mass of the Coriolis field to the right side of the equation (12), we have by putting it on the left hand side d - F I G' 4IV --. =- llYP. 2c" (19) 7 UNCLASSIFIED/ ,'1'81l 8PPll!lllit tl!II!! 8HLV
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Report, from the dia collection. The PDF is mirrored here; the original link is under it. 43 pages are in the text index: search them above, or from the library's search.