DOW-UAP-D123, AAWSAP DIRD, Positron Aerospace Propulsion, March 2010

53
⬇ Download HD (37.8 MB)
SHARE Reddit X Facebook HN Email
Agency
DoD
Category
military
Type
PDF
Event Date
3/2/2010
Size
37.8 MB
Original Filename
DOW-UAP-D123_AAWSAP-DIRD-Positron-Aerospace-Propulsion-March-2-2010.pdf
Location
Las Vegas, Nevada
Status
REDACTED

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 positrons as a possible fuel for advanced aerospace propulsion, arguing that antimatter offers extraordinary energy density and could, in principle, support applications ranging from long-endurance aircraft and missiles to single-stage launch vehicles, onboard power systems, and crewed Mars missions. At the same time, it makes clear that the concept depends on resolving major unsolved problems in producing positrons in sufficient quantities and storing them safely for long periods, and much of the document’s discussion of flight systems and Mars missions remains conceptual rather than closely tied to demonstrated engineering practice. Its overall conclusion is that positron propulsion is theoretically attractive, but remains highly speculative as a practical technology because its core production and storage requirements remain unsolved.

The summary above is sourced from the released file metadata as published to war.gov. The analysis sections below are original to this tracker.

Text of the document

Machine-extracted from the PDF war.gov published (its text layer or OCR), so expect errors, especially in names, numbers and handwriting; the PDF is the authoritative copy. Lines that did not extract as readable text are left out. Showing about 998 words from pages 2, 3, 4, 5, 6, 7 of 35.

PAGE 2

UNCLASSIFIED//POI\ OFFICIAL USE Oiltt Positron Aerospace Propulsion Prepared by: Acquisition Support Division (DW0-3) Defense Warning Office Directorate for Analysis Defense Intelligence Agency AAP Person 69 Administrative Note COPYRIGHT WARNING: Further dissemination of the photographs in this publication is not authorized. This product is one in a series of advanced technology reports produced in FY 2009 under the Defense Intelligence Agency, Defense Warning Office's Advanced Aerospace Weapon System Applications (AAWSA Pro ram. Comments or uestions pertaining to this document should be addressed to AAP Person 1 , AAWSA Program Manager, Defense Intelligence Agency, ATTN: CLAR/DWO-3, Bldg 6000, Washington,

PAGE 3

Positron Air-Breathing Propulsion.......................................................................... 2 Unmanned Aerial Vehicle (UAV) ......................................................................... 5 Ramjet-Assisted Missile (RAM) .......................................................................... 7 The Solid-Core Positron Rocket ........................................................................ 12 The Gas-Core Positron Rocket .......................................................................... 14 The Sanger Photon Positron Rocket ................................................................. 16 Positron Rocket System Comparison ................................................................ 17 Positron Energy Conversion for Onboard Power............................................... 18 Positrons for a Manned Mars Mission ................................................................... 19 Positron Production.............................................................................................. 22 Formation of Positronium in Porous Media ....................................................... 25 Long-Term Storage of Positronium .................................................................. 25 Figure 1. Specific Energy for Chemical, Nuclear and Antimatter Materials............. 1 Figure 2. Tory-IIC Ready for Testing ...................................................................... 3 Figure 3. PTRE Turbojet and Turbo-Ramjet Modes ................................................. 3 Figure 4. Details of the PTRE Engine.......................,............................................... 4 Figure 5. Combustion Turbo-Ramjet....................................................................... 4

PAGE 4

UNCLASSIFIED/J FOR OFFICIAL USE ONLY Figure 8. BOMARC and Talos Ramjet-Assisted Missiles........................................... 8 Figure 10. Artist's Rendition of a Four-Engine Positron SSRV............................... 11 Figure 11. Solid-Core Positron Rocket Engine With a Hot-Bleed Configuration..... 12 Figure 13. Modified Sanger Photon Rocket Concept ............................................. 17 Figure 14. Closed Brayton Cycle Using Positron Annihilation ............................... 18 Figure 15. Conceptual 110 Watt Positron Closed Cycle Generator Based on the NASA Glenn Research Center Stirling Radioisotope Generator (SRG) .. 18 Figure 16. Mars Trajectories (X-Coordinates Defined in Direction of Aries) ......... 20 Figure 17. Spacecrafts Using Positron Engines..................................................... 21 Figure 18. Proposed Undulator-Based Positron Source for the International Figure 22. TEM of Silica Aerogel ........................................................................... 26 Table 4. Comparison of Space Propulsion and Power Systems - Solid Core ......... 13 Table 5. Comparison of Three Positron Propulsion Concepts for Mars Mission ..... 17 Table 6. Positron and Antiproton Expected Costs in the Next 10 Years ................ 23

PAGE 5

Positron Aerospace Propulsion Antimatter is considered an extremely attractive fuel for aerospace propulsion because of its enormous advantage in energy density over all other known sources of energy. However, because antimatter does not occur naturally and is unstable in the presence of matter, no vehicles have ever flown using it. After a short overview of the various aerospace applications of antimatter, this paper provides a detailed analysis of air-breathing turbojets and turbo-ramjet missiles, as well as rockets for manned interplanetary missions. It discusses new methods of producing and storing large numbers of antielectrons, or positrons, and compares their costs with those of antiprotons. Finally, the paper considers the prospects for the first, modest demonstration of positron propulsive flight within the next 10 years. Interplanetary missions on positron-propelled spaceships are described in detail, with estimates of positron requirements for each mission. Standalone positron power systems are described briefly. Studies of positrons as a fuel for aerospace propulsion applications have been sponsored by the Air Force Research Laboratory, Eglin Air Force Base, Florida, and the NASA Institute for Advanced Concepts, Atlanta, Georgia. This paper is an anthology of that work and not a general review of antimatter propulsion. The positron was predicted by Dirac in 19291 and discovered by Anderson in 1932.2 Along with the antiproton, which was discovered in 1954,3 the positron has the largest specific energy of any known material. Because aerospace propulsion performance is ultimately limited by specific power, this advantage was immediately appreciated. However, compared with chemical sources of energy, positrons presented new and serious production and storage Antimatter has a long history of appearing in science fiction literature, dating to a 1942 short story in Astounding Science Fiction and the 1949 book Seetee. It later appeared in the Star Trek television and film series and continues to be an appealing subject for contemporary books and films, such as Angels and Positron aerospace propulsion is now entering a critical period owing to new technologies that bear on production and storage issues. To their advantage, positrons, unlike nuclear fission and antiprotons, present no radiation or environmental safety problems.

PAGE 6

Antimatter appears in the form of fundamental particles that have their sign of electric charge reversed from their matter counterpart. For example, the positron, e+, is the antiparticle to the electron, e·. According to the CPT theorem,4 properties of matter and their counterpart antimatter particles are identical. This has been tested in the laboratory to an accuracy of roughly 1 part in 10 million. Antimatter is appealing for aerospace uses because its specific energy by annihilation is 180 MJ/µg, or 10 orders of magnitude larger than chemical energy, as shown in Figure Olerrical Fission Fusion Fbsitron Figure 1. Specific Energy for Chemical, Nuclear, and Antimatter Materials In the presence of matter, the positron binds with an electron to form a short-lived atom called positronium (Ps). Depending on the relative spin orientations of the positron and electron, Ps has a mean lifetime in a vacuum of 125 picoseconds (para-Ps, spins antiparallel), or 142 nanoseconds (ortho-Ps, spins parallel). From quantum number conservation, para-Ps decays into two gamma rays of equal energy, 511 kiloelectronvolts (keV), whereas ortho-Ps decays into three gamma rays whose energies add up to 1022 keV. Hence, when Ps self-annihilates, there is 100 percent conversion of mass into electromagnetic energy given by Einstein's famous equation, E = mc2, where c is the speed of light. Although the energies of positron annihilation gamma rays are on the nuclear scale, they have none of the undesirable features associated with nuclear energy. First, the annihilation evolves rapidly (nanoseconds) and is controllable under predictable electromagnetic forces. There is no long-term inertia as with nuclear reactors. Consequently, positron-generated thrust can be throttled.

PAGE 7

Second, low-energy gamma rays from positron annihilation cannot make residual radioactivity in surrounding air and containment vessels. In contrast, antiprotons

Where this file fits in the PURSUE archive

This file is one of DoD's 282 files in the Trump PURSUE disclosure. Within the DoD agency block it ranks #239 of 282 by Anomalousness Index. Across the entire 478-file archive it ranks #414 of 478.

That places it in the lower-scoring band of the archive (414 of 478 by score), typical of investigative-record style files where the report is paper-based rather than instrumented.

Anomalousness Index: 53/100

This is a reference document, not an encounter report, so the index has no encounter to measure here. The value above is the rubric's default for a document that describes no event, shown so every file in the archive can be ranked the same way. Not a probability of extraterrestrial origin - that number is not honestly computable from the released files and this tracker refuses to publish it.

🤖 AI-ASSISTED SCORING · methodology

The six rubric components break down for this file as follows. Each component has a weighted contribution to the final score; the per-component explanation below describes what this file's particular value on that component means in the rubric's framework.

sensor quality (eyewitness only) 30 × 0.25 = 7.5

This file is a reference document, not an observation, so no sensor, camera, or witness captured anything. The rubric's sensor axis has no not-applicable option, so a document with no instrument record sits on its lowest tier by default.

witness credibility (military personnel) 80 × 0.2 = 16.0

There is no witness: this is a document released by the Department of War, not a first-hand account. The rubric assigns this axis from the originating body, so the value reflects the source of the record, not anyone's testimony.

corroboration (single witness instrument) 60 × 0.2 = 12.0

Nothing is being corroborated, because the file does not report an event. Like every file in the archive it takes the rubric's single-source default.

kinematic anomaly (no kinematic data) 30 × 0.15 = 4.5

The file describes no object and no motion, so the kinematic axis takes the archive-wide 'no kinematic data' default.

mundane explanation available (weak mundane candidate) 70 × 0.1 = 7.0

Every file in the archive scores this tier. For a document that describes no event it carries no information about the record at all.

official disposition (unresolved no review) 60 × 0.1 = 6.0

The rubric's default for the file's release status (files released with redactions are catalogued as unresolved, unredacted ones as open). For a document that reports no event this describes how the file was released, not anything that happened.

Bottom line on the score: the 53/100 is the rubric's default for a document that reports no encounter, so it is not a finding about any event and should not be compared with the scores of sighting reports. For the full per-axis weights and the rubric JSON, see /methodology.

Related files in DoD

Other PURSUE files in the same category, ranked by Anomalousness Index.

DoD · VIDEO SCORE 68

DOW-UAP-PR024, Unresolved UAP Report, Middle East, 2023

DoD · VIDEO SCORE 68

DOW-UAP-PR072, "ADMINISTRATIVE REVISION: IIR 1777 J0032 22 Kazakhstan - UAP in the vicinit…

DoD · VIDEO SCORE 68

DOW-UAP-PR106, Unresolved UAP Report, Eastern United States, 2020

DoD · VIDEO SCORE 68

DOW-UAP-PR108, Unresolved UAP Report, Western United States, 2020

DoD · VIDEO SCORE 68

DOW-UAP-PR109, Unresolved UAP Report, Eastern United States, 2015

DoD · VIDEO SCORE 68

DOW-UAP-PR110, Unresolved UAP Report, Eastern United States, 2020

BROWSE ALL 478 FILES →

Verification

SHA-256:

96294b90e769ff43e4153438331153aa62fb01bc4345af61647fa06503801b82

This hash is the SHA-256 of the file body war.gov served on the verification date above. War.gov has re-processed some file bodies since first release (re-compression + OCR, no content removed - see /changes); we re-verify and record the change rather than silently serve a stale hash. How to check this yourself →

Source: https://www.war.gov/medialink/ufo/sept-18/release-06/assets/DOW-UAP-D123_AAWSAP-DIRD-Positron-Aerospace-Propulsion-March-2-2010.pdf

📡 Subscribe via RSS 🔔 Watch on GitHub