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Defense Intelligence Reference Document Advanced Nuclear Propulsion For Manned Deep Space Missions

Defense Intelligence Agency · 37 pages · text from the file's own layer

This Defense Intelligence Reference Document from the Defense Intelligence Agency, dated 11 March 2010, was produced under the Advanced Aerospace Weapon System Applications (AAWSA) Program. It argues that spaceships powered by deuterium thermonuclear reactions could be built with current science and technology. The paper covers ignition by GeV proton beams, magnetic insulation, the Super Marx generator and conjectured chemical superexplosives, and it concludes that such craft could make manned exploration of the entire solar system possible.

  • p. 2 …2009 Advanced Aerospace uestions pertaining to AAWSA Program Bldg 6000, Wash;ngton, under the Defense Intelligence…
  • p. 5 UNCLASSIFIED/ «F&A 8FFI~IIP 1!55 0111 YI Advanced Nuclear Propulsion for Manned Deep Space…
  • p. 7 …to the Einstein gravitational lens focus is likely to be needed, possible only with advanced nuclear…
  • p. 16 …the Moon, nuclear propulsion is indispensible. Nuclear thermal propulsion is really not much better than advanced…
UNCLASSIFIED/ ,SF&lil: 8FFIIItliL '11815 8HL?/
• Bombardment of a solid target with beams or by hypervelocity impact, followed by a
convergent shock wave.
BOMBARDMENT OF A SOLID TARGET WITH AN INTENSE
RELATIVISTIC ELECTRON OR ION BEAM
This possibility was considered by Kidder (Reference 20), who computes a pressure of
SO Mb, if an iron plate is bombarded with a 1-MJ - 10-MeV - 106 A relativistic electron
beam, focused down to an area of 0.1 cm 2 . Accordingly, a 2-MJ beam would produce
100 Mb. Instead of an intense relativistic electron beam, one may use an intense ion
beam. It can be produced by the same high-voltage technique, replacing the electron
beam diode by a magnetically insulated diode (Reference 21).
Using intense ion beams has the additional benefit that the stopping of the ions in a
target is determined by a Bragg curve, generating the maximum pressure inside the
target, not on its surface.
HYPERVELOCITY IMPACT
A projectile with the density p :::::: 20 g/cm 3 accelerated to a velocity v = 30 km/s would,
upon impact, produce a pressure of p z 100 Mb. The acceleration of the projectile to
these velocities can be done by a magnetic traveling wave accelerator.
BOMBARDMENT OF A SOLID TARGET WITH BEAMS OR BY
HYPERVELOCITY IMPACT, FOLLOWED BY A CONVERGENT SHOCK
WAVE
If, upon impact of either a particle beam or a projectile, the pressure is less than 100
Mb (for example, only on the order of 10 Mb) but is acting over a larger area, a tenfold
increase in the pressure over a smaller area is possible by launching a convergent
shock wave from the larger area on the surface of the target onto a smaller area inside.
According to Guderley, the rise in pressure in a convergent spherical shock wave goes
as r - 0 -9 , which means 100 Mb could be reached by a tenfold reduction in the radius of
the convergent shock wave.
While it is difficult to reach 30 km/s with a traveling magnetic wave accelerator, it is
easy to reach a velocity of 10 km/s with a two-stage light gas gun.
We assume an equation of state of the form p/ p 0 = (n/n 11 Y. For a pressure of 100 Mb =
1014 dyn/cm 2 , we may set y= 3 and p 11 = 10 11 dyn/cm2, p 11 being the Fermi pressure of
a solid at the atomic number density 110 , with n being the atomic number density at the
elevated pressure p > Pn. With d = n- 113, where dis the lattice constant, one has
I I _, ''ddo=(PPn) ( 41)
Such a lowering of the inneratomic distance is sufficient for the formation of molecular
states.
28
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Report, from the dia collection. The PDF is mirrored here; the original link is under it. 37 pages are in the text index: search them above, or from the library's search.