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Nuclear Isomer Decay: A Possibility for Breakthrough Space
Radsafers,
The below fascinating abstract is about inducing gamma decay as a deep space
propulsion method.
Can anyone explain:
How can isomeric transition be triggered?
How can the resulting gamma rays be made to go in one direction so as to
produce propulsion. I thought the direction of gammas must be isotropic.
Regards,
Wes
--
Wesley R. Van Pelt, Ph.D., CIH, CHP KF2LG
President, Van Pelt Associates
Radiation Safety and Environmental Radioactivity
mailto:vanpeltw@idt.net http://idt.net/~vanpeltw/
Title: Nuclear Isomer Decay: A Possibility for Breakthrough Space
Propulsion
Document ID: 19990023229
Report #: None
Sales Agency: CASI Hardcopy A01
CASI Microfiche A04
No Copyright
Authors: Carpenter, Phillip A. (Oak Ridge Operations Office)
Gat, Uri (Oak Ridge National Lab.)
Journal: NASA Breakthrough Propulsion Physics Workshop Proceedings,
Page: 217-220
Published: 19990101
Source: Oak Ridge National Lab. (TN United States)
Pages: 4
Contract #: DE-AC05-96OR-22464
Abstract: A novel propulsion system for deep space missions that
utilizes accelerated decay of nuclear isomers via induced
gamma emission is proposed. The propulsion is accomplished
by ejection of gamma particles resulting from controlled
nuclear isomeric decay. The specific impulse per unit mass
is comparable with that of chemical-thermal sources;
however, the specific energy comparison on the same basis
is about five orders of magnitude higher. It is expected
that the nuclear isomers can be recharged while in space by
gamma rays to "pump-up" the isomers. A prime candidate for
this application is the isotope Hf-178. The nuclear
isomeric transition is a transition of an excited nucleus
to its ground state by release of energy as gamma
particles. The accelerated nuclear decay is accomplished by
further exciting the isomer so that the degree of
forbiddenness of transition to the ground state is reduced
and occurs rapidly. The recharging is done by supplying
energy in quantities that recreate the decay inhibited
state. The rechargeability of the isomers in space makes
accelerated nuclear decay attractive for long space
missions. It may be possible to collect gamma rays while
traveling in space to recharge the isomers. Further, it is
possible that with controlled releases, the non-propulsion
energy requirements of the spacecraft can also be met.
Onboard power could be provided through the controlled
release of gamma rays (i.e., photons) which can be
converted to electricity via photoelectric or other effect.
On long trips, gathered energy from space can be used for
continued acceleration for about the first half of the trip
and then for deceleration for the remaining half of the
trip. The photons momentum provides the propulsion
momentum. This concept is akin to the early light-sail
(i.e., photon pressure propulsion) concepts as proposed,
for example, by Dr. Robert L. Forward in the 1970s, and
earlier by others. The major initial development areas
proposed are: verification and confirmation of the
principles; establish theory and develop physical control;
quantitative control of energy and impulse release;
direction and collimation of the release; development of
the recharge ("pump-up") mechanism of the isomers and the
controlled triggering of release(s); concept definition of
applications as propulsion; and as an onboard energy
storage and generation source.
Language: English
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