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Thursday, April 15, 2010 - 11:59 AM
here are no known post-Big Bang processes which would produce
significant amounts of deuterium. Hence observations about deuterium
abundance suggest that the universe is not infinitely old, which is in
accordance with the Big Bang theory.
During the 1970s, there were major efforts to find processes that
could produce deuterium, which turned out to be a way of producing
isotopes other than deuterium. The problem was that while the
concentration of deuterium in the universe is consistent with the Big
Bang model as a whole, it is too high to be consistent with a model that
presumes that most of the universe consists of protons
and neutrons.
If one assumes that all of the universe consists of protons and
neutrons, the density of the universe is such that much of the currently
observed deuterium would have been burned into helium-4.
This inconsistency between observations of deuterium and observations
of the expansion rate of the universe led to a large effort to find
processes that could produce deuterium. After a decade of effort, the
consensus was that these processes are unlikely, and the standard
explanation now used for the abundance of deuterium is that the universe
does not consist mostly of baryons, and that non-baryonic matter (also
known as dark matter) makes up most of the matter mass of the
universe. This explanation is also consistent with calculations that
show that a universe made mostly of protons and neutrons would be far
more clumpy than is observed.
It is very hard to come up with that would produce
deuterium via nuclear fusion. What this process would require is that
the temperature be hot enough to produce deuterium, but not hot enough
to produce helium-4, and that this process immediately cools down to
non-nuclear temperatures after no more than a few minutes. Also, it is
necessary for the deuterium to be swept away before it reoccurs.
Producing deuterium by fission is also difficult. The problem here
again is that deuterium is very subject to nuclear processes, and that
collisions between atomic nuclei are likely to result either in the
absorption of the nuclei, or in the release of free neutrons or alpha particles. During the 1970s,
attempts were made to use cosmic ray spallation to produce deuterium. These
attempts failed to produce deuterium, but did unexpectedly produce other
light elements.
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