Number 719 #2, February 10, 2005 by Phil Schewe and Ben Stein
Liquid Carbon Chemistry
The chemistry of carbon atoms, with their
gregarious ability to bond to four other atoms, is a major
determinant of life on Earth. But what happens when carbon is
heated up to its melting temperature of 5000 K at pressures greater
than 100 bars? Although liquid carbon may exist inside the planets
Neptune and Uranus, the main interest in studying liquid carbon here
on Earth might be in the indirect information provided about bonding
in ordinary solid carbon or in hypothetical novel forms of solid
carbon A new experiment creates liquid carbon by blasting a solid
sheet of C with an intense laser beam. Before the liquid can
vaporize, its structure is quickly probed by an x-ray beam. At low
carbon density, two bonds seem to be the preferential way of hooking
up, while at higher density, three and four bonds are typical.
This is not to say that complex organic molecules (carbon bonded to
other atoms such as hydrogen or oxygen) could survive at 5000 K, but
carbon bonds are tougher and can persist. The experiment was performed
by physicists from UC Berkeley, the Paul Scherrer Institute (PSI) in
Switzerland, Lawrence Berkeley National Lab, Kansas State, and Lawrence
Livermore National Lab. A team member, Steve Johnson (steve.johnson@mailaps.org),
says that one next step will be to study carbon, as well as other materials,
at even higher temperatures in order to look at "warm dense matter,"
a realm of matter too hot to be considered by conventional solid-state
theory but too dense to be considered by conventional plasma theory.
(Johnsonet al., Physical Review Letters,11 February 2005; lab website
at http://www.physics.berkeley.edu/research/falcone/ )