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Add enough antifreeze and the water in your car's
cooling system will keep on flowing through the iciest
winter. Applying basically the same idea, say NCSA
physicists David Ceperley and M. Carmen Gordillo, you
can prevent hydrogen from freezing into a solid as it
usually does at low temperatures (below 14° Kelvin).
Their simulations show, furthermore, that when it gets
even chillier (1.2° K) this unfreezable liquid
hydrogen shifts to the strange, frictionless state of
matter known as superfluidity.
Their work (reported in Physical Review Letters, 20
Oct. 97) opens new avenues for research in
condensed-matter
physics by adding hydrogen to the exclusive
list of substances that become superfluid. At the top
of this list is helium, which has been a focal point
of research into low-temperature properties of matter
since it was first liquefied in 1908.
Since hydrogen is in many fundamental respects
similar to helium, physicists speculated for years
that hydrogen should be a candidate for superfluidity.
Hydrogen molecules, however, attract each other more
strongly than do helium atoms and normally combine at
low temperatures to form a solid. Ceperley and
Gordillo surmised that adding impurities to liquid
hydrogen would suppress this molecular urge to get
together and solidify. "It's so close to becoming a
liquid," says Ceperley, "if we could just make the
liquid more stable, then maybe it could become a
superfluid."
Simulations on NCSA's HP-Convex Exemplar confirmed
this insight. With an exact quantum approach that
Ceperley derived from 1950s work by Richard Feynman,
the researchers modeled hydrogen molecules on a flat
surface salted with potassium atoms. The repulsive
effect of the alkali-metal stops the hydrogen
molecules from combining to freeze into a solid,
explains Ceperley, and the liquid hydrogen undergoes a
transition to superfluidity just above absolute zero.
Liquids that flow without friction
Although a number of this century's outstanding
physicists have contributed to the understanding of
superfluidity, it remains one of the fascinating
phenomena of physics. No one knew there was such a
thing until early liquefied helium experiments by the
Dutch physicist J. Kamerlingh Onnes. In 1910 he found
that helium wouldn't freeze even at one degree above
absolute zero -- as cold as he could go -- and
measurements showed, strangely, that as liquid helium
declined in temperature its density peaked at 2.2° K.
Later studies by Dutch, Canadian, and Russian
physicists, including the noted theorist Lev Landau,
identified this density maximum as a transition to a
special state, which by the late 1930s was called
superfluidity.
Experiments show that superfluid helium has no
viscosity and flows through even the tiniest capillary
tubes with no resistance. Perhaps the most striking
demonstration of superfluid defiance of the ordinary
is its behavior in a rotating container. Put a cup of
coffee on a turntable and the coffee rotates with the
cup. Place liquid helium above superfluid temperature
inside a rotating container, explains Ceperley,
and it acts like the cup of
coffee. As you cool it through
the superfluid transition, however, the liquid stops
rotating and comes to rest. That's the lower-energy
state that superfluids get into. They completely
insulate themselves from what's going on around them."
Landau and others recognized these strange
behaviors as quantum phenomena occurring at an
observable scale. "It's a manifestation at the
macroscopic level of the fact that the quantum
particles are indistinguishable," says Ceperley.
Instead of moving independently, like the atoms of a
liquid normally do, atoms of superfluid helium cohere
in a collective state. The effect is similar to a
laser beam, notes Ceperley, in that in both cases --
photons from the laser and helium atoms or hydrogen
molecules -- the quantum particles are bosons, particles
with integral spin. "The physical effect is that the
more there are in a particular state, the more want to
go into that state."
Superfluidity also bears similarities to its better
known first cousin, superconductivity, another
macroscopic realization of quantum effects. "If you
try to put a magnetic field on a superconductor, you
can't," says Ceperley. "It pushes out the magnetic
field. It's like rotation to a superfluid." Similarly,
as it's possible to establish current in a
superconducting circuit that will flow forever,
superfluid helium can be made to flow in a loop, a
"superflow" that continues as long as superfluid
conditions are maintained.
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Line dancing in imaginary time
To accurately simulate the exotic properties of
superfluid helium and to test their hypothesis about
hydrogen, Ceperley and Gordillo used a computational
approach, path-integral Monte Carlo (PIMC)
calculations, which Ceperley developed as an extension
of work by Nobel Prize-winning American physicist
Richard Feynman. "Feynman provided the first
satisfactory theoretical explanation of superfluids,"
says Ceperley, "and he introduced the idea of
imaginary time path-integrals."
In the 1950s, Feynman's ideas were limited by
computational technology. Ceperley developed PIMC into
a practical numerical algorithm for calculating
superfluid properties: "Essentially, Feynman showed
that this quantum system is equivalent mathematically
to a classical system of exchanging polymers. The
thermodynamic properties -- energy, pressure and
superfluid properties -- have exact equivalents in the
classical domains, and the PIMC simulation translates
from one domain to the other. There are many
refinements needed to make it effective on computers,
and that's what we developed."
The method relies on a simple mathematical
transformation -- changing time in Schrödinger's
equation, the fundamental equation of quantum
mechanics, to imaginary time. "You can only do these
calculations -- many-body quantum calculations in
imaginary time -- so we have to make a virtue of
necessity." The calculations trace the particles as
they move in imaginary time and, like a game of
musical chairs, they must either return to their
starting place or the starting place of another
particle.
In this formalism, says Ceperley, it turns out that
superfluidity is equivalent to what happens if you
progress from one position to the next in a line
dance. "It takes a long time to get back to where you
started. If the line is 20 couples long, it takes 20
iterations. That's the property we look for -- it's
called a permutation of labels -- an exchange that
extends across the system. If you look at those paths,
you'll see they're all linked together, like one huge
molecule, and that's superfluidity, in this imaginary
time."
Looking ahead
Ceperley and Gordillo's result with simulated
hydrogen and alkali-metal atoms suggests an obvious
direction for experimental work, and several research
teams are expected to try to confirm their finding of
superfluid hydrogen. In future simulations, they'll
refine their calculations of hydrogen superfluidity
and address the possibility of hybrid superfluids such
as mixtures of helium and hydrogen.
As part of the effort of the Alliance, they will
also work to forge PIMC into a generalized
computational tool. "We hope that eventually PIMC can
be a 'black box,' " says Ceperley. "A nonexpert could
specify temperature, particle masses, spins,
interactions, chemical potentials, and boundary
conditions of the quantum system, and the computer
could return estimates of various observables,
complete with error bars. It should be a major goal of
computational many-body physics to show how this can
be done."
References:
M. C. Gordillo & D. M. Ceperley,
"Superfluidity in H2
Films," Physical Review Letters 79, 3010 (1997).
D. M. Ceperley & M. C. Gordillo, "Conditions of
Superfluidity in Molecular Hydrogen," Proceedings of
the International Workshop on Condensed Matter
Theories, v. 12, ed. J. W. Clark, P. V. Plant (Nova
Science, New York: 1997).
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