One of the words most frequently used to describe the state of turbulence is "ubiquitous." Turbulent flows are found not only throughout the world of nature, but throughout the world of research. The understanding of turbulence theory is essential in a range of scientific disciplines, including engineering, astrophysics, geology, and weather prediction. Turbulence is also, in the words of the legendary physicist Richard Feynman, "the last great unsolved problem of classical physics." Indeed, progress in the theory of turbulence has remained relatively stagnant for the past 30 years, while the exponential growth in computing power has allowed turbulence researchers to model turbulent flow to an extent never before dreamed possible. Mathematician George Papanicolaou, now at Stanford University, has been a major figure in the application of turbulence theory for two decades. In the mid-1970s, with Alain Bensoussan, now president of the French Institute National des Recherche Informatique et Automatique, and Jacques-Louis Lions of the College de France, Papanicolaou pioneered the mathematical study of the effective properties of materials. This concept, which has come to be known as "homogenization," has had applications in the study of composite materials and complex fluids. Papanicolaou, who describes himself as a "user of turbulence theory," has also done seminal work in the mathematical study of wave propagation in reflective seismograms and of the focusing of high intensity laser beams when they pass through inhomogenous media. Papanicolaou, 52, was born in Athens, Greece. He received his bachelor's degree in engineering at Union College in Schenectady, New York, and his master's degree and Ph.D. degree in mathematics at the Courant Institute at New York University, where he became a full professor in 1976 and, three years later, the director of the Division of Wave Propagation and Applied Mathematics. From 1990 to 1992, he was a visiting member of the Institute for Advanced Study in Princeton. In the summer of 1993, he moved to Stanford University, where he is a professor of mathematics. From his office at Stanford, Papanicolaou spoke with Science Watch correspondent Gary Taubes.
Papanicolaou: Simply, turbulence is very hard. Every hard problem in classical physics finds itself embedded in turbulence. It is nonlinear, chaotic, stochastic. And there is no separation of scalesyou must deal with a very large number of scales of irregularities. It's just a mess. In most other physics problems, you can get control by reducing them to simpler problems that you can understand. You can separate scales, for instance, and determine that certain scales are not important. You can limit the phenomena. Or perhaps the inhomogeneity, the chaotic behavior, is not there all the time, so you can somehow approach it. In turbulence all these things happen at once, and you don't know how to separate them out.
Papanicolaou: In
communication theory, for instance, turbulence theory is used to understand how radio
waves degrade by going through a turbulent atmosphere. We're interested in how radio waves
are affected by the turbulent environment. The electromagnetic waves move so fast, we can
assume that the turbulent motion is frozen. So the waves sample a frozen picture of the
turbulent atmosphere. What will happen? If the waves are very long, they're not affected
by the turbulence because the turbulence is on a finer scale. It's when the wavelengths
are comparable to the scales of turbulence in the atmosphere that you get interactions.
For the atmosphere, for example, it could be anywhere from one meter to 10 to 20
centimeters. And the shorter the waves get, the more prone they are to be scattered by
inhomogeneities.
Papanicolaou: Most of the interesting things that have happened in turbulence are empirical models that are checked computationally. Of course, the big progress since the 1960s is the ability to do numerical simulations with a computer. That's an enormous improvement. Nowadays, the kind of tedious analytical work that was being done 30 years ago has almost disappeared. Instead, people do bigger and bigger numerical simulations. A huge bank of data for turbulent flows has been generated, and people use it to test their empirical theories.
Papanicolaou: Here's a
striking thing: In 1941, Kolmogorov, the great Soviet mathematician, wrote a two-page
paper on turbulence, using very exciting physical reasoning to produce a heuristic law
that tells how energy is distributed among different scales in turbulence. In the
atmosphere, for instance, turbulence manifests itself on scales from millimeters and
centimeters to meters and maybe even tens of meters. So how much energy does each scale
carry in a typical developed turbulence? How does the energy distribute itself among the
various scales? That's a very essential question. Is there a universal law that describes
this?
Papanicolaou: Chaos theory is related to the subject of the onset of turbulence, when you take a fluid which is at first quiet, then drive it harder and harder until the flow becomes turbulent. I, on the other hand, am talking about fully developed turbulence, which is thoroughly distinct in terms of the mathematical technology involved. For instance, turbulence in the atmosphere is there and never ceases to be thereit's fully developed. So the question is, how do you describe developed turbulence? It's well past the point of its onset and has spread everywhere. The tools needed are traditionally very different from those pertaining to the onset of turbulence.
Papanicolaou: There really
hasn't been much progress. There was the so-called renormalization group method that was
started in the 1970s by physicists, primarily Kenneth Wilson of Cornell. His idea was that
when you're dealing with problems in which many scales interact simultaneously, you take a
few scales at a time and calculate the interactions between them and then put the whole
thing together in a self-consistent way and come up with a global theory. It's a nice
idea, but it has been understood mathematically only for toy problems. So far it hasn't
really played any role that we would have wanted it to playfor example, in actually
generating equations that drive interactions between the scales so that we can really
solve problems.
Papanicolaou: One really interesting problem is to think of clever ways to make numerical calculations that really straddle many scales. So far the numerical calculations have been rather straightforwarddirect numerical calculation: write down the equations, put them on the computer, solve them. There have to be more intelligent ways of approaching this, to put more insight into the computer modeling. In the next 10 or 20 years, that's what's going to happen. The computational schemes are going to become increasingly intelligent, more adaptive. We are going to put into computer code the ability to recognize its environment and adapt, to become more efficient, and to be guided by the theory.The scant theory that exists right now is not employed in any intrinsic way when you use a computer to help make the problem more efficient. For turbulence it would be enormously important to be able to do that.
Papanicolaou: Of course I'm
not satisfied. There are two things I still hope I'll be able to do. One is to find a way
to create numerical computational methods that really use theoretical insight. This is the
Holy Grail among a small group of people who really understand the mathematics: to find a
way to really make the computer leverage your insight. I'm trying to do that now. As far
as analytical things, I underestimated the importance in the last 20-some years of chaos
theory. I felt it was overplayed and that the results were too qualitative and too thin
for my tastes. But now I'm beginning to change my mind. Some substance is really coming
out of chaos theory and the subject is solidifying, and I'd like to understand it. The
glitz is wearing off, and now there seems to be some interesting work going on. |
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