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Session F1 - Dreams for the Future of Physics.
INVITED session, Monday evening, March 03
Ballroom A, Austin Convention Center

[F1.001] The Future of Condensed Matter Physics

Steven Girvin (Yale University)

Where are we? Where are we going? Where should we be going? Condensed matter systems have proven capable of existing in a marvelous variety of physical states that exhibit fundamental phenomena of interest even outside our subfield, particluarly in elementary particle physics. Will this continue or are the different subfields beginning to lose touch with each other as they mature? It is already clear that a large and unfortunate communication gulf has developed even inside our own community between the soft matter and electronic materials camps.

Most members of our community have been proud to celebrate the technological relevance of our subfield. The past few decades have seen a marvelous synergy in which advances in condensed matter physics have led to technological advances. These in turn have permitted explorations of new realms and allowed new fundamental physics advances. Will this synergy continue or are we in danger of becoming technologically irrelevant?

It is clear that we are entering a new era of confluence between atomic/molecular/optical physics and condensed matter physics. It is less clear but quite possible, that we are at the dawn of an age in which we will spin off a new subfield of quantum electrical engineering and quantum computation.

Can we develop a useful understanding of complex materials? Whither nano-scale physics? Our colleagues in other subfields of physics seem to be better at communicating the excitement of their research to the public. What can we do on this front? I do not have answers to all these questions, but will at least attempt to make a few observations on them.

[F1.002] The Future of Particle and Nuclear Physics

Frank Wilczek (MIT)

The standard model of particle physics is extremely successful, but incomplete. Its mathematical structure suggests how it might be derived from a more comprehensive unified theory. The arguments are both aesthetic and quantitative. They predict specific new phenomena observable which will be observable at the Large Hadron Collider (LHC). Recent results on neutrino masses confirm and encourage this line of thought. Another problem within the standard model, the so-called strong CP problem, is one of a number of reasons to suspect the existence of a radically new class of very light, very weakly interacting particles. All these ideas have important implications for cosmology; in particular, they provide plausible, testable candidates for the ``dark matter''.

For nuclear physics, the future is QCD. This theory opens new possibilities for understanding hadronic matter at extreme temperatures (as in the big bang, and at RHIC) and extreme density (as in neutron star interiors). Recent insights concerning color superconductivity are especially beautiful, and shed penetrating new light on the problem of quark confinement. Another lively frontier is the direct solution of the QCD equations using the full power of modern parallel computing.

[F1.003] Dreams for the Future of Physics: Astrophysics and Cosmology

Michael S. Turner (The University of Chicago and Fermilab)

Our understanding of the Universe and the objects within is in the midst of a revolution powered by technology and ideas. The richness of the opportunities and the deep connections to physics are illustrated by the questions astrophysicists are trying to answer: What is the dark matter that holds galaxies together? What is the frequency of planetary systems like ours and how do they form? How did the Universe begin? What are the highest energy particles in the Universe and how were they accelerated? How does superconductivity work at ten billion degrees and what other states of exotic matter exist in neutron stars? Do black holes work the way Einstein's theory predicts? What is the nature of the dark energy that is causing the expansion of the Universe to speed up? How does the nuclear deflagration of a white dwarf star proceed and produce a supernova? What is the origin of the ubiquitous magnetic fields in the Universe and how do they power phenomena such as stellar coronae?

[F1.004] The Future of Physics in Biology

Albert Libchaber (Detlev W. Bronk Professor, The Rockefeller University, NYC and Fellow, NEC Research Institute, Princeton, NJ)

There is an apparent conflict between the search for universality in physics and the intricate and necessary search for details in biology, between formal theory and story telling. Research in genomes and gene networks tends to reduce this contradiction. Also, implementation of computational aspects of biology into physical processes leads to stimulating interchange. A theory of information and computation as a natural phenomenon is in limbo and needs to be extended. Finally, the development of new tools and techniques is a very active ground for research.

[F1.005] The Future of String Theory

David Gross (Univ. Calif. / Santa Barbara)

Part F of program listing