Research Groups

    Astrophysics
    Computational Physics
    Materials Science
    Particle Physics

Astrophysics

   Our research in astronomy and astrophysics focuses on studying the formation of our Milky Way Galaxy, using positions, velocities, and chemical compositions of stars. Additional astrophysics research on radio galaxy jets in included under computational physics.

m54 star chart

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Computational Physics

   Much of the Department's research effort centers around unifying interest in computational physics. Members of this group are interested in the application of the methods of computational physics to a wide variety of research areas, including:

  • Materials Physics

  • Astrophysics

  • General Relativity

  • Elementary Particles

  • Rayleigh-Benard Convection; Lattice Boltzmann Methods

  • Environmental Physics

computational 1 computational 2

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Materials Science

   The materials physics group is interested in the experimental investigation of electrical, magnetic and optical properties of solids, with special attention paid to those materials which have application in device technology.

materials 1 materials 2

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Elementary Particle Physics

   The goals of the research effort in particle physics are twofold: to find a fundamental explanation of the spins, masses and decay modes of the mesons and baryons and to find a compact mathematical description of these properties with a minimum number of adjustable parameters. Both of these goals are now being pursued within the context of our present theory of strong interactions, Quantum Chromodymanics, the theory of quarks and gluons.

    Dr. Lewis Fulcher is collaborating with Baker, Ball and Zachariasen, who have spent more than a decade developing the dual superconducting theory of QCD. Initial tests of their theory give good indications of agreement with the measured energies and splittings of the heavy-quark systems (charmonium and the upsilon system). Their results for the quark-antiquark potential are also supported by lattice gauge calculations.

   His role in this collaboration is to extend the tests of the theory to systems consisting of a heavy quark and a light antiquark (or its charge conjugate), where relativistic effects are much more important. This additional series of tests is made possible by a new procedure for solving relativistic wave equations with nonlocal operators, such as the Salpeter equation.

   Other applications of the procedure focus on quasiparticle reductions of the Bethe-Salpeter equation. Additional interests include the general properties of nonlocal wave equations and the detailed calculation of meson properties with QCD-based phenomenological potentials, such as Richardson's potential.

   References:

   1. Fulcher, Physical Review D50, 447 (1994)

   2. Baker, Ball and Zachariasen, Physical Review D51, 1968 (1996)

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