University of Redlands

Research

The Nuclear Physics Research Program

The active program of nuclear research conducted by Redlands' physics faculty and students involves experimental work done in collaboration with various research laboratories throughout the world. Current projects include elastic scattering experiments at the Crocker Nuclear Laboratory at the University of California, Davis, and total reaction cross-section measurements conducted at the Svedberg Cyclotron Laboratory, Uppsala University in Sweden. The University of Redlands nuclear group is a world leader in the measurement of total reaction cross-sections, and student participants often become co-authors, along with the faculty, of the resulting published research papers.

The Laser Photonics Laboratory

Jointly operated by faculty from physics and chemistry, the Laser Photonics Laboratory offers students the opportunity to work with faculty members to conduct state-of-the-art research. Students participate in directed study and honors research projects on laser-based spectroscopy, holography, electro-optics, computer control of laser systems, and experimental laser development.

Atom Trapping

Lasers and special magnetic fields are used to cool large numbers of neutral atoms to within a fraction of a degree of absolute zero and to confine them to a region of a few cubic centimeters. Students are constructing such "atom traps" for use in high precision spectroscopic and atomic collision experiments.

Scanning Tunneling Microscopy (STM)

The atomic scale investigation and manipulation of conducting surfaces. This falls under the heading of surface science within the broader field of condensed matter physics.

Planetary Science

Studying solid planetary surfaces such as Venus, Mars, and the moons of Jupiter. Looking at volcanoes and other thermal processes on planets.

Stellar and extragalactic astronomy

Studying stellar surfaces and structure through the new field of optical interferometry. In addition, investigating various aspects of galaxy formation and interaction using optical and radio observatories.

Updated 10/4/01