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Session S5 - Atoms and Ions.
ORAL session, Saturday morning, October 25
LaPaz, Memorial Union

[S5.001] Total Energies of Atoms from Path Integral Monte Carlo Simulations

Daejin Shin, John Shumway (Department of Physics and Astronomy, Arizona State University, Tempe, Arizona 85287)

Several ab initio methods exist for calculating energies of atoms, molecules, and solids. We are testing a new technique that uses Feynman path integrals. This new many-body method includes finite temperature and can be much more accurate than other popular techniques. We calculated the ground state energies of the first four atoms in the periodic table, H, He, Li and Be with Path Integral Monte Carlo simulations. We find total energies that are more accurate than both density functional theory and Hartree-Fock. We are also studying diatomic molecules to see thermal effects on geometry and polarization.

[S5.002] Monte Carlo Simulation of Wave Damping in a Dilute Gas

Ryan Clary (Utah Valley State College), Ross Spencer (Brigham Young University)

A computer simulation has been written that simulates the evolution of a perturbed dilute gas using the Direct-Simulation Monte Carlo method, with the ultimate goal of adding collisions to a simulation of ultra-cold plasmas. As a test, it has been used to study fluid dynamic affects in one dimension using a small velocity perturbation so that comparison with standard gas-dynamic theory is possible. This comparison has been used to investigate the limitations on certain simulation parameters such as cell size, size of each time step, number of simulation particles, and mean-free-path. The simulation and the theory agree well when the mean-free path is a small fraction of the sound wavelength, but for long mean free paths the simulation and the theory diverge. As an illustration, the famous ``bell in a bell jar'' demonstration will be examined to see if wave damping might play a role.

[S5.003] Low-field orientation dependence of ^3He relaxation in spin-exchange cells

J. Teter, R. E. Jacob, B. Saam (University of Utah), W. C. Chen, T. R. Gentile (NIST)

^3He, a spin-\frac12 noble gas, can be highly polarized by spin-exchange optical pumping (SEOP) for use in applications such as magnetic resonance imaging (MRI). The ability to maximize and maintain the ^3He polarization is crucial when using ^3He as a signal source for MRI. We have observed a significant dependence of ^3He longitudinal relaxation times (T_1) in glass SEOP cells due only to the physical orientation of the cell in a \approx30 G measurement magnetic field. In contrast with previous work, the cells either had no previous exposure to higher fields or were thoroughly degaussed prior to T_1 measurements. The presence of Rb metal and heating of the cells associated with the SEOP process is necessary to produce this low-field orientation dependence. Our data suggest that the hysteretic (R. E. Jacob, \emphet al., Phys. Rev. Lett. \underline87 143004 (2001)) magnetic relaxation sites involved here may be the dominant cause of wall-relaxation in SEOP cells at any field.

[S5.004] Quantum Monte Carlo treatment of Spin Orbit Interaction

Raghu Chatanathody, John Shumway, Kevin Schmidt (Department of Physics and Astronomy, Arizona State University)

We treat the spin-orbit interaction in many-electron systems within variational and diffusion Monte Carlo. We explicitly include the spin degrees of freedom by putting a two-component spinor on each electron. In our all-electron atomic calculations, the spin-orbit interaction is a parameter-free relativistic correction to the Schrodinger equation. This interaction is simply the local electric field at each electron, which appears as a magnetic field in that electron's rest frame. Thus our many-body calculations give the atomic spin-orbit coupling strengths by evaluating the electric field from the nucleus and all other electrons, and coupling to the electron's spin and velocity. We illustrate this method on first and second row atoms, and discuss its potential applications to solids and molecules. (Work supported by DARPA/ONR )

[S5.005] Laser Beam Energy Deposition by Ray Tracing in a Laser-Produced Plasma

Zafar Yasin (Department of Physics, UNLV , Las Vegas.)

Uniformity of energy deposition in the coronal plasma surrounding the pellet surface is crucial for meeting Lawson criteria for ICF. Energy deposition can be computed by tracing laser rays through the plasma using approximation of geometrical optics. Ray tracing equations for a focused laser beam propagating through the plasma are derived, for various beam target configurations. S-polarized laser light is considered for energy absorption by inverse bremstrahlung, and p-polarized for resonance absorption. A ray tracing code has been used to see optical interference effects on the uniformity of energy deposition.

[S5.006] Semi-classical Study of Electron Blurring in the Magnetic Field of a Current Ring

Daniel James, Jean-Francois Van Huele (Brigham Young University)

We develop a semi-classical method for determining small quantum variations around classical trajectories and apply it to the dynamical variables of an axial beam of charged particles passing through the center of a current ring. We obtain a complete set of coupled differential equations that describe the evolution of the beam and we solve numerically to determine the blurring introduced by the small quantum corrections. We compare the longitudinal blurring of the beam to the spin separation under the influence of the inhomogenous magnetic field. The results will be illustrated with animations. Implications on the feasability of a longitudinal Stern-Gerlach experiment with electrons will be discussed.

Part S of program listing