INTERACTION ENERGY IN GEOMETROSTATICS
Interaction energy in geometrostatics - geometrodynamic description of particles by topological features of empty space-time
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Interaction energy in geometrostatics - geometrodynamic description of particles by topological features of empty space-time
Long range retarded interaction energies, obtaining energy term coefficient from minimal principle using Karplus and Kolker method
Retarded long range interaction energies between two like atoms in different energy states, noting selection rules for resonant interactions
Relativistic interaction energies between atoms in degenerate states determined, using Breit-Pauli approximation
Complete sets of ion-atom interaction energies have been computed for nitrogen and oxygen with accurate large scale structure calculations. The computed energies agree well with the accurate potential curves available from spectroscopic measurement. The state functions from the nitrogen calculations have been applied to determine the transition moment for all allowed dipole transitions. These results can be combined to compute a detailed radiation spectrum such as that required to define the highly nonequilibrium environment of aeroassisted orbital transfer vehicle (AOTV). The long-range interaction energies have been used to determine the ion-atom resonance charge exchange cross sections that are important for transport processes such as diffusion. A calculation to determine reliable transport properties for energies that include the AOTV temperature range from these computed properties is described.
Interaction energies for the H-H (sub 2) and H (sub 2) - H (sub 2) systems have been obtained by a semi-empirical perfect-pairing procedure used previously. The results have been compared with interaction energies obtained from other sources and the agreement among the different curves is reasonably good. A brief discussion of the previous applications of this semi-empirical scheme to other systems is included.
Hyperfine splitting of spin interaction energy of two hydrogen atoms, determining eigenfunctions for effective Hamiltonian
Interaction energy and dipole moment in collisions of two hydrogen molecules
Hyperfine interaction of ground state D atom with ground state H or D atom, obtaining interaction energy hyperfine splitting and potential energy curves
The highlights of seven sessions of the Conference dealing with high energy interactions of cosmic rays are discussed. High energy cross section measurements; particle production-models of experiments; nuclei and nuclear matter; nucleus-nucleus collision; searches for magnetic monopoles; and studies of nucleon decay are covered.
The energies for the interaction of a hydrogen atom with a nitrogen molecule have been calculated for large separation distances using a complete-active-space self-consistent-field/externally contracted configuration interaction method. H-N2 transport cross sections and collision integrals have been calculated using sudden approximations and a semiclassical description of the scattering. The values of these quantities are found to be close to the corresponding values determined from the average (isotropic) potential energy. The collision integrals are applied to determine diffusion and viscosity coefficients; the theoretical diffusion agrees well with the measured data available from experiments at low temperatures.
Interaction energy levels and transport coefficients of lithium-hydrogen and oxygen- hydrogen gas mixtures at high temperatures
The lateral distribution of gamma-families observed by emulsion chamber is sensitive to test transverse momentum of high energy interaction. But most part gamma-families are succesive interation's results which makes it necessary to analyze the propagation of gamma-ray in atmosphere. A gamma-ray with energy Er and transverse momentum Pt is produced at the altitude h. In the emulsion chamber experiment, Eob is estimated by decascade method. There are 30 gamma-families observed by Ganbala emulsion Chamber. A group of Monte-Carlo simulation gamma-families are used to compare with experimental data with the same treatment. It is found that both distributions are consistent.
Interaction energies, charge exchange cross sections, & diffusion cross sections for collisions of atoms of nitrogen & oxygen with corresponding positive ions
Interaction energies from scattering cross section of hydrogen ions in methane, ethane, carbon tetrafluoride, and hexafluoroethane
Interaction energies from scattering cross section of hydrogen ions in methane, carbon tetrafluoride, ethane, and hexafluoroethane
Long range first order interaction between two excited hydrogen atoms yielding perturbation energy matrix, discussing diagonalization process
The aerothermodynamic studies of proposed space missions require atmospheric charge-transfer data. N2(+) eigenstate energies are calculated with use of the complete-active-space self-consistent-field method with an extended Gaussian basis set. The N(+)-N charge-exchange cross section, determined from these energies, agrees with merged-beam measurements. This contradicts the previous theoretical conclusion. A simple physical description of the long-range interaction is presented and should expedite future charge-transfer studies.