@article {409,
	title = {Velocity distributions of energetic atoms in planetary exospheres from dissociative recombination},
	journal = {Journal of Geophysical Research-Planets},
	volume = {107},
	number = {E7},
	year = {2002},
	note = {ISI Document Delivery No.: 610UBTimes Cited: 3Cited Reference Count: 47},
	month = {Jul},
	pages = {9},
	type = {Article},
	abstract = {[1] A kinetic theory description of translational energetic atoms in the upper planetary atmosphere is presented. A new analytical result for the velocity distribution of the products of reactive collisions is described. Our calculation takes into account different temperatures of the reactants and arbitrary dependence of the cross section on the relative velocity of the colliding particles. The final result is applied to the production of hot oxygen and carbon by dissociative recombination of O-2(+) and CO+, respectively. The nascent distribution of hot atoms generated in this way is compared with the earlier Monte Carlo calculations. We use the Boltzmann equation to study the thermalization of the hot oxygen via collisions with the thermal oxygen population. The results of this calculation demonstrate quasi-steady state velocity distribution of high-energy oxygen atoms near the exobase of Venus for daytime conditions.},
	keywords = {Boltzmann equation, CROSS-SECTIONS, dissociative recombination, ESCAPE, gas kinetic, hot atoms, HOT OXYGEN-ATOMS, HYDROGEN, ION STORAGE-RING, MARS, MONTE-CARLO, NITROGEN-ATOMS, theory, UPPER-ATMOSPHERE, VENUS},
	isbn = {0148-0227},
	url = {<Go to ISI>://000178978400004},
	author = {Kabin, K. and Shizgal, B. D.}
}
@article {3659,
	title = {Analysis of X-ray photoelectron spectra of eight polymers by deMon density-functional calculations using the model oligomers},
	journal = {Journal of Physical Chemistry},
	volume = {100},
	number = {50},
	year = {1996},
	note = {ISI Document Delivery No.: VX875Times Cited: 29Cited Reference Count: 57},
	month = {Dec},
	pages = {19455-19460},
	type = {Article},
	abstract = {The X-ray photoelectron spectra of eight polymers [(CH2CH2)(n), (CH2CH2NH)(n), (CH2O)(n), (CH2CH2S)(n), (CH(2)CHX)(n), and (CH(2)CX(2))(n) (X = F, Cl)] were analyzed by the deMon density-functional method using the model oligomers. Calculated AIK a valence photoelectron spectra were obtained using Gaussian line shape functions of an approximate Line width (0.10I(k)), where I-k = I-k{\textquoteright} - WD, I-k{\textquoteright} is the vertical ionization potential of each MO, and WD is a shift to account for sample work function, polarization energy, and other effects. The theoretical spectra showed good agreement with the experimental spectra of the polymers between 0 and 40 eV. The core-electron binding energies (CEBEs) of C1s, N1s, O1s, F1s, S2p, and Cl2p of the model oligomers were calculated by unrestricted generalized transition-state models. The difference between the calculated and the experimental CEBEs reflects the trend in WDs of the polymers.},
	keywords = {APPROXIMATION, CORE, ELECTRON BINDING-ENERGIES, LOCAL-DENSITY, MOLECULES, POLY(METHYL METHACRYLATE), POLY(VINYL ALCOHOL), SEMIEMPIRICAL MO, theory, VALENCE ENERGY-LEVELS, XPS SPECTRA},
	isbn = {0022-3654},
	url = {<Go to ISI>://A1996VX87500039},
	author = {Endo, K. and Kaneda, Y. and Okada, H. and Chong, D. P. and Duffy, P.}
}
