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Quantum calculation, vibrational energy

The vibrational relaxation of simple molecular ions M+ in the M+-M collision (where M = 02, N2, and CO) is studied using the method of distorted waves with the interaction potential constructed from the inverse power and the polarization energy. For M-M collisions the calculated values of the collision number required to de-excite a quantum of vibrational energy are consistently smaller than the observed data by a factor of 5 over a wide temperature range. For M+-M collisions, the vibrational relaxation times of M+ (r+) are estimated from 300° to 3000°K. In both N2 and CO, t + s are smaller than ts by 1-2 orders of magnitude whereas in O r + is smaller than t less than 1 order of magnitude except at low temperatures. [Pg.50]

The time constant r, appearing in the simplest frequency equation for the velocity and absorption of sound, is related to the transition probabilities for vibrational exchanges by 1/r = Pe — Pd, where Pe is the probability of collisional excitation, and Pd is the probability of collisional de-excitation per molecule per second. Dividing Pd by the number of collisions which one molecule undergoes per second gives the transition probability per collision P, given by Equation 4 or 5. The reciprocal of this quantity is the number of collisions Z required to de-excite a quantum of vibrational energy e = hv. This number can be explicitly calculated from Equation 4 since Z = 1/P, and it can be experimentally derived from the measured relaxation times. [Pg.53]

A vibrational basis set is chosen for the molecule and the quantum mechanical variational method (Eqs. (2.66)-(2.68)) is used to calculate vibrational energy levels from the analytic potential. The parameters/ -, byi i in the potential are varied until the experimental vibrational energy levels are fit. This variational method is only practical at low levels of excitation. [Pg.60]

J. L. Skinner and K. Park,/. Phys. Chem. B, 105,6716 (2001). Calculating Vibrational Energy Relaxation Rates from Classical Molecular Dynamics Simulations Quantum Correction Factors for Processes Involving Vibration-Vibration Energy Transfer. [Pg.303]

Skinner, ).L. and Park, K. (2001) Calculating vibrational energy relaxation rates from classical molecular dynamics simulations quantum correction factors for processes involving vibration-vibration energy transfer. J. Phys. Chem. B, 105 (28), 6716 6721. [Pg.272]

Fig. 5. The probability of energy transfer per unit energy P2(As) for the initial nj=2 vibrational level of D2, vevsus the energy transfer Ae, calculated with a Morse potential for D2 and hard-core repulsion for H-D, at initial kinetic energy E. The unit of energy is the first quantum of vibrational energy. Fig. 5. The probability of energy transfer per unit energy P2(As) for the initial nj=2 vibrational level of D2, vevsus the energy transfer Ae, calculated with a Morse potential for D2 and hard-core repulsion for H-D, at initial kinetic energy E. The unit of energy is the first quantum of vibrational energy.
Quantum Calculations of Vibrational Energy Levels of Acetylene (HCCH) up to 13000 cm-1. [Pg.341]

A58, 727 (2002). Quantum Calculation of Highly Excited Vibrational Energy Levels of CS2(X) on a New Empirical Potential Energy Surface and Semiclassical Analysis of 1 2 Fermi Resonances. [Pg.344]

Equilibrium stable isotope fractionation is a quantum-mechanical phenomenon, driven mainly by differences in the vibrational energies of molecules and crystals containing atoms of differing masses (Urey 1947). In fact, a list of vibrational frequencies for two isotopic forms of each substance of interest—along with a few fundamental constants—is sufficient to calculate an equilibrium isotope fractionation with reasonable accuracy. A succinct derivation of Urey s formulation follows. This theory has been reviewed many times in the geochemical... [Pg.69]


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