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Hydrogenic Atomic Systems

The fundamental problem of hydrogenic atom relies on considering the atomic effective (Coulombie + eentrifiigal contributions) potential [Pg.219]

Quantum Nanochemistry-Volume I Quantum Theory and Observability [Pg.220]

FIGURE 3.13 The complex integration contours resulting in the poles I and II and in the closed integral between and turning points of atomic hydrogenic action in the semiclassical quantification. [Pg.220]

Now we can immediately perform the semiclassical quantification for hydro-genic atoms through calling back the performed notations for 4, B and C  [Pg.221]


Barker, R. S., Snow, R. L., and Eyring, H., J. Chem. Phys. 23, 1686, "Energy calculations of multiple hydrogen-atom systems by VB and MO methods."... [Pg.340]

In Section 2 we define the symmetrized hyperspherical coordinates for the electron-hydrogen atom system and express the hamiltonian in these coordinates. In Section 3 symmetry is discussed. The appropriate symmetry wave functions are introduced in Section 4, the local surface eigenfunctions and energy eigenvalues in Section 5, and the scattering equations and asymptotic analysis in Section 6. Finally, some representative results are given and discussed in Section 7 and a summary of the conclusions is presented in Section 8. [Pg.193]

The exotic hydrogen atoms, systems consisting of a proton and a negative particle, or a positive particle and an electron, are special in many aspects (Eides et al. 2001). Their basic properties are summarized in O Table 28.2. [Pg.1498]

Figure 17.1 The Hydrogen Atom System Consisting of a Nucieus and an Eiectron. Figure 17.1 The Hydrogen Atom System Consisting of a Nucieus and an Eiectron.
Applications of quantum mechanics to chemistry invariably deal with systems (atoms and molecules) that contain more than one particle. Apart from the hydrogen atom, the stationary-state energies caimot be calculated exactly, and compromises must be made in order to estimate them. Perhaps the most useful and widely used approximation in chemistry is the independent-particle approximation, which can take several fomis. Conuiion to all of these is the assumption that the Hamiltonian operator for a system consisting of n particles is approximated by tlie sum... [Pg.24]

Thakkar A J 1988 Higher dispersion coefficients accurate values for hydrogen atoms and simple estimates for other systems J. Chem. Phys. 89 2092... [Pg.212]

The simplest system exliibiting a nuclear hyperfme interaction is the hydrogen atom with a coupling constant of 1420 MHz. If different isotopes of the same element exhibit hyperfme couplings, their ratio is detemiined by the ratio of the nuclear g-values. Small deviations from this ratio may occur for the Femii contact interaction, since the electron spin probes the inner stmcture of the nucleus if it is in an s orbital. However, this so-called hyperfme anomaly is usually smaller than 1 %. [Pg.1556]

The elements of an organic compound are listed in empirical formulas according to the Hill system [8] and the stoichiometry is indicated by index numbers. Hill positioned the carbon and the hydrogen atoms in the first and the second places, with heteroatoms following them in alphabetical order, e.g., C9H11NO2. However, it was recognized that different compounds could have the same empirical formula (see Section 2.8.2, on isomerism). Therefore, fine subdivisions of the empirical... [Pg.20]

The correction term in Eq. (9) shows that the basic assumption of additivity of the fragmental constants obviously does not hold true here. Correction has to be appHed, e.g., for structural features such as resonance interactions, condensation in aromatics or even hydrogen atoms bound to electronegative groups. Astonishingly, the correction applied for each feature is always a multiple of the constant Cu, which is therefore often called the magic constant . For example, the correction for a resonance interaction is +2 Cj, or per triple bond it is -1 A detailed treatment of the Ef system approach is given by Mannhold and Rekker [5]. [Pg.493]

Temperature also determines step size. An acceptable time step for room temperature simulations is about 0..5-1 fs for All Atom system s or for sim Illation s that do not con strain hydrogen atoms. For United Atom systems or systems containing only heavy atoms, you can use steps of 1-2 fs. [Pg.89]

II of the actual atoms (or at least the non-hydrogen atoms) in the core system are lented explicitly. Atomistic simulations can provide very detailed information about haviour of the system, but as we have discussed this typically limits a simulation to nosecond timescale. Many processes of interest occur over a longer timescale. In the if processes which occur on a macroscopic timescale (i.e. of the order of seconds) rather simple models may often be applicable. Between these two extremes are imena that occur on an intermediate scale (of the order of microseconds). This is the... [Pg.418]


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