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Open shell atom

The nonrelativistic open shell formalism of Roothaan [35] has been adapted to the one-centre relativistic case by Kagawa [96] and this work has been further expanded by Mohanty and dementi [105]. The reader is referred to these papers for the details. [Pg.166]

A less demanding, but still useful, approximation is the configuration average model, which is an adaptation of the closed shell DHF scheme. The starting point of this scheme is the closed shell expression (95) which, after dropping the Breit terms, takes the form [Pg.166]

In terms of subshell quantities, the system energy can be expressed in the form [Pg.166]

The coefficients for open-shell configurations are state-dependent [25,27] and are difficult to write in compact form. However, a simple and useful model may [Pg.166]

We now assume that shell A has at most two j -labelled subshells a and a, with Qa and q a electrons respectively, with + , where = (4 + 2) is the [Pg.167]


What is obviously needed is a generally accepted recipe for how atomic states should be dealt with in approximate density functional theory and, indeed, a few empirical rules have been established in the past. Most importantly, due to the many ways atomic energies can be obtained, one should always explicitly specify how the calculations were performed to ensure reproducibility. From a technical point of view (after considerable discussions in the past among physicists) there is now a general consensus that open-shell atomic calculations should employ spin polarized densities, i. e. densities where not necessarily... [Pg.166]

Results for the other open-shell atoms are encouraging. One would expect the P3 method to be considerably less accurate when an unrestricted Hartree-Fock reference state is used. The lowest MAD for B -Ar obtains with the largest of the Dunning sets examined here, i.e. cc-pVQZ. The 6-311++G(3df,3pd) and well-tempered basis sets (WTBS) are roughly equivalent, with MADs of 0.50 eV and 0.57 eV, respectively. [Pg.146]

Fig. 12.1 An ultra-fast heating of a cluster containing both N2 and 02 molecules upon impact at a surface. [9] Shown is the instantaneous configuration of 14 N atoms (dark) and 14 O atoms (light) 50 fsec after a cluster of 7 N2 and 7 02 molecules embedded in 97 Ne atoms impacts a surface at a velocity of 20 Mach. The potential used allows for alii 25 atoms of the cluster to interact with one another and with the atoms of the surface. In addition, each atom-atom chemical interaction is influenced by the presence or absence of other open-shell atoms nearby. Fig. 12.1 An ultra-fast heating of a cluster containing both N2 and 02 molecules upon impact at a surface. [9] Shown is the instantaneous configuration of 14 N atoms (dark) and 14 O atoms (light) 50 fsec after a cluster of 7 N2 and 7 02 molecules embedded in 97 Ne atoms impacts a surface at a velocity of 20 Mach. The potential used allows for alii 25 atoms of the cluster to interact with one another and with the atoms of the surface. In addition, each atom-atom chemical interaction is influenced by the presence or absence of other open-shell atoms nearby.
In Section 3 we have formulated Strutinsky s shell-correction method in the framework of the analytic HFR scheme, for single open-shell atoms and molecules in their ground state. The consideration of two or many open-shell systems could be performed following the same pattern. Both the averaged part of the energy, E,jp, and its first-order shell-correction part, 8,E pr, have been derived in analytic form, and the self-consistent process for determining them has been described. [Pg.62]

M.L. Dubernet, J.M. Hutson, Atom-molecule van der Waals complexes containing open-shell atoms. 2. The bound states of C1-HC1, J. Phys. Chem. 98 (1994) 5844. [Pg.164]

This work done is path-independent since V x R(r) = 0. For systems of certain symmetry such as closed shell atoms or open-shell atoms in the central-field approximation, the jellium and structureless-pseudopotential models of a metal surface considered here, etc., the work Wxc (r) and Wt (r) are separately path-independent since for these cases Vx xc(r) = VxZt (r) = 0. [Pg.246]

Dubernet ML, Hutson JM (1994) Atom-molecule Van der Waals complexes containing open-shell atoms. I. General theory and bending levels. J Chem Phys 101 1939-1958... [Pg.151]

In protoplanetary disks, a number of neutral-neutral reactions can also be fast, and not restricted to the warm inner region. In particular, neutral-neutral reactions between radicals and radicals, radicals and open-shell atoms, and radicals and unsaturated molecules are quite effective (van Dishoeck 1998). The typical rate coefficient for these reactions is 10-11-10-1°cm-3s-1, i.e. only about an order of magnitude lower than for the ion-molecule processes (e.g. Clary et al. 1994 Smith et al. 2004). One of the most interesting reactions of this type is the formation of HCO+ upon collision between O and CH (a0 = 2.0 10-11 cm-3 s-1 and ft = 0.44 Woodall et al. 2007). Another vital neutral-neutral reaction is the formation of formaldehyde CH3 + O -> H2CO + H ( o = 1-3 10-1°cm-3 s-1 and = 0 Woodall et al. 2007). [Pg.108]

Explicit expressions for the effective adiabatic potential curves, F(0), in the Hund s case (c) representation are given below [183]. They correlate with states of the open-shell atom defined by the atomic total electronic angular momentum and its projection along the internuclear axis. For the interaction of Hg( Pj) with Rg, the KfO) interactions are ... [Pg.333]

As we have seen previously (Chapter 5), the eigenfunction for a polyelec-tronic atom is antisymmetric with respect to the exchange of the coordinates of any two electrons, and can be expressed as a Slater determinant whose elements are the various occupied spin-orbitals (or a linear combination of Slater determinants, in the case of open-shell atoms). The same appfies to polyelectronic molecules, the atomic orbitals being replaced by the various occupied molecular orbitals associated with the a and /3 spin-functions spin molecular orbitals. Thus, for the molecules H2O, NH3 or CH4 having five doubly occupied m.o.s (one core s orbital and four valence m.o.s), we have... [Pg.193]

Meyer. H.-D. and Miller. W. H. (1979) Classical models for electronic degrees of freedom Derivation via spin analogy and application to F +H2 ->F+H2, J. Chem. Phys. 71, 2156-69. Dubemet, M.-L. and Hutson, J. M. (1994) Atom-molecule van der Waals complexes containing open-shell atoms. 1. General thoery and bending levels, J. Chem. Phys. 101. 1939-58. [Pg.66]

The interaction between an open shell atom with a closed shell atom or molecule can be modeled with the Diatomics-in-Molecule (DIM) method [11]. This is an approximate approach, however, with a sounel r hemir al mothntion. The total interaction energy between an open shell atom anel all the remaining closed shell atoms in the cduster can be expressed in a pair additive way as Vo/m = X) =i n where r is the raelius vector between the i-th rare gas atom anel the p-atom (open shell atom) anel is the interaction energy between a single rare gas atom... [Pg.481]

H.P. Kelly, Many-body perturbation theory applied to open-shell atoms, Phys. Rev. 144 (1966) 39. [Pg.101]

In 1978, Ludena [102] carried out a Hartree-Fock calculation by using a wave function consisting of a single Slater determinant for the closed-shell atoms, whereas he used a linear combination of the Slater determinants for the open-shell atoms. Each Slater-type orbital times a cut-off function of the form (1 — r/R) to satisfy the boundary conditions. Ludena studied pressure effects on the electronic structure of the He, Li, Be, B, C and Ne neutral atoms. The energies he obtained for the confined helium atom are slightly lower than those Gimarc obtained, especially for box radii in the range R > 1.6 au. [Pg.155]


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See also in sourсe #XX -- [ Pg.469 ]




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