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Radius orbital

The ir-bond between two silicon atoms (>Si=Si<) was formerly thought to be non-existent and then was found to be extremely weak. This has been explained in the past by the extended bond length, with respect to ethylene, which was thought to be the origin of a seemingly low 3p-3p(ir) atomic overlap S(tt) [1]. However, the overlap actually has never been calculated before. Calculations indicate quite similar p-p(ir) overlap integrals in disilene and ethylene so that the different bond lengths for C=C and Si=Si must be explained by the different orbital radii (Fig. 1). [Pg.81]

Figure 3.19 illustrates the dependence of Asp on location in the periodic table for each of the first three elements of main groups 13-17. The promotion energy varies with group number in a manner similar to electronegativity (cf. Fig. 3.17). Although Asp is doubtless important, other factors (such as differences in orbital radii) appear to play a role in general spd hybridization. Figure 3.19 illustrates the dependence of Asp on location in the periodic table for each of the first three elements of main groups 13-17. The promotion energy varies with group number in a manner similar to electronegativity (cf. Fig. 3.17). Although Asp is doubtless important, other factors (such as differences in orbital radii) appear to play a role in general spd hybridization.
The size of an atom or molecule is important in numerous physical phenomena and properties, and its value depends on the circumstances. Table 4.2 gives the orbital radii of the atoms compiled by Karplus and Porter (1970), which are the radii of the... [Pg.75]

An approach based on orbital radii of atoms effectively rationalizes the structures of 565 AB solids (Zunger, 1981). The orbital radii derived from hard-core pseudopotentials provide a measure of the effective size of atomic cores as felt by the valence electrons. Linear combinations of orbital radii, which correspond to the Phillips structural indices and have been used as coordinates in constructing structure maps for AB solids. [Pg.9]

The frozen planet model also agrees with classical calculations of Richter and Wintgen,39 who find a classically stable state in which both electrons are on the same side of the atom in orbits which exhibit pronounced angular correlation, even though the orbital radii of the two electrons are very different. [Pg.488]

This equation must hold for all values of r which occur in the orbits. Let us assume it holds identically for all values of r, as it surely holds for all those in which we are interested and as the use of —F = dV/dr implies other values of r at least in the vicinity of the orbital radii. [Pg.2]

For low ion populations, a first estimate of achievable ejection resolution might be obtained from the cyclotron frequency spread that occurs over the range of cyclotron orbit radii through which the ion must pass to be ejected. This is based on the notion that an ejection waveform that is just adequate to eject one ion must have a frequency spectral peak that is at least as wide as the above spread of frequencies. Such a waveform would then excite, at least to some extent, all ions with frequencies falling within the width of the peak, thus limiting the ejection resolution. For ions with low z-mode amplitudes, we can use Dunbar s (46) approximate expression for the average radial field strength,... [Pg.52]

Difference of the orbital radii of maximal electron density between the valence p and s orbitals from Reference 40. [Pg.7]

Antimony and bismuth lie at the fifth and sixth rows of the 15th group in the periodic table, and a variety of trivalent and pentavalent organic compounds derived from these elements have been reported. As shown in Table 1, antimony and bismuth have relatively small ionization potentials and electronegativities as well as large orbital radii. Due to these properties, elemental antimony and bismuth behave as metals, and the respective organic compounds possess relatively weak and polarized element-carbon bonds. These characteristics of antimony and bismuth have been... [Pg.425]

In order to compute the approximate magnitude of the term in r 6, it is necessary to know the polarizabilities and diamagnetic susceptibilities of the components considered in the interaction. Where these could not be found in the literature, they were calculated from the Slater average electron orbit radii using the relations... [Pg.132]

Waber J.T., Cromer D.T. Orbital Radii of Atoms and Ions HJ.Chem. Phys —1965.-V 42.-Xol2.-p. 4116-4123. [Pg.27]

Godovikov, Alexandr, Orbital Radii and Properties of Elements. Novosibirsk Nauka, 1977. [Pg.37]

Table 2 Atomic orbital radii for Fe in various oxidation states (a.u.)... Table 2 Atomic orbital radii for Fe in various oxidation states (a.u.)...
Using the orbit radii equation, calculate hydrogen s first seven electron orbit radii and then construct a scale model of those orbits. Use a compass and a metric ruler to draw your scale model on two sheets of paper that have been taped together. (Use caution when handling sharp objects.) Using the orbit energy equation, calculate the energy of each electron orbit and record the values on your model. [Pg.130]

The working principle of a helium-specific mass spectrometer leak detector is as follows [7], The mass spectrometer mainly consists of three parts an ion source, a deflection system and an ion collector. When the atoms pass the ionisation chamber of the detector, they are ionised to become positive ions. When these ions are then accelerated in the ionisation chamber, they obtain sufficient energy and enter into the magnetic field of the detector. These positive ions travel in a specific mbit in the magnetic field. As different ions have specific orbit radii only ions with the same orbit radius as that of the spectrometer can pass a narrow gap, as indicated by K in Figure 2.13, and reach the ion collector K to form an ion stream. [Pg.53]


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See also in sourсe #XX -- [ Pg.9 ]

See also in sourсe #XX -- [ Pg.207 ]




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Atomic orbitals radii

Bohr orbit, radius

Core orbital radius

Metallic Radii and Hybrid Bond Orbitals

Orbit radius

Orbit radius

Outer-shell orbital radius

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