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Ionization energy definition

One more step provides an operational definition. The HOMO level lies, I = ionization energy, below the vacuum level, while the LUMO level lies, A = electron affinity, below it. Thus, the chemical hardness lies midway in the gap and usually is given in units of eV. [Pg.193]

To remove any possible confusion, we further refine the definition of ionization energy, and say that 7 is the minimum energy required to ionize 1 mol of a gaseous element. The ionization energy 7 relates to process (2) process (1) is additional. [Pg.70]

The potential energy curves of the species AB, AB+, and AB- are used in figure 4.1 to summarize the definitions of the adiabatic ionization energy and electron affinity of AB. Note that the arrows start and end at vibrational ground states (vibrational quantum number v = 0). [Pg.49]

Definition The ionization energy (IE) is defined as the minimum amount of energy which has to be absorbed by an atom or molecule in its electronic and vibrational ground states form an ion that is also in its ground states by ejection of an electron. [Pg.16]

Any molecule has an infinity of excited orbitals in the continuum above the first ionization energy. The electric dipole polarizability is connected partly with a few of these continuum orbitals and partly with the valence orbitals (7). If the simultaneous formation of empty orbitals of X, but with the continuum, it is reasonable to think of M being polarized by X. The population of the continuum orbitals of X is expected to be the more... [Pg.110]

Owing to lanthanide contraction, niobium and tantalum have virtually identical atomic rad (1.47 A) and close ionization energies (Nb6.67, Ta7.3eV), and usually display very similt chemical behavior. Some definite differences can however be noted these can usually be trace to the lower sensitivity of tantalum to reduction and to its higher affinity for dioxygen. lb tantalum-element multiple bonds are usually stabler, while MfiXg arrangements are so ft known only for niobium. [Pg.588]

R. D. Levine To answer the question of Prof. Lorquet, let me say that the peaks in the ZEKE spectra correspond to the different energy states of the ion. From the beginning one was able to resolve vibrational states, and nowadays individual rotational states of polyatomics have also been resolved. The ZEKE spectrum is obtained by a (weak) electrical-field-induced ionization of a high Rydberg electron moving about the ion. The very structure of the spectrum appears to me to point to the appropriate zero-order description of the states before ionization as definite rovibrational states of the ionic core, each of which has its own Rydberg series. Such a zero-order description is inverse to the one we use at far lower energies where each electronic state has its own set of distinct rovibrational states, known as the Bom-Oppenheimer limit. [Pg.647]

The relationship between the Mulliken definition and that of Jaffe can be shown quite amply. Taking Eq. 5.62 and substituting q +1, we know that the energy, E, of the system will be that of the +1 cation, or the first ionization energy. Likewise for <7=1. the energy will be the negative29 of the electron affinity, so ... [Pg.104]

Fig. 4.3 The allowed energies for an electron In a hydrogen atom, given by eqn 4.14. Two sets of transitions, with ni = 1 and 2, are also shown. The ionization energy is - ), tn energy required to take the electron from the n = 1 level to infinity, where (by definition) the energy is zero. Fig. 4.3 The allowed energies for an electron In a hydrogen atom, given by eqn 4.14. Two sets of transitions, with ni = 1 and 2, are also shown. The ionization energy is - ), tn energy required to take the electron from the n = 1 level to infinity, where (by definition) the energy is zero.
Fock matrix elements are actually calculated. The EHM Fock matrix elements are calculated from well-defined physical quantities (ionization energies) with the aid of well-defined mathematical functions (overlap integrals), and so are closely related to ionization energies and have definite quantitative values. [Pg.153]

Electronegativity is the ability of an atom or molecule to attract electrons. Why then is it (from one definition) the average of the ionization energy and the electron affinity (Eq. 7.32), rather than simply the electron affinity ... [Pg.519]

Figure 3. Definition of the ionization energy I for an isolated atom (A) and an atom in a molecule (B). In the first case, the electron is moved to infinite distance and does not interact with the cation. In the latter case, the charge of the electron is distributed in the vicinity of the cation. This results in a deformation of the electron cloud (in this case a tetrahedral one). The definition of an atom-in-molecule electron affinity is analogous. Figure 3. Definition of the ionization energy I for an isolated atom (A) and an atom in a molecule (B). In the first case, the electron is moved to infinite distance and does not interact with the cation. In the latter case, the charge of the electron is distributed in the vicinity of the cation. This results in a deformation of the electron cloud (in this case a tetrahedral one). The definition of an atom-in-molecule electron affinity is analogous.
This section will use gas-phase thermochemical data from Appendices 6 for molecules and 7 for radicals. These data include ionization energy (IE), electron affinity (EA), proton affinity (PA), gas-phase basicity (GB) and gas-phase acidity. Definitions of these parameters are given in Table 1.5. Some values of gas-phase basicities are given in Table 1.6. [Pg.75]

The work function is the energy required to remove an electron from the surface of a metal. How does this definition differ from that for ionization energy ... [Pg.578]


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See also in sourсe #XX -- [ Pg.16 ]

See also in sourсe #XX -- [ Pg.25 ]




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