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Ionization molecular orbital formation

Change in the Ionization Cross Section and Splitting of theK L Line due to Molecular Orbital Formation... [Pg.41]

Molecular orbital calculations, whether by ab initio or semiempirical methods, can be used to obtain structures (bond distances and angles), energies (such as heats of formation), dipole moments, ionization energies, and other properties of molecules, ions, and radicals—not only of stable ones, but also of those so unstable that these properties cannot be obtained from experimental measurements." Many of these calculations have been performed on transition states (p. 279) this is the only way to get this information, since transition states are not, in general, directly observable. Of course, it is not possible to check data obtained for unstable molecules and transition states against any experimental values, so that the reliability of the various MO methods for these cases is always a question. However, our confidence in them does increase when (1) different MO methods give similar results, and (2) a particular MO method works well for cases that can be checked against experimental methods. ... [Pg.34]

The photoelectron spectrum is frequently discussed in terms of Koopmans theorem, which states that the ionization potentials (IPs) are approximately related to the energies of the canonical orbital found in molecular orbital calculations.106. The relationship is approximate because two factors are neglected the change in the correlation energy, and the reorganization energy, which is a consequence of the movement of electrons in response to the formation of a cation. The two quantities are approximately equal and opposite. [Pg.20]

Table 5 Average Absolute Deviations (in kcal/mol) from Experiment of Various Composite Ab Initio Molecular Orbital Methods for Ionization Energies, Electron Affinities, Proton Affinities, and Enthalpies of Formation in the G2/97 Test Set"... [Pg.162]

Molecular orbital computational analysis by PM3 CI UHF semiempirical methods have been used to support the contention that preferable HSOMO-LUMO interactions produce a favored biradical and explain the site selectivity in the sensitized photochemical [2 + 2] cycloadduct formation of 2-pyrones with electron-deficient ethylenes <92BCJ354>. The lowest ionization energies, dipole moment, and dominant electronic configurations of a 5-methylidenated version of 7-nitroso-oxazolo[4,5- ]cyclopenta[e]pyrimidine of unknown origin were calculated by the ADC(3) ab initio method <92CPHii>. An extensive semiempirical and ab initio investigation into the mechanism of oxidation of methanol by PQQ is cited in Section 7.22.12.4. [Pg.876]

Molecular orbital (MO) calculations have been used to obtain properties of molecules, ions, and radicals, some of which include bond distances, bond angles, heats of formation, ionization energies, and dipole moments. [Pg.628]

Exceptions do exist, however, and one must be particularly alert to substituent-induced changes in the direction of polarization, as well as to their affect upon the energy of the frontier molecular orbitals. For example, nitrone cycloaddition regiochemistry is generally LU controlled, leading to the production of C-S substituted isoxazolines in excellent yield. However, as the ionization potential of the nitrone decreases or the electron affinity of the dipolarophile increases, there exists an increased propensity for formation of the C-4 regioisomer. Eventually, a switch from LU to HO control occurs and substantial amounts of the C-4 isomer are produced (equation 14). [Pg.250]

Molecular-orbital calculations, whether by ab initio or semiempirical methods, can be used to obtain stmctures (bond distances and angles), energies (e.g., heats of formation), dipole moments, ionization energies, and other properties of molecules,... [Pg.35]


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See also in sourсe #XX -- [ Pg.41 , Pg.42 , Pg.43 , Pg.44 , Pg.45 ]




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Molecular orbital formation

Molecular orbitals formation

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