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Excitation, low-energy

Ah initio methods pose problems due a whole list of technical difficulties. Most of these stem from the large number of electrons and low-energy excited state. Core potentials are often used for heavier elements to ease the computational requirements and account for relativistic elfects. [Pg.288]

Convergence problems are very common due to the number of orbitals available and low-energy excited states. The most difficult calculations are generally those with open-shell systems and an unfllled coordination sphere. All the techniques listed in Chapter 22 may be necessary to get such calculations to converge. [Pg.288]

Many transition metal systems are open-shell systems. Due to the presence of low-energy excited states, it is very common to experience problems with spin contamination of unrestricted wave functions. Quite often, spin projection and annihilation techniques are not sufficient to correct the large amount of spin contamination. Because of this, restricted open-shell calculations are more reliable than unrestricted calculations for metal system. Spin contamination is discussed in Chapter 27. [Pg.288]

Chemical reactions of molecules at metal surfaces represent a fascinating test of the validity of the Born-Oppenheimer approximation in chemical reactivity. Metals are characterized by a continuum of electronic states with many possible low energy excitations. If metallic electrons are transferred between electronic states as a result of the interactions they make with molecular adsorbates undergoing reaction at the surface, the Born-Oppenheimer approximation is breaking down. [Pg.386]

Pelletier and Reber315 present new luminescence and low-energy excitation spectra of Pd(SCN)42 in three different crystalline environments, K2Pd(SCN)4, [K(18-crown-6)]2Pd(SCN)4, and (2-diethylammonium A -(2,6-dimethylphcnyl)acetamide)2Pd(SCN)4, and analyze the vibronic structure of the luminescence spectra, their intensities, and lifetimes as a function of temperature. The spectroscopic results are compared to the HOMO and LUMO orbitals obtained from density functional calculations to qualitatively illustrate the importance of the bending modes in the vibronic structure of the luminescence spectra. [Pg.582]

Nowadays it is widely accepted that there should be realized various phases of QCD in temperature (T) - density (ftp,) plane. When we emphasize the low T and high pp region, the subjects are sometimes called physics of high-density QCD. The main purposes in this field should be to figure out the properties of phase transitions and new phases, and to extract their symmetry breaking pattern and low-energy excitation modes there on the basis of QCD. On the other hand, these studies have phenomenological implications on relativistic heavy-ion collisions and compact stars like neutron stars or quark stars. [Pg.241]

It would be important to figure out the low energy excitation modes (Nambu-Goldstone modes) built on the ferromagnetic phase. The spin waves are well known in the Heisenberg model [10]. Then, how about our case [32] ... [Pg.259]

In support of this model, it is noted that LnFj - which has F ions on both octahedral and tetrahedral sites of a face-centred-cubic Ln -ion array - becomes a fast F -ion conductor below its melting point without any change in the cation array (O Keeffe and Hyde, 1975). This observation shows that some low-energy excitation other than the displacement of F ions into octahedral sites is operative, as is postulated with the cluster-rotation model for PbF2. [Pg.63]

Photochemistry and Radiation Chemistry of Liquid Alkanes Formation and Decay of Low-Energy Excited States... [Pg.365]

Characteristic Decomposition Modes of the Low-Energy Excited Aikane Moiecuies... [Pg.375]

For an average molecule, there are typically one or more low-energy excited states that may be reasonably well described as valence-MO-to-valence-MO single electronic excitations, and the language of spectroscopy reflects this point. Thus certain states are referred to as n TT, TT -> TT, etc., indicating the orbital from which the electron is excited on the left... [Pg.492]

This brings us to consider the size of excited molecules. In the low-energy excited states this remains very close to that of the ground state species, but it increases gradually with the energy of the states the higher excited states are more polarizable, until the limiting case of ionization is reached when the molecule becomes theoretically of infinite size. [Pg.77]

Low-energy excited states occur by promoting an electron from the 1tt orbital to the 2ttu orbital. The electronic configuration... [Pg.65]


See other pages where Excitation, low-energy is mentioned: [Pg.307]    [Pg.2208]    [Pg.33]    [Pg.196]    [Pg.216]    [Pg.289]    [Pg.33]    [Pg.126]    [Pg.179]    [Pg.68]    [Pg.564]    [Pg.25]    [Pg.71]    [Pg.922]    [Pg.163]    [Pg.194]    [Pg.63]    [Pg.231]    [Pg.245]    [Pg.582]    [Pg.119]    [Pg.119]    [Pg.37]    [Pg.177]    [Pg.63]    [Pg.393]    [Pg.395]    [Pg.458]    [Pg.480]    [Pg.486]    [Pg.502]    [Pg.30]    [Pg.71]    [Pg.132]    [Pg.164]   
See also in sourсe #XX -- [ Pg.228 , Pg.232 ]




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Excitation energy

Low energy

Low lying excitation energies

Low-energy excitation mode

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