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Energy bands dispersion

As indicated above, the ARUPS results were all taken at cryogenic temperatures. In fact the TTF-TCNQ energy band dispersion cannot be observed at RT because of the considerable vibration of the surface molecules in UHV. These surface thermal vibrations, facilitated by the weak intermolecular interactions, should induce a reduction of q at the surface. Indeed, if we model the ID energy dispersion of the TTF HQMQ and TCNQ LUMQ bands using Eq. (1.33), then we obtain ... [Pg.268]

Figure 1 2 10. The reduced Lifshitz parameter"z" - (ET - EF)/(EA- ET), where (EA- Er) is the full energy band dispersion in the c-axis direction, as a function of the number of holes in the G subband in A1 doped MgB2. The quantum uncertainty in the z value is indicated by the error bars that are given by D ( Figure 1 2 10. The reduced Lifshitz parameter"z" - (ET - EF)/(EA- ET), where (EA- Er) is the full energy band dispersion in the c-axis direction, as a function of the number of holes in the G subband in A1 doped MgB2. The quantum uncertainty in the z value is indicated by the error bars that are given by D (<r ,)/( , - r) where D is the deformation potential and (ct .) is the mean square boron displacement at T=0K associated with the E2g mode measured by neutron diffraction [139]. The Tc amplification by Feshbach shape resonance occurs in the O hole density range shown by the double arrow indicating where the 2D-3D ETT sweeps through the Fermi level because of zero point lattice motion, i.e., where the error bars intersect the z=0 line...
The next problem is the band filling and the position of the Fermi level Ep at zero Kelvin. We have seen that the supposed uniform degree of ionicity p can be defined from the stoichiometry (cf. Table 2). It allows us to define the number of charge carriers per molecule, (Ng/N), and therefore, from the energy band dispersion E(k), the wave vector kp which is associated with the Fermi level position. It follows that every orbital can hold two electrons ... [Pg.50]

In order to obtain the energy band dispersion from UPS experiments, we need to use the momentum conservation role as well as the energy conservation role upon photoelectron emission. A three-step model is generally adopted for the photoelectron spectroscopy process, which consists of an optical dipole excitation in the solid, followed by transport to the surface and emission to the vacuum [37, 38]. General assumptions are as follows (i) both the energy and momentum of the electrons are conserved during the optical transition, (ii) the momentum component parallel to the surface is conserved while the electron escapes through the surface, and (iii) the final continuum state in the solid is a parabolic free-electron-like band in a constant inner potential Vq,... [Pg.76]

Energy Band Dispersion and Band Transport Mobility... [Pg.79]

Figure 20.11 shows the energy band dispersion diagram and DOS for Srln204 [20]. The lowest band consisted of the Sr 4s atomic orbital (AO). The second, third, and fourth bands from the bottom were formed by the O 2s, Sr 4p, and In 4d AOs, respectively. The valence band consisted of 48 orbitals, which was the number that all the O 2p AOs for 16 0 atoms were fully occupied ( 73 through 120 in this numbering as shown in Figure 20.11). [Pg.636]

Fig. 18. One-dimensional energy dispersion relations for (a) armchair (5,5) nanotubes, (b) zigzag (9,0) nanotubes, and (c) zigzag (10,0) nano tubes. The energy bands with a symmetry arc non-degenerate, while the e-bands are doubly degenerate at a general wave vector k [169,175,176]. Fig. 18. One-dimensional energy dispersion relations for (a) armchair (5,5) nanotubes, (b) zigzag (9,0) nanotubes, and (c) zigzag (10,0) nano tubes. The energy bands with a symmetry arc non-degenerate, while the e-bands are doubly degenerate at a general wave vector k [169,175,176].
Because the ID unit cells for the symmorphic groups are relatively small in area, the number of phonon branches or the number of electronic energy bands associated with the ID dispersion relations is relatively small. Of course, for the chiral tubules the ID unit cells are very large, so that the number of phonon branches and electronic energy bands is also large. Using the transformation properties of the atoms within the unit cell transformation... [Pg.31]

Detailed electronic energy-band calculations have revealed the existence of appropriate surface states near the Fermi energy, indicative of an electronically driven surface instability. Angle-resolved photoemission studies, however, showed that the Fermi surface is very curved and the nesting is far from perfect. Recently Wang and Weber have calculated the surface phonon dispersion curve of the unreconstructed clean W(100) surface based on the first principles energy-band calculations of Mattheis and Hamann. ... [Pg.267]

The photoconductivity and absorption spectra of the multilayer polydiacetylene are shown in Fig. 22 [150]. The continuous and dotted line relate to the blue and red polymer forms respectively. Interpretation is given in terms of a valence to conduction band transition which is buried under the vibronic sidebands of the dominant exciton transition. The associated absorption coefficient follows a law which indicates either an indirect transition or a direct transition between non-parabolic bands. The gap energies are 2.5 eV and 2.6 eV for the two different forms. The transition is three dimensional indicating finite valence and conduction band dispersion in the direction perpendicular to the polymer chain. [Pg.35]


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See also in sourсe #XX -- [ Pg.67 , Pg.76 , Pg.79 , Pg.92 ]




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