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Sommerfeld value

Adequate prediction of the thermal conductivity for pure metals can be made by means of the Wiedeman-Franz law which states that the ratio of the thermal conductivity to the product of the electrical conductivity and the absolute temperature is a constant. This ratio for high-conductivity metals extrapolates essentially to the Sommerfeld value of 2.449 x 10" W f2/K at 0 K, but falls considerably below it at higher temperatures. High-purity aluminum and copper exhibit peaks in thermal conductivity between 20 to 50 K, but these peaks are rapidly suppressed with increased impurity levels and cold work of the metal. Some metals including Monel, Inconel, stainless steel, and structural and aluminum alloys show a steady decrease in thermal conductivity with a decrease in temperature. [Pg.1296]

HTSC high-temperature To Sommerfeld value of the Lorentz... [Pg.108]

Figure 9 Ratio of mon-dlmensional minimum film thickness calculated according to the Reynolds and half-Sommerfeld boundary conditions as a function of the half-Sommerfeld value. Figure 9 Ratio of mon-dlmensional minimum film thickness calculated according to the Reynolds and half-Sommerfeld boundary conditions as a function of the half-Sommerfeld value.
Wiedemann-Franz relationship X q T = L (X = thermal conductivity, q = electrical resistivity) was equal to about twice the Sommerfeld value (Lq = 2.45 x lO V -K" ). This shows that phonons play a significant part in the thermal conductivity of NdSe. Magnons may also be important at low temperatures, Zhuze et al. [7]. [Pg.128]

This equation, including succeeding terms, was obtained originally by Sommerfeld from relativistic considerations with the old quantum theory the first term, except for the screening constant sQ> has now been derived by Heisenberg and Jordan] with the use of the quantum mechanics and the idea of the spinning electron. The value of the screening constant is known for a number of doublets, and it is found empirically not to vary with Z. [Pg.678]

The y values (Sommerfeld constants) for some metals are reported in Table 3.1. [Pg.73]

Fine structure. Evidently the set of term values is exactly the same as on the usual theory but the quantum numbers are different, making new transitions possible and changing the intensities of the fine structure. The hydrogen fine structiure is so obscured by the natural breadth of the lines that no information can be obtained from it, and we must turn to the spectrum of ionized helium. For Paschen s data the reader is referred to Sommerfeld, figures 89-92. The only measurements of value for the... [Pg.4]

Fig. 58. Composition dependence of the density of states N(E ) at the Fermi level ( ) of Y Lui-xl I C calculated by CPA, experimental data for the Sommerfeld parameter /n end the phenomenologically extracted values of the electron-phonon coupling constant Ae. ph (in this article usually written as Apt,), using eq. (9). Fig. 58. Composition dependence of the density of states N(E ) at the Fermi level ( ) of Y Lui-xl I C calculated by CPA, experimental data for the Sommerfeld parameter /n end the phenomenologically extracted values of the electron-phonon coupling constant Ae. ph (in this article usually written as Apt,), using eq. (9).
There were lines in the spectra corresponding to transitions other than simply between two n values (cf. Eq. 4.14). This was rationalized by Sommerfeld in 1915, by the hypothesis of elliptical rather than circular orbits, which essentially introduced a new quantum number k, a measure of the eccentricity of the elliptical orbit. Electrons could have the same n but different k s, increasing the variety of possible electronic transitions k is related to what we now call the azimuthal quantum number, Z l = k — 1). [Pg.97]

With these new, accurate data, Smekal,4 Coster,8 Dauvillier8 and Wentzel6 have constructed atomic systems to explain the source of each known emission line. The systems are based on the Bohr-Sommerfeld theory of the origin of characteristic X-radiation. In developing and discussing their systems, these investigators have used the values of the L absorption limits measured by us. Certain criticisms have been made of a few of our values. It has therefore seemed desirable to measure some of the limits again. [Pg.1]

For a brief period the Sommerfeld model enjoyed general acceptance in chemistry. The most powerful argument in its favour was the obvious agreement with the periodic law, e.g. by providing for 2 and Figure 2.8 Sommer-8 electrons in the first two shells, respectively. The feld model of the Ne predicted number of orbits for higher values of n are atom. also in agreement with the periodic law. [Pg.29]

The Kepler model was ceased upon by Sommerfeld to account for the quantized orbits and energies of the Bohr atomic model. By replacing the continuous range of classical action variables, restricting them to discrete values of... [Pg.83]

We shall frequently encounter cases with angular momentum values of / = and / = 1. For J =, such as for electron spin, there are only two possible orientations of the angular momentum they are depicted in Figure 9. Commemorative of the old Bohr-Sommerfeld theory, we say that the angular momentum is oriented parallel to the z axis in the case of M = + and antiparallel for M = - j. [Pg.121]


See other pages where Sommerfeld value is mentioned: [Pg.1127]    [Pg.1131]    [Pg.114]    [Pg.133]    [Pg.195]    [Pg.1127]    [Pg.1131]    [Pg.114]    [Pg.133]    [Pg.195]    [Pg.4]    [Pg.56]    [Pg.63]    [Pg.686]    [Pg.711]    [Pg.711]    [Pg.724]    [Pg.249]    [Pg.7]    [Pg.160]    [Pg.167]    [Pg.301]    [Pg.198]    [Pg.198]    [Pg.280]    [Pg.282]    [Pg.692]    [Pg.92]    [Pg.161]    [Pg.163]    [Pg.13]    [Pg.26]    [Pg.240]    [Pg.297]    [Pg.299]    [Pg.106]    [Pg.326]    [Pg.163]   
See also in sourсe #XX -- [ Pg.195 ]




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