By Jennifer Wick
Resource ebook for the Legend of the 5 jewelry position enjoying online game (1st edition).
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Two spectra calculated from Born-von Karman models folded with the experimental resolution [74Sal] are also to be seen. IFig. 4. Bi. Debye temperatures 0, calculated from the experimental spectrum of Fig. 2 Bi compared to experimental values [74Sal]. 32 24 I 16 t-t 8 0 20 40 60 80 I- 100 120 140 K 160 Fig. 5. Bi. of bismuth calculated from the experimental spectra of Figs, 2 Bi and 3 Bi [74Sal]. 3. Theoretical models The models reproduce only roughly the overall shape of the dispersion curves. Born-von Karrnan models: [67Sml, 73Cz1, 68Brl].
Specific heat, calculated to lowest order in the phonon anharmonicity (C, specific heat at constant pressure, C, total lattice specific heat, C, harmonic lattice specific heat) according to [71Mil]. 2 PhononenzustZnde: Cu [Lit. S. 180 Table 4. Cu. Phonon frequency spectraat various temperaturescalculated from Born-von Karman forceconstants. T 49 K 298K 296K 673K 1336K T 49 K 298K 296K 673K 1336K Ref. 67Nil 67Nil 76Lal 76Lal 76Lal Ref. 2713 r, 3. Theoretical models A reasonable fit to the dispersion curves is already obtained with a general nearest neighbour force model.
2 PhononenzustEnde: Ce Ce TLit. S. 16A. BZ: seep. 449. 1. Phonon dispersion Table 1. Ce. Measurements. Method Fig. Ref. 1 Ce Stassiset al. This relative softening is more pronounced in those branches whose initial slopes involve the elastic constants cI1 and cIz which enter into the bulk modulus. Thus it seemsthat premontory effectsof the y-x phasetransition are present in the room temperature dispersion curves. 5 s- Fig. 1. Ce. Measuredphonon dispersionof y-Ce at 295K. The solid lines wereobtainedfrom the Born-von Karman fit parametersgiven in Table3 Ce [79%1-j.