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Transition temperature magnetic field

Table 1 Cation and anion S values basic structural motives Weiss constants transition temperatures, magnetic ordering critical fields of the salts based on metallocenium and on metal bisdichalcogenate complexes ... [Pg.104]

Figure 6. Magnetization jump at the martensitic transition in magnetic fields of 3 and 5 T. For 0 < x < 0.16 compositions M(T) dependencies were measured upon heating. For the x = 0.19 composition, a temperature hysteresis loop of the magnetization observed at martensitic transition is shown. Figure 6. Magnetization jump at the martensitic transition in magnetic fields of 3 and 5 T. For 0 < x < 0.16 compositions M(T) dependencies were measured upon heating. For the x = 0.19 composition, a temperature hysteresis loop of the magnetization observed at martensitic transition is shown.
We say that a phase transition does occur and is accompanied by a symmetry breaking when the Gibbs state , computed at fixed values of the external parameters of the theory (such as temperature, magnetic field, chemical potential) is a KMS state without being extremal KMS, and moreover can be decomposed into pure thermodynamic phases (hence extremal KMS states) which have a lower symmetry than that of the interactions one starts from it is understood that in the course of the computation of the thermodynamic limit one chooses the boundary conditions in such a way that itself inherits the full symmetry of the interactions. [Pg.353]

Consider how the change of a system from a thennodynamic state a to a thennodynamic state (3 could decrease the temperature. (The change in state a —> f3 could be a chemical reaction, a phase transition, or just a change of volume, pressure, magnetic field, etc). Initially assume that a and (3 are always in complete internal equilibrium, i.e. neither has been cooled so rapidly that any disorder is frozen in. Then the Nemst heat... [Pg.371]

Fig. 12. UV-visible absorption and VTMCD spectra of the [Fe3S4] cluster in wild-type P. furiosus Fd. The absorption spectrum was recorded at room temperature and the MOD spectra were recorded at 1.67, 4.22, 9.0, 15.8, and 51.0 K (all transitions increasing in intensity with decreasing temperature) with an applied magnetic field of 4.5 T. The band at 314 nm in the absorption spectrum (marked with an asterisk) is due to excess dithionite. Fig. 12. UV-visible absorption and VTMCD spectra of the [Fe3S4] cluster in wild-type P. furiosus Fd. The absorption spectrum was recorded at room temperature and the MOD spectra were recorded at 1.67, 4.22, 9.0, 15.8, and 51.0 K (all transitions increasing in intensity with decreasing temperature) with an applied magnetic field of 4.5 T. The band at 314 nm in the absorption spectrum (marked with an asterisk) is due to excess dithionite.
Fig. 13. VTMCD spectra of [Fe3S4] clusters in wild type and mutant forms of P. furiosus Fd. In each case the spectra shown were recorded at temperatures between 1.5 and 50 K with an applied magnetic field of 4.5 or 6 T (all transitions increase in intensity with decreasing temperature). Fig. 13. VTMCD spectra of [Fe3S4] clusters in wild type and mutant forms of P. furiosus Fd. In each case the spectra shown were recorded at temperatures between 1.5 and 50 K with an applied magnetic field of 4.5 or 6 T (all transitions increase in intensity with decreasing temperature).

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