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Frequency-Dependent and Spectral Properties

Frequency-Dependent and Spectral Properties the superposition will still be a plane-polarized wave... [Pg.158]

For an isolated spin-1 system, it is convenient to define sum and difference magnetizations [Eqs. (2.84)-(2.85)] in the J-B experiment. The decay of the difference (quadrupolar order) proceeds exponentially at a rate T q, while the sum (Zeeman order) recovers exponentially towards equilibrium at a different rate. The J-B experiment allows simulataneous determination of these rates from which Ji uJo) and J2 2ujo) can be separated. Table 5.1 briefly summarizes thermotropic liquid crystals in which spectral density measurements were reported. Figure 5.4 illustrates the temperature and frequency dependences of spectral densities of motion (in s by including the interaction strength Kq factor) for 5CB-di5. The result is fairly typical for rod-like thermotropic liquid crystals. The spectral densities increase with decreasing temperature in the nematic phase of 5CB. The frequency dependence of Ji uJo) and J2(2a o) indicate that molecular reorientation is likely not in the fast motion regime. However, the observed temperature dependence of the relaxation rates is opposite to what is expected for simple liquids. This must be due to the anisotropic properties (e.g., viscosity) of liquid crystals. [Pg.125]

The fundamental quantity for interferometry is the source s visibility function. The spatial coherence properties of the source is connected with the two-dimensional Fourier transform of the spatial intensity distribution on the ce-setial sphere by virtue of the van Cittert - Zemike theorem. The measured fringe contrast is given by the source s visibility at a spatial frequency B/X, measured in units line pairs per radian. The temporal coherence properties is determined by the spectral distribution of the detected radiation. The measured fringe contrast therefore also depends on the spectral properties of the source and the instrument. [Pg.282]

Uniform and pitting-type corrosion of various materials (carbon steels, stainless steels, aluminum, etc.) could be characterized in terms of noise properties of the systems fluctuation amplitudes in the time domain and spectral power (frequency dependence of power) of the fluctuations. Under-film corrosion of metals having protective nonmetallic coatings could also be characterized. Thus, corrosion research was enriched by a new and sufficiently correct method of looking at various aspects of the action of corrosive media on metals. [Pg.628]

High resolution and temperature dependance measurements were recorded for the lowest energy UV transition (230-250 nm) of thiophene. Based on these results, the first system of the UV spectrum is assigned to the 1/ 4 <-1/ 3 (B2) transition <82JCS(P2)76l). The results were confirmed by comparisons of the UPS and UV spectral properties of the Group 16 five-membered heterocycles. A vibrational progression in the 965 cm frequency mode is found to dominate. The absorption spectra between 225 nm and 246 nm has also been studied at elevated temperatures <85SA(A)1413>. At 296 K, 13 features are observed between 227.6 nm and 242.7 nm. At 573 K there is almost no vibrational structure in the system, while near 773 K the vibration structure is lost. [Pg.468]

The interactions of uncharged species have been touched upon above. Since the van der Waals forces dominate these interactions, they will be discussed at length in the final section of this chapter. It suffices here to say that these forces arise from the frequency-dependent electric and magnetic susceptibilities of the interacting species, and it is precisely these susceptibilities which are responsible for the spectral properties of the molecules comprising the particle. Thus, molecular (or chemical) specificity of particle interaction forces is of central importance. From another standpoint, this can be understood by considering an individual molecule as the limiting case of a particle. Then for the intermolecular van der Waals force to be consistent as two such particles (molecules) approach to the point of orbital overlap, their interaction must reduce to the relevant chemical interaction force which is fundamentally dependent upon chemical specificity. [Pg.121]

If near-field is to be used as a measurement tool for intrinsic fluorescence properties, then one needs to know the operating conditions or samples that are appropriate for lifetime and/or spectroscopic measurements. To address this question, the FDTD method was used to compute the spectral shift and fluorescence lifetime as a function of the tip-sample gap with the molecule directly under the center of the aperture. Fig. 18 shows these results. For a yg of about 3 x 10 /s, the frequency can red shift by about 10 GHz for distances less than 50 nm. This frequency shift is not important at room temperature where the vibronic bands are approximately 10 GHz wide. At low temperatures, the linewidths are in the 0.01 to 10 GHz range, and probe-induced frequency shifts should be measurable. The frequency dependence on distance was not calculated at the larger distances, 200-400 nm, relevant to the experiment of Moerner et al. [11] (Section 2.4.2). On the other hand, the fluorescence lifetime of high quantum yield molecules was predicted to be affected in first order throughout the near-field region. Bian et al. [25] point out that for systems with fast non-radiative decay channels, the perturbations by the probe may not be significant. [Pg.210]

The above characteristics make these systems very promising for radiation effect studies and in particular for metrological applications such as the measurement of the Rydberg constant directly in frequency units. One can indeed expect very narrow resonances between circular states, with spectral lines only quadratically sensitive to stray electric fields and frequencies depending only slightly upon the atomic ion core properties and being easily related to the hydrogen frequencies via the determination of very small quantum defects corrections. [Pg.30]


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Frequency Dependencies

Frequency dependence

Spectral dependencies

Spectral frequency

Spectral properties

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