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Scattering functions Subject

The mathematical basis of the Mie theory is the subject of this chapter. Expressions for absorption and scattering cross sections and angle-dependent scattering functions are derived reference is then made to the computer program in Appendix A, which provides for numerical calculations of these quantities. This is the point of departure for a host of applications in several fields of applied science, which are covered in more detail in Part 3. The mathematics, divorced from physical phenomena, can be somewhat boring. For this reason, a few illustrative examples are sprinkled throughout the chapter. These are just appetizers to help maintain the reader s interest a fuller meal will be served in Part 3. [Pg.82]

This article deals with one of the above mentioned subjects already treated in the 1940 s branched polymers. We present a survey of a number of scattering functions for special branched polymer structures. Hie basis of these model calculations is still the Flory-Stockmayer (FS) theory1,14,15) but now endowed with the more powerful technique of cascade theory which greatly simplifies the calculations. [Pg.4]

As we have just implied, solutions to the many-electron scattering problem, like solutions to the many-electron bound-state problems of quantum chemistry, are obtained in terms of products of one-electron functions, subject to constraints of spin, exchange antisymmetry (the Pauli principle), and possibly spatial (point... [Pg.121]

Elastically scattered radiation reaching a detector from different scattering centers in a macromolecule will be subject to interference effects, provided the dimensions of the macromolecule are comparable to or larger than the wavelength of the radiation (22). The Debye scattering function P(u) describes the variation, arisir from intramolecular interference effects, of the scattered... [Pg.514]

Fig. 2.29 (a) Wide-angle X-ray scattering curve for a sample of perdeuterated poly (vinylchloride) (b) Neutron scattering function for the sample subjected to X-ray scattering in the left hand image (Reproduced from Mitchell 2011)... [Pg.61]

The scattering function I q, t) at a given time in the late-stage SD was subjected to a Fourier inversion in 3D space to obtain y(r), the results of which are used for a plot shown in Fig. 4 [24]. We can determine R from the slope and intercept at r = 0. In order to compare R with that determined from the direct real-space analysis, we need to know . For this purpose, we have developed an algorithm to evaluate distribution function of H and K [25]. [Pg.135]

Equation [61] is only valid in the asjmiptotic Q" tail of the scattering function. A full treatment yields the dynamic stmc-tme factor also in the low Q limit. At r=0, this leads to the well-known Debye function (eqn [20]). Figure 33 displays the temporal evolution of the quasielastic SANS. The uppermost curve corresponds to the Debye function, while the lower curves visualize the decay of the sHucture factor due to the Rouse relaxation. For t —> CX> all internal chain correlations are lost and the stmcture factor displays the Gaussian density profile within a polymer coil. We note that the polymer coil in addition to the Rouse modes is also subject of translational diffusion. [Pg.350]

Radiation probes such as neutrons, x-rays and visible light are used to see the structure of physical systems tlirough elastic scattering experunents. Inelastic scattering experiments measure both the structural and dynamical correlations that exist in a physical system. For a system which is in thennodynamic equilibrium, the molecular dynamics create spatio-temporal correlations which are the manifestation of themial fluctuations around the equilibrium state. For a condensed phase system, dynamical correlations are intimately linked to its structure. For systems in equilibrium, linear response tiieory is an appropriate framework to use to inquire on the spatio-temporal correlations resulting from thennodynamic fluctuations. Appropriate response and correlation functions emerge naturally in this framework, and the role of theory is to understand these correlation fiinctions from first principles. This is the subject of section A3.3.2. [Pg.716]

The Newns-Anderson approximation successfully accounts for the main features of bonding when an adsorbate approaches the surface of a metal and its wave functions interact with those of the metal. It can also be used to describe features of the dynamics in the scattering of ions, atoms and molecules on surfaces. In particular the neutralization of ions at surfaces is well understood in this framework. The subject is beyond the scope of this book and the reader is referred to the literature [J.K. N0rskov, J. Vac. Sci. Technol. 18 (1981) 420],... [Pg.242]

From the observed correlation function the scattering pattern is obtained by Fourier transformation. As Eq. (2.31) is subjected to the Fourier transform, it will only act on the correlation function of the template because hu (a) is no function of r. With Eq. (2.29) we obtain the expected result... [Pg.37]

The data collected are subjected to Fourier transformation yielding a peak at the frequency of each sine wave component in the EXAFS. The sine wave frequencies are proportional to the absorber-scatterer (a-s) distance /7IS. Each peak in the display represents a particular shell of atoms. To answer the question of how many of what kind of atom, one must do curve fitting. This requires a reliance on chemical intuition, experience, and adherence to reasonable chemical bond distances expected for the molecule under study. In practice, two methods are used to determine what the back-scattered EXAFS data for a given system should look like. The first, an empirical method, compares the unknown system to known models the second, a theoretical method, calculates the expected behavior of the a-s pair. The empirical method depends on having information on a suitable model, whereas the theoretical method is dependent on having good wave function descriptions of both absorber and scatterer. [Pg.70]

In the cellular multiple scattering model , finite clusters of atoms are subjected to condensed matter boundary conditions in such a manner that a continuous spectrum is allowed. They are therefore not molecular calculations. An X type of exchange was used to create a local potential and different potentials for up and down spin-states could be constructed. For uranium pnictides and chalcogenides compounds the clusters were of 8 atoms (4 metal, 4 non-metal). The local density of states was calculated directly from the imaginary part of the Green function. The major features of the results are ... [Pg.282]

Equation (8.43) provides us with an approximate criterion, subject to the limitations of diffraction theory, for when a finite cylinder may be regarded as effectively infinite if R > 10, say, there will be comparatively little light scattered in directions other than those in a plane perpendicular to the cylinder axis. The greater is R, the more the scattered light is concentrated in this plane in the limit of indefinitely large R, no light is scattered in directions other than in this plane. We may show this as follows. The phase function may be written in the form p(0, ) = G(0, )F(0, ), where... [Pg.211]


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