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Figure 5 b presents the change (dynamics) of the extinction cross section spectra within the fractal grows stages.
The Fano factors that are obtained from the nonradiative power spectra of the Au shell and the Au core of a nanomatryoshka are in accordance with those obtained from the absorption cross section spectra.
Two photon excitation cross section spectra of ECFP and EYFP were measured by Zipfel et al. [32].
Simulated extinction cross section spectra showing the effect of increasing the water percentage in the porous materials.
Thus, it is necessary to study the influence of the eccentricity on the absorption cross-section spectrum at the constant refractive index of the DLC.
b Total scattering cross-section spectrum (red solid line) of a core/shell NW (Ag core radius a c = 18 nm and Si shell radius a s = 73 nm) for TE-polarized light and scattering contributions of individual angular modes.
Förster's radius is calculated as 1where J = ∫ IDσAλ dλ is the overlap integral between the normalized donor emission spectrum ID and the acceptor absorption cross-section spectrum σA, and QD is the donor emission quantum yield in the absence of the acceptor.
e Normalized absorption cross-section spectra of the NW.
b Scattering cross-section spectra of the NW in the lossless case.
Absorption cross-section spectra, fluorescence quantum distributions and quantum yields, degrees of fluorescence polarisation, and fluorescence lifetimes are determined.
Figure 5 Simulated light extinction cross-section spectra for semi-ellipsoid- and parallelepiped-shaped Au nanoparticles on glass substrates.
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Justyna Jupowicz-Kozak
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