Topic
Absorption (logic)
About: Absorption (logic) is a research topic. Over the lifetime, 5733 publications have been published within this topic receiving 236302 citations.
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TL;DR: In this paper, the electronic structure of epitaxially grown thin films was studied by in situ photoemission spectroscopy (PES) and x-ray-absorption (XAS) measurements.
Abstract: We have studied the electronic structure of epitaxially grown thin films of ${\mathrm{La}}_{1\ensuremath{-}x}{\mathrm{Sr}}_{x}{\mathrm{FeO}}_{3}$ by in situ photoemission spectroscopy (PES) and x-ray-absorption spectroscopy (XAS) measurements. The $\mathrm{Fe}$ $2p$ and valence-band PES spectra and the $\mathrm{O}$ $1s$ XAS spectra of ${\mathrm{LaFeO}}_{3}$ have been successfully reproduced by configuration-interaction cluster-model calculation and, except for the satellite structure, by band-structure calculation. From the shift of the binding energies of core levels, the chemical potential was found to be shifted downward as $x$ was increased. Among the three peaks in the valence-band spectra of ${\mathrm{La}}_{1\ensuremath{-}x}{\mathrm{Sr}}_{x}{\mathrm{FeO}}_{3}$, the peak nearest to the Fermi level $({E}_{F})$, due to the ``${e}_{g}$ band,'' was found to move toward ${E}_{F}$ and became weaker as $x$ was increased, whereas the intensity of the peak just above ${E}_{F}$ in the $\mathrm{O}$ $1s$ XAS spectra increased with $x$. The gap at ${E}_{F}$ was seen for all values of $x$. These results indicate that changes in the spectral line shape around ${E}_{F}$ are dominated by spectral weight transfer from below to above ${E}_{F}$ across the gap and are therefore highly nonrigid-bandlike changes.
112 citations
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TL;DR: In this paper, photoluminescence (PL) spectroscopy of pillar-suspended single-walled carbon nanotubes has been measured for temperatures between 300 and $5\phantom{\rule{0.3em}{0ex}}
Abstract: Photoluminescence (PL) and photoluminescence excitation (PLE) spectroscopy of pillar-suspended single-walled carbon nanotubes has been measured for temperatures between 300 and $5\phantom{\rule{0.3em}{0ex}}\mathrm{K}$. The atmospheric environment strongly affects the low-temperature luminescence. The PL intensity is quenched at temperatures below $\ensuremath{\sim}40\phantom{\rule{0.3em}{0ex}}\mathrm{K}$ for nanotubes in high vacuum, while nanotubes in helium ambient remain luminescent. The PL peak emission energy is only very weakly dependent on temperature, with a species-dependent blueshift upon cooling corresponding to a relative shift in bandgap of $\ensuremath{-}3\ifmmode\times\else\texttimes\fi{}{10}^{\ensuremath{-}5}\phantom{\rule{0.3em}{0ex}}{\mathrm{K}}^{\ensuremath{-}1}$ or less. The integrated peak intensities change by only a factor of 2, with linewidths showing a moderate temperature dependence. In PLE, the second absorption peak energy $({E}_{22})$ is also only weakly temperature dependent, with no significant shift and a limited reduction in linewidth upon cooling to $20\phantom{\rule{0.3em}{0ex}}\mathrm{K}$. In addition to the previously assigned nanotube PL peaks seen at room temperature, at least two distinct new classes of PL peaks are observed at cryogenic temperatures.
112 citations
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TL;DR: In this article, high-resolution polarized absorption and fluorescence spectra of an ion in LiY${\mathrm{F}}_{4}$ were measured at temperatures between 10 and 300 K.
Abstract: High-resolution polarized absorption and fluorescence spectra of ${\mathrm{Pr}}^{3+}$ in LiY${\mathrm{F}}_{4}$ were measured at temperatures between 10 and 300\ifmmode^\circ\else\textdegree\fi{}K. Energy-level assignments were made assuming electric-dipole transition selection rules for ${S}_{4}$ site symmetry. Forty-six energy levels of the $4{f}^{2}$ ground configuration were established, including 44 in the lowest nine multiplets. Crystal-field parameters were determined that gave a rms deviation of 15.8 ${\mathrm{cm}}^{\ensuremath{-}1}$ between 41 of the experimental energy levels and calculated values. The parameters were ${B}_{20}=488.9$, ${B}_{40}=\ensuremath{-}1043$, ${B}_{44}=1242$, ${B}_{60}=\ensuremath{-}42$, Re ${B}_{64}=1213$, and Im ${B}_{64}=22.5$ ${\mathrm{cm}}^{\ensuremath{-}1}$. These parameters were used to obtain the remaining energy levels, yielding a complete energy-level scheme for the $4{f}^{2}$ configuration of ${\mathrm{Pr}}^{3+}$. The crystal-field parameters for ${\mathrm{Pr}}^{3+}$ in LiY${\mathrm{F}}_{4}$ were compared to those for other ions in this host. A theoretical calculation of line intensities was performed in which the odd-fold crystal-field parameters were obtained from a lattice sum. Line intensities were measured and compared with theory.
112 citations
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01 Jan 1972TL;DR: The linear absorption coefficient as mentioned in this paper describes the magnitude of absorption after passing through one centimeter of matter, where the negative sign indicates that x-rays are reduced in intensity when passing through matter.
Abstract: X-rays are absorbed by materials in differing degrees; absorption coefficients are defined to quantitatively describe the magnitudes of this process. Let us assume that when an x-ray beam passes through a thin layer of material a fraction dN/N of the pulse rate N is absorbed. This fraction is proportional to the thickness dx of the layer
$$\frac{{d N}} {N} = - \mu dx$$
where μ is a proportionality factor. The negative sign indicates that x-rays are reduced in intensity when passing through matter. If the factor μ is independent of x, we then obtain by integration
$$N = {N_0}\exp \left[ { - \mu x} \right]$$
where N 0 is the pulse rate of the primary incident radiation and N the pulse rate after passage through the layer of the thickness x. The term μ is known as the linear absorption coefficient and, in the following, is therefore always written as μ l . It is
$$\frac{{mu _l}} = - {\{{1}} {N}{{dN}} {dx}\left[ {{\mu _l}} \right] = c{m^-1}$$
where μ l describes the magnitude of absorption after passage through one centimeter of matter.
111 citations
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TL;DR: Room temperature picosecond recovery of the optical transparency suggests the strong potential of Sr2CuO3 for all-optical switching and theoretical calculation indicates that the strong two-photon absorption is due to a very large dipole coupling between nearly degenerate one- and two- photon states.
Abstract: We report strong instantaneous photoinduced absorption in the quasi-one-dimensional Mott insulator ${\mathrm{Sr}}_{2}{\mathrm{CuO}}_{3}$ in the IR spectral region. The observed photoinduced absorption is to an even-parity two-photon state that occurs immediately above the absorption edge. Theoretical calculation based on a two-band extended Hubbard model explains the experimental features and indicates that the strong two-photon absorption is due to a very large dipole coupling between nearly degenerate one- and two-photon states. Room temperature picosecond recovery of the optical transparency suggests the strong potential of ${\mathrm{Sr}}_{2}{\mathrm{CuO}}_{3}$ for all-optical switching.
111 citations