Academic literature on the topic 'Core hole lifetime'

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Journal articles on the topic "Core hole lifetime"

1

Tohyama, Takami, and Kenji Tsutsui. "Spectral weight of resonant inelastic X-ray scattering in doped cuprates: Effect of core-hole lifetime." International Journal of Modern Physics B 32, no. 17 (2018): 1840017. http://dx.doi.org/10.1142/s0217979218400179.

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We examine the effect of core-hole lifetime on the spectral weight of resonant inelastic X-ray scattering (RIXS) in hole-doped cuprates. We calculate the spectral weight by using the exact diagonalization technique for a 4 × 4 doped Hubbard lattice and find that the spin-flip channel detecting single-magnon excitation is less sensitive to the core-hole lifetime while in the non-spin-flip channel the spectral weight is strongly dependent on the lifetime. In the latter, charge and two-magnon excitations predominately contribute to RIXS for short and long core-hole lifetimes, respectively. For a
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2

Ohno, Masahide. "Lifetime of core two-hole states in atoms." Journal of Electron Spectroscopy and Related Phenomena 143, no. 1 (2005): 13–19. http://dx.doi.org/10.1016/j.elspec.2004.09.019.

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3

Hämäläinen, Keijo, J. B. Hastings, D. Peter Siddons, and Lonny Berman. "X-Ray Absorption Spectroscopy beyond the Core-Hole Lifetime." Japanese Journal of Applied Physics 32, S2 (1993): 170. http://dx.doi.org/10.7567/jjaps.32s2.170.

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4

Carroll, T. X., N. Berrah, J. Bozek, et al. "Carbon1sphotoelectron spectrum of methane: Vibrational excitation and core-hole lifetime." Physical Review A 59, no. 5 (1999): 3386–93. http://dx.doi.org/10.1103/physreva.59.3386.

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5

Zhou, Ke-Jin, Satoshi Matsuyama, and Vladimir N. Strocov. "hv 2-concept breaks the photon-count limit of RIXS instrumentation." Journal of Synchrotron Radiation 27, no. 5 (2020): 1235–39. http://dx.doi.org/10.1107/s1600577520008607.

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Upon progressive refinement of energy resolution, the conventional resonant inelastic X-ray scattering (RIXS) instrumentation reaches the limit where the bandwidth of incident photons becomes insufficient to deliver an acceptable photon-count rate. Here it is shown that RIXS spectra as a function of energy loss are essentially invariant to their integration over incident energies within the core-hole lifetime. This fact permits RIXS instrumentation based on the hv 2-concept to utilize incident synchrotron radiation over the whole core-hole lifetime window without any compromise on the much fin
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6

Drube, W., A. Lessmann, and G. Materlik. "Reduced Core Hole Lifetime Broadening in Auger Final State Yield Spectra." Japanese Journal of Applied Physics 32, S2 (1993): 173. http://dx.doi.org/10.7567/jjaps.32s2.173.

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7

Nishihata, Y., O. Kamishima, Y. Kubozono, H. Maeda, and S. Emura. "XAFS in the high-energy region." Journal of Synchrotron Radiation 5, no. 3 (1998): 1007–9. http://dx.doi.org/10.1107/s0909049597016749.

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XAFS (X-ray absorption fine-structure) spectra were measured near K-absorption edges of Ce (40.5 keV), Dy (53.8 keV), Ta (67.4 keV) and Pt (78.4 keV). The blunt K-edge jump due to the finite lifetime of the core hole was observed. This makes it difficult to extract EXAFS (extended X-ray absorption fine-structure) functions at low k values. Local structure parameters can be evaluated from the EXAFS spectra above K-absorption edges in the high-energy region as well as from those above L III-edges. It was found that the finite-lifetime effect of the core hole is effectively taken into the photoel
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8

Ohno, Masahide. "Effect of the final-state interaction on the initial core–hole lifetime: the case of the 4s-hole lifetime of Sn metal." Journal of Electron Spectroscopy and Related Phenomena 130, no. 1-3 (2003): 7–17. http://dx.doi.org/10.1016/s0368-2048(02)00306-7.

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9

Riffe, D. M., G. K. Wertheim, and P. H. Citrin. "Different core-hole lifetime and screening in the surface of W(110)." Physical Review Letters 63, no. 18 (1989): 1976–79. http://dx.doi.org/10.1103/physrevlett.63.1976.

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10

Riffe, D. M., G. K. Wertheim, P. H. Citrin, and D. N. E. Buchanan. "Core-hole lifetime and screening are different in the surface of W(110)." Physica Scripta 41, no. 6 (1990): 1009–13. http://dx.doi.org/10.1088/0031-8949/41/6/066.

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