2007
DOI: 10.1016/j.elspec.2007.06.003
|View full text |Cite
|
Sign up to set email alerts
|

Absolute photoionization cross sections with ultra-high energy resolution for Ar, Kr, Xe and N2 in inner-shell ionization regions

Help me understand this report

Search citation statements

Order By: Relevance

Paper Sections

Select...
2
1
1
1

Citation Types

6
45
0

Year Published

2010
2010
2023
2023

Publication Types

Select...
8

Relationship

0
8

Authors

Journals

citations
Cited by 56 publications
(51 citation statements)
references
References 53 publications
6
45
0
Order By: Relevance
“…The xenon pressure was 500 mTorr. This spectrum contains an isolated resonance 3d −1 5/2 -6p, for which Kato et al 16 natural linewidth, we infer an instrumental resolution of 1/3200 for the 100 l/mm grating at this photon energy. Different M1 pitch angles are required to optimize the monochromator focusing for the zero order and for the first order of the 100 and 200 l/mm gratings.…”
Section: Commissioning Of the Sxr Monochromatormentioning
confidence: 47%
“…The xenon pressure was 500 mTorr. This spectrum contains an isolated resonance 3d −1 5/2 -6p, for which Kato et al 16 natural linewidth, we infer an instrumental resolution of 1/3200 for the 100 l/mm grating at this photon energy. Different M1 pitch angles are required to optimize the monochromator focusing for the zero order and for the first order of the 100 and 200 l/mm gratings.…”
Section: Commissioning Of the Sxr Monochromatormentioning
confidence: 47%
“…4 for different values of the momentum transfer. While the velocity form approximately reproduces the 4s 3/2 :3d 3/2 line intensity ratio in the optical limit [29], the length form strongly underestimates this ratio, and GOS for 2p → 4s 3/2 transition is below the value of 7.84 × 10 −3 , calculated by the configuration interaction PWBA approach in the optical limit [26]. The Hartree-Fock 4 s orbital therefore more accurately describes the wave function close to the nucleus than in the outer atomic region.…”
Section: A Excitation Strengthsmentioning
confidence: 63%
“…According to Shaw et al [23], this is a reasonable assumption until E 0 > 350 eV, but our experimental setup detects scattered electrons at much larger angles where the importance of the exchange interaction is expected to increase. As shown by the photoabsorption data [29], the spin-orbit effect is mainly manifested by 2p 3/2 -2p 1/2 energy splitting, and relative intensities of corresponding lines obey the statistical ratio of 2:1 well. However, to describe the excitation strengths of overlapping resonances with different total angular momentum J more accurately (that populate different final states by the Auger decay), we have employed distorted-wave Born approximation (DWBA) with exchange [32].…”
Section: A Excitation Strengthsmentioning
confidence: 73%
“…The solid lines in the upper panel represent thê tting curves using Voigt functions, where the natural lifetime width is taken to be 113 meV 18) . The Gaussian width obtained from theˆtting is 39.96 meV.…”
Section: Measured Performance Of Bl-13amentioning
confidence: 99%
“…7). The spectrum wasˆtted using Voigt functions, where the natural lifetime width was taken to be 113 meV 18) . Using the Gaussian width obtained from the curveˆtting, E/DE was estimated to be about 10,000 at a photon energy of 401.1 eV.…”
Section: Photon-energy Resolutionmentioning
confidence: 99%