2002
DOI: 10.1006/adnd.2002.0886
|View full text |Cite
|
Sign up to set email alerts
|

PHOTOELECTRON ANGULAR DISTRIBUTION PARAMETERS FOR ELEMENTS Z=55 to Z=100 IN THE PHOTOELECTRON ENERGY RANGE 100–5000 eV

Help me understand this report

Search citation statements

Order By: Relevance

Paper Sections

Select...
1
1
1
1

Citation Types

4
99
1

Year Published

2011
2011
2023
2023

Publication Types

Select...
6
2

Relationship

0
8

Authors

Journals

citations
Cited by 201 publications
(104 citation statements)
references
References 8 publications
4
99
1
Order By: Relevance
“…No spectral O 2p valence band weight is found in the gap or at the chemical potential, thus indicating the absence of a potential gradient within the GAO film. The absence of spectral weight from interfacial Ti 3d charge carriers is due to the very small Ti 3d photoionization cross section for hard x rays [25,26].…”
Section: Resultsmentioning
confidence: 99%
See 1 more Smart Citation
“…No spectral O 2p valence band weight is found in the gap or at the chemical potential, thus indicating the absence of a potential gradient within the GAO film. The absence of spectral weight from interfacial Ti 3d charge carriers is due to the very small Ti 3d photoionization cross section for hard x rays [25,26].…”
Section: Resultsmentioning
confidence: 99%
“…Since the direct investigation of the interfacial 2DES by HAXPES is hindered by the small photoabsorption cross section of Ti 3d states, an indirect analysis based upon Ti 2p core levels, which exhibit a three orders of magnitude higher cross section [25,26], is the method of choice. As shown in Ref.…”
Section: Interfacial Confinement Of Charge Carriersmentioning
confidence: 99%
“…One can expect to suppress the spectral weight derived mainly from s states in the spectrum measured with the spolarized light. Meanwhile, the value of σ Ir 5d 5 /σ (O 2p 6 ) 4 for the s-polarized light is smaller (∼20 at hν = 8 keV in BL19LXU) than that for the p-polarized light (∼80 at hν = 8 keV in BL19LXU and ∼90 at hν = 6 keV in P09) [28]. As can be seen in Fig.…”
mentioning
confidence: 81%
“…The spectra were acquired at photon energies from 2 keV to 6 keV and, in some cases, to 9 keV; the slit width was of 0.5 mm for all the excitation photon energies. Atomic ratios of elements (I i,h ) relative to S were calculated from the intensity area of the detail spectra for each energy (A i,h ) employing photoionization cross-sections ( i,h ) tabulated in [57,58] and the ones extrapolated for the higher energies, and taking into account IMFP ( (KE) i ) calculated for FeS 2 and Fe 9 S 10 employing TPP−2M formula [38] and analyzer's transmission function (T(KE) i ) [40][41][42] using following equation…”
Section: Methodsmentioning
confidence: 99%