2008
DOI: 10.1002/qua.21585
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Electron impact K‐shell ionization cross sections of atoms at relativistic energies

Abstract: ABSTRACT:We propose an extension of the modified simplified-improved-binaryencounter dipole (MRIBED) model (Uddin et al., Phys Rev A 2005, 72, 032715), incorporating both the ionic and relativistic corrections, to investigate the K-shell ionization of atomic targets with atomic numbers Z ϭ 1 Ϫ 92 for incident energies up to 2 GeV. We also revisit our earlier models, MBELL (Haque et al. Phys Rev A 2006, 73, 012708) and MKLV (Uddin et al. Eur Phys J D 2006, 37, 361), for the K-shell ionization at these ultra-r… Show more

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Cited by 12 publications
(3 citation statements)
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“…We calculate here the temporal profile of Kα radiation looking from the laser side of the target, and at the inner 160 μm cylinder. We account for Kα production cross section as a function of energy (Patoary et al, 2008) as well as for the self-absorption. In Figure 7, we give the number of 160 μm cylinder counts as a function of time for the 330 fs primary beam as well as for the next six refluxing steps from the back and front of the target.…”
Section: Appendix Temporal Behavior Of Kα Radiation and Of Energy Depmentioning
confidence: 99%
“…We calculate here the temporal profile of Kα radiation looking from the laser side of the target, and at the inner 160 μm cylinder. We account for Kα production cross section as a function of energy (Patoary et al, 2008) as well as for the self-absorption. In Figure 7, we give the number of 160 μm cylinder counts as a function of time for the 330 fs primary beam as well as for the next six refluxing steps from the back and front of the target.…”
Section: Appendix Temporal Behavior Of Kα Radiation and Of Energy Depmentioning
confidence: 99%
“…At each interval dx, the probability for Kα emission is also calculated using the cross-sections derived from Patoary et al (2008) and which are based on the Binary Encounter Approximation (BEA). The secondary electrons are set into motion at their point of emission.…”
Section: Present Calculationsmentioning
confidence: 99%
“…Many researchers like Haque et al 15 , Uddin et al 16 , Patoatry et al 17 , Kumar S and Kumar Y. 18 , Talukder et al 19 , etc.…”
Section: Introductionmentioning
confidence: 99%