2007
DOI: 10.1116/1.2794067
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Extracting the Boersch effect contribution from experimental energy spread measurements for Schottky electron emitters

Abstract: Energy spread is critical to the performance of probe forming systems working at high resolution. The energy spread in the probe is the convolution of the intrinsic spread upon emission and the broadening due to Coulomb interactions in the beam. In order to optimize the design, the two need to be distinguished. The Boersch effect in a Schottky electron gun is difficult to calculate because of the low initial velocity at emission and the strong potential gradient. This article presents a method to extract it fr… Show more

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Cited by 25 publications
(3 citation statements)
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“…When V E was 3,000 and 3,500 V, the FWHMs of the energy spread were measured and found to be 1.27 eV ( J Ω = 92 μ A/sr) and 1.47 eV ( J Ω = 137 μ A/sr), respectively, where J Ω is the angular current density. We assume that the angular current density increases as the electric field increases, resulting in a broadened energy distribution owing to electron-electron interaction, known as the Boersch effect (Bronsgeest et al, 2007). Therefore, when the parameter q is increased by V E in the theoretical TED, the ES model becomes inaccurate.…”
Section: Resultsmentioning
confidence: 99%
“…When V E was 3,000 and 3,500 V, the FWHMs of the energy spread were measured and found to be 1.27 eV ( J Ω = 92 μ A/sr) and 1.47 eV ( J Ω = 137 μ A/sr), respectively, where J Ω is the angular current density. We assume that the angular current density increases as the electric field increases, resulting in a broadened energy distribution owing to electron-electron interaction, known as the Boersch effect (Bronsgeest et al, 2007). Therefore, when the parameter q is increased by V E in the theoretical TED, the ES model becomes inaccurate.…”
Section: Resultsmentioning
confidence: 99%
“…In Ref. 28,Bronsgeest et al presented the way to distinguish the Boersch effect from the intrinsic energy distribution. Since the intrinsic energy distribution is a function of temperature, work function, and the field at the emitter, this distribution can be assumed to be the same in case of the suppressorless configuration.…”
Section: Discussionmentioning
confidence: 99%
“…During the last few decades, brightness limitations caused by Coulomb interactions have been the subject of many experimental 18,34,53,54 and theoretical studies [55][56][57][58][59][60][61][62][63][64] considering continuous electron sources as well as pulsed photoemitters.…”
Section: Introductionmentioning
confidence: 99%