Please use this identifier to cite or link to this item: https://hdl.handle.net/10316/4512
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dc.contributor.authorTavora, L. M. N.-
dc.contributor.authorGilboy, W. B.-
dc.contributor.authorMorton, E. J.-
dc.date.accessioned2008-09-01T11:08:22Z-
dc.date.available2008-09-01T11:08:22Z-
dc.date.issued2001en_US
dc.identifier.citationRadiation Physics and Chemistry. 61:3-6 (2001) 527-529en_US
dc.identifier.urihttps://hdl.handle.net/10316/4512-
dc.description.abstractWhen energetic electrons are incident on high atomic number absorbers, a substantial fraction is back-scattered. This phenomenon is responsible for several undesirable effects in X-ray tubes, in particular a reduction in the X-ray output. The extent of this shortfall has been estimated by using Monte Carlo simulation to start electrons at increasing depth inside the anode, the results indicating that an output enhancement of nearly 50% could be achieved in principle if the electrons wasted in back-scatter events could be trapped inside a tungsten anode. To test this idea a further set of simulations were done for a novel anode geometry. Results showed that X-ray tube efficiencies might be substantially enhanced by this approach.en_US
dc.description.urihttp://www.sciencedirect.com/science/article/B6TVT-43P41Y7-30/1/526566f6ea15332c302cdad2886e583den_US
dc.format.mimetypeaplication/PDFen
dc.language.isoengeng
dc.rightsopenAccesseng
dc.subjectX-ray tubeen_US
dc.subjectAnode designen_US
dc.subjectMonte Carlo simulationen_US
dc.titleMonte Carlo studies of a novel X-ray tube anode designen_US
dc.typearticleen_US
dc.identifier.doi10.1016/S0969-806X(01)00322-X-
item.openairecristypehttp://purl.org/coar/resource_type/c_18cf-
item.openairetypearticle-
item.cerifentitytypePublications-
item.grantfulltextopen-
item.fulltextCom Texto completo-
item.languageiso639-1en-
Appears in Collections:FCTUC Física - Artigos em Revistas Internacionais
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