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Please use this identifier to cite or link to this item: http://dspace.bits-pilani.ac.in:8080/jspui/xmlui/handle/123456789/9520
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dc.contributor.authorKumar, A. V. Praveen-
dc.date.accessioned2023-03-06T08:54:12Z-
dc.date.available2023-03-06T08:54:12Z-
dc.date.issued2011-11-
dc.identifier.urihttps://www.sciencedirect.com/science/article/pii/S0168900211010229-
dc.identifier.urihttp://dspace.bits-pilani.ac.in:8080/xmlui/handle/123456789/9520-
dc.description.abstractThe bunch size and crossing angle planned for CERN's compact linear collider CLIC dictate that crab cavities on opposing linacs will be needed to rotate bunches of particles into alignment at the interaction point if the desired luminosity is to be achieved. Wakefield effects, RF phase errors between crab cavities on opposing linacs and unpredictable beam loading can each act to reduce luminosity below that anticipated for bunches colliding in perfect alignment. Unlike acceleration cavities, which are normally optimised for gradient, crab cavities must be optimised primarily for luminosity. Accepting the crab cavity technology choice of a 12 GHz, normal conducting, travelling wave structure as explained in the text, this paper develops an analytical approach to optimise cell number and iris diameter.en_US
dc.language.isoenen_US
dc.publisherElsevieren_US
dc.subjectEEEen_US
dc.subjectCrab cavityen_US
dc.subjectX-banden_US
dc.subjectLuminosityen_US
dc.titleCLIC crab cavity design optimisation for maximum luminosityen_US
dc.typeArticleen_US
Appears in Collections:Department of Electrical and Electronics Engineering

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