Generation of relativistic electron bunches with arbitrary current distribution via transverse-to-longitudinal phase space exchange

We propose a general method for tailoring the current distribution of relativistic electron bunches. The technique relies on a recently proposed method to exchange the longitudinal phase space emittance with one of the transverse emittances. The method consists of transversely shaping the bunch and...

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Main Authors: P. Piot, Y.-E Sun, J. G. Power, M. Rihaoui
Format: Article
Language:English
Published: American Physical Society 2011-02-01
Series:Physical Review Special Topics. Accelerators and Beams
Online Access:http://doi.org/10.1103/PhysRevSTAB.14.022801
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spelling doaj-3d2324935006439ba147e4ef495c630f2020-11-25T00:12:43ZengAmerican Physical SocietyPhysical Review Special Topics. Accelerators and Beams1098-44022011-02-0114202280110.1103/PhysRevSTAB.14.022801Generation of relativistic electron bunches with arbitrary current distribution via transverse-to-longitudinal phase space exchangeP. PiotY.-E SunJ. G. PowerM. RihaouiWe propose a general method for tailoring the current distribution of relativistic electron bunches. The technique relies on a recently proposed method to exchange the longitudinal phase space emittance with one of the transverse emittances. The method consists of transversely shaping the bunch and then converting its transverse profile into a current profile via a transverse-to-longitudinal phase-space-exchange beam line. We show that it is possible to tailor the current profile to follow, in principle, any desired distributions. We demonstrate, via computer simulations, the application of the method to generate trains of microbunches with tunable spacing and linearly ramped current profiles. We also briefly explore potential applications of the technique.http://doi.org/10.1103/PhysRevSTAB.14.022801
collection DOAJ
language English
format Article
sources DOAJ
author P. Piot
Y.-E Sun
J. G. Power
M. Rihaoui
spellingShingle P. Piot
Y.-E Sun
J. G. Power
M. Rihaoui
Generation of relativistic electron bunches with arbitrary current distribution via transverse-to-longitudinal phase space exchange
Physical Review Special Topics. Accelerators and Beams
author_facet P. Piot
Y.-E Sun
J. G. Power
M. Rihaoui
author_sort P. Piot
title Generation of relativistic electron bunches with arbitrary current distribution via transverse-to-longitudinal phase space exchange
title_short Generation of relativistic electron bunches with arbitrary current distribution via transverse-to-longitudinal phase space exchange
title_full Generation of relativistic electron bunches with arbitrary current distribution via transverse-to-longitudinal phase space exchange
title_fullStr Generation of relativistic electron bunches with arbitrary current distribution via transverse-to-longitudinal phase space exchange
title_full_unstemmed Generation of relativistic electron bunches with arbitrary current distribution via transverse-to-longitudinal phase space exchange
title_sort generation of relativistic electron bunches with arbitrary current distribution via transverse-to-longitudinal phase space exchange
publisher American Physical Society
series Physical Review Special Topics. Accelerators and Beams
issn 1098-4402
publishDate 2011-02-01
description We propose a general method for tailoring the current distribution of relativistic electron bunches. The technique relies on a recently proposed method to exchange the longitudinal phase space emittance with one of the transverse emittances. The method consists of transversely shaping the bunch and then converting its transverse profile into a current profile via a transverse-to-longitudinal phase-space-exchange beam line. We show that it is possible to tailor the current profile to follow, in principle, any desired distributions. We demonstrate, via computer simulations, the application of the method to generate trains of microbunches with tunable spacing and linearly ramped current profiles. We also briefly explore potential applications of the technique.
url http://doi.org/10.1103/PhysRevSTAB.14.022801
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