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Mitigation of the hose instability in plasma-wakefield accelerators

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arxiv 1704.02188 v2 pith:PTME3ST7 submitted 2017-04-07 physics.plasm-ph

classification physics.plasm-ph
keywords instabilityacceleratorsbeamhoseplasma-wakefieldpropagationdistancesenergy
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Current models predict the hose instability to crucially limit the applicability of plasma-wakefield accelerators. By developing an analytical model which incorporates the evolution of the hose instability over long propagation distances, this work demonstrates that the inherent drive-beam energy loss, along with an initial beam energy spread detune the betatron oscillations of beam electrons, and thereby mitigate the instability. It is also shown that tapered plasma profiles can strongly reduce initial hosing seeds. Hence, we demonstrate that the propagation of a drive beam can be stabilized over long propagation distances, paving the way for the acceleration of high-quality electron beams in plasma-wakefield accelerators. We find excellent agreement between our models and particle-in-cell simulations.

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Cited by 1 Pith paper

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  1. TeV Electron Beams from Plasma Acceleration via Regenerative Cascading

    physics.acc-ph 2026-07 conditional novelty 7.0 of 10

    PIC simulations of regenerative cascading show a 45 GeV, 100 nC driver yields a 1.1 TeV, 0.12 nC electron bunch with 0.3% energy spread in two plasma stages totaling under 1 km.

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