• Open Access

Current-horn suppression for reduced coherent-synchrotron-radiation-induced emittance growth in strong bunch compression

T. K. Charles, D. M. Paganin, A. Latina, M. J. Boland, and R. T. Dowd
Phys. Rev. Accel. Beams 20, 030705 – Published 31 March 2017

Abstract

Control of coherent synchrotron radiation (CSR)-induced emittance growth is essential in linear accelerators designed to deliver very high brightness electron beams. Extreme current values at the head and tail of the electron bunch, resulting from strong bunch compression, are responsible for large CSR production leading to significant transverse projected emittance growth. The Linac Coherent Light Source (LCLS) truncates the head and tail current spikes which greatly improves free electron laser (FEL) performance. Here we consider the underlying dynamics that lead to formation of current spikes (also referred to as current horns), which has been identified as caustics forming in electron trajectories. We present a method to analytically determine conditions required to avoid the caustic formation and therefore prevent the current spikes from forming. These required conditions can be easily met, without increasing the transverse slice emittance, through inclusion of an octupole magnet in the middle of a bunch compressor.

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  • Received 1 November 2016

DOI:https://doi.org/10.1103/PhysRevAccelBeams.20.030705

Published by the American Physical Society under the terms of the Creative Commons Attribution 4.0 International license. Further distribution of this work must maintain attribution to the author(s) and the published article’s title, journal citation, and DOI.

Published by the American Physical Society

Physics Subject Headings (PhySH)

Accelerators & Beams

Authors & Affiliations

T. K. Charles1,2, D. M. Paganin3, A. Latina3, M. J. Boland2,4, and R. T. Dowd1,2

  • 1School of Physics and Astronomy, Monash University, Clayton 3800, Victoria, Australia
  • 2Australian Synchrotron, 800 Blackburn Road, Clayton 3168, Victoria, Australia
  • 3European Organization for Nuclear Research (CERN), CH-1211 Geneva 23, Switzerland
  • 4School of Physics, University of Melbourne, Parkville 3010, Victoria, Australia

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Vol. 20, Iss. 3 — March 2017

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