Abstract

Impedance-driven (but not only) coherent beam instabilities are usually studied analytically with the linearized Vlasov equation, ending up with an eigenvalue system to solve. The eigenvalues describe the beam oscillation mode-frequency shifts, leading in particular to intensity thresholds defined by the longitudinal mode coupling instability in the longitudinal plane and by the transverse mode coupling instability in the transverse plane in the absence of chromaticity. This can be directly compared to measurements in particular for the lowest modes and in the absence of tune spread. In the presence of nonlinearities or when higher-order modes are involved, this becomes quite difficult, if not impossible, and the coupling between the modes cannot be directly measured (or simulated) anymore. Another important observable is the intrabunch motion, which can be also accessed analytically thanks to the eigenvectors. To the author's knowledge, until now, the intrabunch signal has only been explained theoretically for independent longitudinal or transverse beam oscillation modes, i.e., when the bunch intensity is sufficiently low compared to the mode coupling threshold. It was never explained theoretically in detail when two (or more) modes are involved. For instance, no answers were already given to these questions: is (are) there some fixed point(s) when the transverse mode coupling instability starts? If yes, where is it (are they)? And what happens in the presence of mode decoupling? Any number of modes can be treated with the general approach discussed in this paper, which is based on the galactic Vlasov solver (which was previously successfully benchmarked against the pyheadtail macroparticle tracking code as concerns the beam oscillation mode-frequency shifts). However, to be able to clearly see what happens when the bunch intensity is increased, the simple case of two modes is discussed in detail. The purpose of this paper is to describe the different regimes, below, at, above the transverse mode coupling instability and also after the mode decoupling (as it happens sometimes), using a simple analytical model (where two modes are considered together), which helps to really understand what happens at each step. Better characterizing an instability is the first step before trying to find appropriate mitigation measures and push the performance of a particle accelerator. The evolution of the intrabunch motion with intensity is a fundamental observable with high-intensity high-brightness beams.

Highlights

  • The intrabunch signal for independent longitudinal or transverse beam oscillation modes, i.e., at sufficiently low intensity, has been explained analytically for impedancedriven coherent beam instabilities already several decades ago by Laclare in [1], and it has been observed and confirmed in many machines and macroparticle tracking simulation codes

  • The latter is defined as q 1⁄4 jmj þ 2k: with this definition, the radial mode number q represents the number of nodes of the superimposed intrabunch signals, which is a usual observable in particle accelerators

  • The GALACTIC Vlasov solver has been explained in detail in [2] for the case of a single bunch interacting with any impedance

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Summary

Metral*

CERN, 1211 Geneva, Switzerland (Received 24 July 2020; accepted 4 January 2021; published 22 January 2021). In the presence of nonlinearities or when higher-order modes are involved, this becomes quite difficult, if not impossible, and the coupling between the modes cannot be directly measured (or simulated) anymore Another important observable is the intrabunch motion, which can be accessed analytically thanks to the eigenvectors. To the author’s knowledge, until now, the intrabunch signal has only been explained theoretically for independent longitudinal or transverse beam oscillation modes, i.e., when the bunch intensity is sufficiently low compared to the mode coupling threshold. It was never explained theoretically in detail when two (or more) modes are involved. The evolution of the intrabunch motion with intensity is a fundamental observable with high-intensity high-brightness beams

INTRODUCTION
ME TRAL
GENERAL APPROACH WITH THE GALACTIC VLASOV SOLVER
SIMPLE MODEL CONSIDERING TWO HIGHER-ORDER MODES TOGETHER
CONCLUSIONS
Full Text
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