Simulation study of halo formation in breathing round beams
Physical Review E - Statistical, Nonlinear, and Soft Matter Physics Volume 55 Issue 4
Page 4694-4705
published_at 1997-04
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Title ( eng ) |
Simulation study of halo formation in breathing round beams
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Creator |
Ikegami Masanori
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Source Title |
Physical Review E - Statistical, Nonlinear, and Soft Matter Physics
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Volume | 55 |
Issue | 4 |
Start Page | 4694 |
End Page | 4705 |
Abstract |
We study halo formation from cylindrical beams propagating in a uniform focusing channel. Of particular interest here are the breathing-mode oscillations excited by an initial beam-size mismatch. We develop a one-dimensional space-charge code which is simple but powerful in exploring the halo properties of breathing beams. After giving a brief description of two particle-core models, we apply the developed code to three different types of nonlinear phase-space distributions. Based on a number of multiparticle simulation runs, we show several interesting results useful for the design considerations of high-power linear machines. In particular, the intensity of halo current as well as the maximum extent of halos are self-consistently evaluated with the different sizes of initial mismatch and beam density. We then find that the halo extent normalized with the initial root-mean-squared beam size is only weakly dependent on the tune depression and that the halo intensity appears to increase with the degree of mismatch. It is further demonstrated that the beam core in phase space is roughly stable and, thus, most halo particles remain outside the core boundary. We also see that it is, in principle, possible to scrape halos, e.g., by means of a multicollimator system.
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Language |
eng
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Resource Type | journal article |
Publisher |
American Physical Society
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Date of Issued | 1997-04 |
Rights |
Copyright (c) 1997 American Physical Society.
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Publish Type | Version of Record |
Access Rights | open access |
Source Identifier |
[ISSN] 1539-3755
[DOI] 10.1103/PhysRevE.55.4694
[NCID] AA11558033
[DOI] http://dx.doi.org/10.1103/PhysRevE.55.4694
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