Analytic model for halo formation in high current ion linacs.

Analytic model for halo formation in high current ion linacs.
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DOI:
10.1103/physrevlett.73.1247
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发表时间:
1994-08
影响因子:
8.6
通讯作者:
R. Gluckstern
R. Gluckstern
中科院分区:
物理与天体物理1区
文献类型:
--
作者:
R. Gluckstern

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We construct an azimuthally symmetric 2D model for halo formation in high current ion linacs. The driving term, a breathing'' oscillation caused by a transverse mismatch along the linac, leads to growth of ion amplitudes in the core through the parametric resonance. As the ion amplitude grows, its wave number increases, enhancing the resonance. This leads to the formation of a halo surrounding the core. We explore the dependence of this mechanism on the tune depression and the size of the mismatch. The model agrees well with simulations at Los Alamos, but does not yet include the effects of chaos observed in the simulations as the tune depression becomes severe.