Resonance, Chaos and Halo Formation in Space Charge Dominated Beams

  • The nonlinear resonance, chaos and halo formation in space charge dominated beams have been studied. The results for the range of the nonlinear resonance versus space charge effects, and the space charge thresholds of halo formation excited by nonlinear resonance are derived. Some numerical results are also given.
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  • [1] Jamtson R A. LA-UR-93-1209. Los Alamos National Laboratory Rcport, 1993[2] Glucksturn R I.Phys. Rev. Lett.,1994. 73(9):1247-1250[3] Lagniel J M. Nucl. lnstrum. Methods Phys. Res,1994, A345(3):405-410[4] Okarncsto H. Ikegami M. Phys. Rev. E.,1997, 55(4):4694-4705[5] Fink、’,CHEN C, Marable W Y. Phys Rev. E.,1997, 55(6):7557-7564[6] Fedotov A V, C}luckstum R 1,Kumnnoy S S et al. In: Pros. of XIX Int. Linear Accel. Conf.,ChicaKo, 1998[7] Lagniel J M, Nath S. In: Proc. of Sixth European Particle Accel. Conf.,Stockholm, Sweden, 1998[8] Ikegami M. Phys. Rev. E,1999, 59(2):2331卜一2338[9] Olsen D. Bieaat Dynamite Newsletter. In: Hirata K, Jowett J M, Lee S Y ed. 1998. (18):17[10] HLiANG Zhif3in, CHEN Yin Pao. High Energy Phys. and Nucl. Phys. (in Chinese),1998, 22(10):943--950 (黄志斌,陈银宝.高能物理与核物理,1998,22(10):943-950)[11] Reiser M. Thmry and Design of Charged Particle Beams. New York: John Wiley Sons Inc.1994. 241-243, 226-228
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CHEN YinBao and HUANG ZhiBin. Resonance, Chaos and Halo Formation in Space Charge Dominated Beams[J]. Chinese Physics C, 2000, 24(6): 560-566.
CHEN YinBao and HUANG ZhiBin. Resonance, Chaos and Halo Formation in Space Charge Dominated Beams[J]. Chinese Physics C, 2000, 24(6): 560-566. shu
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Received: 1999-04-09
Revised: 1900-01-01
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Resonance, Chaos and Halo Formation in Space Charge Dominated Beams

    Corresponding author: CHEN YinBao,
  • China Institute of Atomic Energy, Beijing 102413, China

Abstract: The nonlinear resonance, chaos and halo formation in space charge dominated beams have been studied. The results for the range of the nonlinear resonance versus space charge effects, and the space charge thresholds of halo formation excited by nonlinear resonance are derived. Some numerical results are also given.

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