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1.
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G. Rumolo, A. Z. Ghalam, T. Katsouleas, C. K. Huang, V. K. Decyk, C. Ren, W. B. Mori, F. Zimmermann, and F. Ruggiero
Show Abstract
The interaction between a low-density electron cloud in a circular particle accelerator with a circulating charged particle beam is considered. The particle beam’s space charge attracts the cloud, enhancing the cloud density near the beam axis. It is shown that this enhanced charge and the image charges associated with the cloud charge and the conducting wall of the accelerator may have important consequences for the dynamics of the beam propagation. The tune shift due to the electron cloud is obtained analytically and compared to a new numerical model (QuickPIC) that is described here. Sample numerical results are presented and their significance for current and planned experiments is discussed.
Phys. Rev. ST Accel. Beams 6, 081002 (2003)
Cited 4 times
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2.
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B. S. Bauer, A. Y. Wong, V. K. Decyk, and G. Rosenthal
Show Abstract
A very intense electron plasma wave is resonantly excited at the top of a broad, flat density profile, by a longitudinal very-high-frequency electric field oscillating at the plasma frequency. Electric field energy densities W=Ẽ 2/4πncTe>103 are produced, along with copious electrons and ions of kinetic energy K>103Te. Reconstruction of the wave, from detailed measurements of electric field amplitude and phase, demonstrates wave breaking and accounts for the observed energetic particles.
Phys. Rev. Lett. 68, 3706 (1992)
Cited 3 times
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3.
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J. M. Dawson, V. K. Decyk, Robert W. Huff, I. Jechart, T. Katsouleas, J. N. Leboeuf, B. Lembege, R. M. Martinez, Y. Ohsawa, and S. T. Ratliff
Show Abstract
Computer simulations of magnetosonic waves, velocity-shell instabilities, and upper-hybrid heating show evidence of a general damping mechanism for large-amplitude electrostatic waves propagating perpendicular to a magnetic field: Particles trapped by a wave of frequency ω and phase velocity Vph see an electric field Vph×B, which accelerates them parallel to the wave front until the v×B force is large enough for detrapping. For ω≫ωc, velocities as large as (ω / 4ωc)Vph can be attained, within a time ωct≈ω / 4ωc.
Phys. Rev. Lett. 50, 1455 (1983)
Cited 18 times
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4.
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C. R. Menyuk, J. M. Dawson, V. K. Decyk, B. D. Fried, and G. J. Morales
Show Abstract
A wave propagating obliquely with respect to a magnetic field has many resonances, located at v∥=(ω-nΩ) / k∥. When they overlap, there is a transition between regular and stochastic particle motion, leading to a strong decrease in the final wave amplitude. Simulations confirm this result. In the regime where particle motion is regular, the usual trapping oscillations disappear as the angle of propagation increases, because of phase mixing of the bounce frequencies in different resonances.
Phys. Rev. Lett. 48, 1104 (1982)
Cited 2 times
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