DocumentCode
3210110
Title
Modeling TeV Class Plasmaa Fterburners
Author
Huang, C. ; Clayton, C. ; Johnson, D. ; Joshi, C. ; Lu, W. ; Mori, W. ; Zhou, M. ; Barnes, C. ; Decker, F.J. ; Hogan, M. ; Iverson, R. ; Deng, S. ; Katsouleas, T. ; Muggli, P. ; Oz, E.
Author_Institution
(UCLA), Los Angeles, CA 90095, USA, huangck@ee.ucla.edu
fYear
2005
fDate
16-20 May 2005
Firstpage
2666
Lastpage
2668
Abstract
Plasma wakefield acceleration can sustain acceleration gradients three orders of magnitude larger than conventional RF accelerator. In the recent E164X experiment, substantial energy gain of about 3 − 4 GeV has been observed. Thus, a plasma afterburner, which has been proposed to double the incoming beam energy for a future linear collider, is now of great interest. In an afterburner, a particle beam drives a plasma wave and generates a strong wakefield which has a phase velocity equal to the velocity of the beam. This wakefield can then be used to accelerate part of the drive beam or a trailing beam. Several issues such as the efficient transfer of energy and the stable propagation of both the drive and trailing beams in the plasma are critical to the afterburner concept. We investigate the nonlinear beam-plasma interaction in such scenario using the 3D computer modeling code QuickPIC. We will report on the preliminary simulation results of both 100 GeV and 1 TeV plasma afterburner stages for electrons including the beam-loading of a trailing beam. Analytic analysis of hosing instability in this regime will be presented.
Keywords
Acceleration; Colliding beam accelerators; Incineration; Particle accelerators; Particle beams; Plasma accelerators; Plasma simulation; Plasma stability; Plasma waves; Radio frequency;
fLanguage
English
Publisher
ieee
Conference_Titel
Particle Accelerator Conference, 2005. PAC 2005. Proceedings of the
Print_ISBN
0-7803-8859-3
Type
conf
DOI
10.1109/PAC.2005.1591222
Filename
1591222
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