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Fowkes, W.R.; Allen, M.A.; Callin, R.S.; Caryotakis, G.; Eppley, K.R.; Fant, K.S.; Farkas, Z.D.; Feinstein, J.; Ko, K.; Koontz, R.F.; Kroll, N.; Lavine, T.L.; Lee, T.G.; Miller, R.H.; Pearson, C.; Spalek, G.; Vlieks, A.E.; Wilson, P.B.
Stanford Linear Accelerator Center, Menlo Park, CA (USA)1990
Stanford Linear Accelerator Center, Menlo Park, CA (USA)1990
AbstractAbstract
[en] The next linear collider will require 200 MW of rf power per meter of linac structure at relatively high frequency to produce an accelerating gradient of about 100 MV/m. The higher frequencies result in a higher breakdown threshold in the accelerating structure hence permit higher accelerating gradients per meter of linac. The lower frequencies have the advantage that high peak power rf sources can be realized. 11.42 GHz appears to be a good compromise and the effort at the Stanford Linear Accelerator Center (SLAC) is being concentrated on rf sources operating at this frequency. The filling time of the accelerating structure for each rf feed is expected to be about 80 ns. Under serious consideration at SLAC is a conventional klystron followed by a multistage rf pulse compression system, and the Crossed-Field Amplifier. These are discussed in this paper
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Jun 1990; 8 p; 8. international conference on high-power particle beams; Novosibirsk (USSR); 2-5 Jul 1990; CONF-9007111--13; CONTRACT AC03-76SF00515; NTIS, PC A02/MF A01 as DE90014804; OSTI; INIS; US Govt. Printing Office Dep
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