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Synchrotron radiation from proton bunches in the LHC creates photoelectrons at the beam screen wall. These photoelectrons are pulled toward the positively charged proton bunch. When they hit the opposite wall, they generate secondary electrons which can in turn be accelerated by the next bunch. Depending on several assumptions about surface reflectivity, photoelectron and secondary electron yield, this mechanism can lead to the fast build-up of an electron cloud (the animation shows simulation results by O. Brüning for 10 subsequent bunch passages, during which the pictures become red) with potential implications for beam stability and heat load on the beam screen. In view of the tight deadline for the design of the LHC cryogenic system, a crash program has been set up to measure the relevant physical quantities with and without magnetic field. |
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J.R.M. Vaughan, Multipactor, IEEE Trans. Electron Devices
35 1172, 1988
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Reports and Notes on Electron Cloud from 2000 and Earlier
Workshops
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| Synchrotron radiation from the DCI machine, with 3 keV critical energy, after reflection in a circular stainless steel vacuum chamber (O. Gröbner et. al., 29/04/1988). The picture shows light in the visible spectrum collected on a paper screen at the end of the vacuum chamber. The light impinges on the right side and is reflected on the opposite side with an opening angle depending on its wave length and on the surface roughness. Multiple reflections may lead to a nearly uniform illumination of the LHC beam screen. |
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