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Observations and predictions at CesrTA, and outlook for ILC
In this paper, we will describe some of the recent experimental measurements [1, 2, 3] performed at CESRTA [4], and the supporting simulations, which probe the interaction of the electron cloud with the stored beam. These experiments have been done over a wide range of beam energies, emittances, bun...
Autores principales: | , , , , , , , , , , , , , , , , , , , , , |
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Lenguaje: | eng |
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CERN
2013
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Materias: | |
Acceso en línea: | https://dx.doi.org/10.5170/CERN-2013-002.31 http://cds.cern.ch/record/1605053 |
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author | Dugan, G. Billing, M. Butler, K. Chu, J. Crittenden, J. Forster, M. Kreinick, D. Meller, R. Palmer, M. Ramirez, G. Rendina, M. Rider, N. Sonnad, K. Williams, H. Campbell, R. Holtzapple, R. Randazzo, M. Flanagan, J. Ohmi, K. Furman, M. Venturini, M. Pivi, M. |
author_facet | Dugan, G. Billing, M. Butler, K. Chu, J. Crittenden, J. Forster, M. Kreinick, D. Meller, R. Palmer, M. Ramirez, G. Rendina, M. Rider, N. Sonnad, K. Williams, H. Campbell, R. Holtzapple, R. Randazzo, M. Flanagan, J. Ohmi, K. Furman, M. Venturini, M. Pivi, M. |
author_sort | Dugan, G. |
collection | CERN |
description | In this paper, we will describe some of the recent experimental measurements [1, 2, 3] performed at CESRTA [4], and the supporting simulations, which probe the interaction of the electron cloud with the stored beam. These experiments have been done over a wide range of beam energies, emittances, bunch currents, and fill patterns, to gather sufficient information to be able to fully characterize the beam-electron-cloud interaction and validate the simulation programs. The range of beam conditions is chosen to be as close as possible to those of the ILC damping ring, so that the validated simulation programs can be used to predict the performance of these rings with regard to electroncloud- related phenomena. Using the new simulation code Synrad3D to simulate the synchrotron radiation environment, a vacuum chamber design has been developed for the ILC damping ring which achieves the required level of photoelectron suppression. To determine the expected electron cloud density in the ring, EC buildup simulations have been done based on the simulated radiation environment and on the expected performance of the ILC damping ring chamber mitigation prescriptions. The expected density has been compared with analytical estimates of the instability threshold, to verify that the ILC damping ring vacuum chamber design is adequate to suppress the electron cloud single-bunch head-tail instability. |
id | cern-1605053 |
institution | Organización Europea para la Investigación Nuclear |
language | eng |
publishDate | 2013 |
publisher | CERN |
record_format | invenio |
spelling | cern-16050532022-08-10T21:10:30Zdoi:10.5170/CERN-2013-002.31http://cds.cern.ch/record/1605053engDugan, G.Billing, M.Butler, K.Chu, J.Crittenden, J.Forster, M.Kreinick, D.Meller, R.Palmer, M.Ramirez, G.Rendina, M.Rider, N.Sonnad, K.Williams, H.Campbell, R.Holtzapple, R.Randazzo, M.Flanagan, J.Ohmi, K.Furman, M.Venturini, M.Pivi, M.Observations and predictions at CesrTA, and outlook for ILCAccelerators and Storage RingsIn this paper, we will describe some of the recent experimental measurements [1, 2, 3] performed at CESRTA [4], and the supporting simulations, which probe the interaction of the electron cloud with the stored beam. These experiments have been done over a wide range of beam energies, emittances, bunch currents, and fill patterns, to gather sufficient information to be able to fully characterize the beam-electron-cloud interaction and validate the simulation programs. The range of beam conditions is chosen to be as close as possible to those of the ILC damping ring, so that the validated simulation programs can be used to predict the performance of these rings with regard to electroncloud- related phenomena. Using the new simulation code Synrad3D to simulate the synchrotron radiation environment, a vacuum chamber design has been developed for the ILC damping ring which achieves the required level of photoelectron suppression. To determine the expected electron cloud density in the ring, EC buildup simulations have been done based on the simulated radiation environment and on the expected performance of the ILC damping ring chamber mitigation prescriptions. The expected density has been compared with analytical estimates of the instability threshold, to verify that the ILC damping ring vacuum chamber design is adequate to suppress the electron cloud single-bunch head-tail instability.In this paper, we will describe some of the recent experimental measurements [1, 2, 3] performed at CESRTA [4], and the supporting simulations, which probe the interaction of the electron cloud with the stored beam. These experiments have been done over a wide range of beam energies, emittances, bunch currents, and fill patterns, to gather sufficient information to be able to fully characterize the beam-electron-cloud interaction and validate the simulation programs. The range of beam conditions is chosen to be as close as possible to those of the ILC damping ring, so that the validated simulation programs can be used to predict the performance of these rings with regard to electroncloud- related phenomena. Using the new simulation code Synrad3D to simulate the synchrotron radiation environment, a vacuum chamber design has been developed for the ILC damping ring which achieves the required level of photoelectron suppression. To determine the expected electron cloud density in the ring, EC buildup simulations have been done based on the simulated radiation environment and on the expected performance of the ILC damping ring chamber mitigation prescriptions. The expected density has been compared with analytical estimates of the instability threshold, to verify that the ILC damping ring vacuum chamber design is adequate to suppress the electron cloud single-bunch head-tail instability.CERNarXiv:1310.0261oai:cds.cern.ch:16050532013-10-01 |
spellingShingle | Accelerators and Storage Rings Dugan, G. Billing, M. Butler, K. Chu, J. Crittenden, J. Forster, M. Kreinick, D. Meller, R. Palmer, M. Ramirez, G. Rendina, M. Rider, N. Sonnad, K. Williams, H. Campbell, R. Holtzapple, R. Randazzo, M. Flanagan, J. Ohmi, K. Furman, M. Venturini, M. Pivi, M. Observations and predictions at CesrTA, and outlook for ILC |
title | Observations and predictions at CesrTA, and outlook for ILC |
title_full | Observations and predictions at CesrTA, and outlook for ILC |
title_fullStr | Observations and predictions at CesrTA, and outlook for ILC |
title_full_unstemmed | Observations and predictions at CesrTA, and outlook for ILC |
title_short | Observations and predictions at CesrTA, and outlook for ILC |
title_sort | observations and predictions at cesrta, and outlook for ilc |
topic | Accelerators and Storage Rings |
url | https://dx.doi.org/10.5170/CERN-2013-002.31 http://cds.cern.ch/record/1605053 |
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