Paper |
Title |
Page |
MOPTS098 |
A Primary Electron Beam Facility at CERN |
1098 |
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- Y. Papaphilippou, R. Corsini, Y. Dutheil, L.R. Evans, B. Goddard, A. Grudiev, A. Latina, S. Stapnes
CERN, Geneva, Switzerland
- T.P.Å. Åkesson
Lund University, Department of Physics, Lund, Sweden
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This paper describes the concept of a primary electron beam facility at CERN, to be used for dark gauge force and light dark matter searches. The electron beam is produced in three stages: A Linac accelerates electrons from a photo-cathode up to 3.5 GeV. This beam is injected into the Super Proton Synchrotron, SPS, and accelerated up to a maximum energy of 16 GeV. Finally, the accelerated beam is slowly extracted to an experiment, possibly followed by a fast dump of the remaining electrons to another beamline. The beam parameters are optimized using the requirements of the Light Dark Matter eXperiment, LDMX, as benchmark.
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DOI • |
reference for this paper
※ https://doi.org/10.18429/JACoW-IPAC2019-MOPTS098
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About • |
paper received ※ 15 May 2019 paper accepted ※ 20 May 2019 issue date ※ 21 June 2019 |
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WEYPLS1 |
Building the Impedance Model of a Real Machine |
2249 |
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- B. Salvant, D. Amorim, S.A. Antipov, S. Arsenyev, M.S. Beck, N. Biancacci, O.S. Brüning, J.V. Campelo, E. Carideo, F. Caspers, A. Farricker, A. Grudiev, T. Kaltenbacher, E. Koukovini-Platia, P. Kramer, A. Lasheen, M. Migliorati, N. Mounet, E. Métral, N. Nasr Esfahani, S. Persichelli, B.K. Popovic, T.L. Rijoff, G. Rumolo, E.N. Shaposhnikova, V.G. Vaccaro, C. Vollinger, N. Wang, C. Zannini, B. Zotter
CERN, Meyrin, Switzerland
- D. Amorim
Grenoble-INP Phelma, Grenoble, France
- T. Dalascu
EPFL, Lausanne, Switzerland
- M. Migliorati
Sapienza University of Rome, Rome, Italy
- R. Nagaoka
SOLEIL, Gif-sur-Yvette, France
- V.V. Smaluk
BNL, Upton, Long Island, New York, USA
- B. Spataro
INFN/LNF, Frascati, Italy
- N. Wang
IHEP, Beijing, People’s Republic of China
- S.M. White
ESRF, Grenoble, France
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A reliable impedance model of a particle accelerator can be built by combining the beam coupling impedances of all the components. This is a necessary step to be able to evaluate the machine performance limitations, identify the main contributors in case an impedance reduction is required, and study the interaction with other mechanisms such as optics nonlinearities, transverse damper, noise, space charge, electron cloud, beam-beam (in a collider). The main phases to create a realistic impedance model, and verify it experimentally, will be reviewed, highlighting the main challenges. Some examples will be presented revealing the levels of precision of machine impedance models that have been achieved.
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Slides WEYPLS1 [5.648 MB]
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DOI • |
reference for this paper
※ https://doi.org/10.18429/JACoW-IPAC2019-WEYPLS1
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About • |
paper received ※ 10 May 2019 paper accepted ※ 23 May 2019 issue date ※ 21 June 2019 |
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WEPRB034 |
Study on the Design of the X-band Waveguide-damped Structure |
2886 |
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- X.X. Huang, W. Fang, Z.T. Zhao
SSRF, Shanghai, People’s Republic of China
- A. Grudiev
CERN, Meyrin, Switzerland
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The design of waveguide-damped structure is optimized to reduce the magnitudes of surface electromagnetic fields and strongly suppress long-range transverse wakefields of the 380 GeV Compact Linear Collider facility currently under study. The optimization is mainly discussed with the elliptical shape of the iris, the wall shape of the damping waveguides, the position of the high-order-mode damping loads and the widths of the waveguide openings of the entire sequence of damping waveguides.
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DOI • |
reference for this paper
※ https://doi.org/10.18429/JACoW-IPAC2019-WEPRB034
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About • |
paper received ※ 13 May 2019 paper accepted ※ 22 May 2019 issue date ※ 21 June 2019 |
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WEPRB043 |
Wakefield Suppression in the Main LINAC of the Klystron-Based First Stage of CLIC at 380 GeV |
2899 |
SUSPFO064 |
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- J.Y. Liu, H.B. Chen, J. Shi, H. Zha
TUB, Beijing, People’s Republic of China
- A. Grudiev
CERN, Meyrin, Switzerland
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An alternative klystron-based scenario for the first stage of Compact Linear Collider (CLIC) at 380 GeV centre-of-mass energy was proposed. To preserve the beam stability and luminosity of CLIC, the beam-induced transverse long-range wakefield in main linac must be suppressed to an acceptable value. The design of klystron-based accelerating structure is based on waveguide damping structure (WDS). The high-order modes (HOMs) propagating into four waveguides are absorbed by HOM damping loads. In this paper, the wakefield suppression in CLIC-K based on GdfidL code simulations are presented.
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DOI • |
reference for this paper
※ https://doi.org/10.18429/JACoW-IPAC2019-WEPRB043
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About • |
paper received ※ 14 May 2019 paper accepted ※ 22 May 2019 issue date ※ 21 June 2019 |
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WEPRB064 |
High Power Conditioning of X-Band Variable Power Splitter and Phase Shifter |
2964 |
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- V. del Pozo Romano, H. Bursali, N. Catalán Lasheras, A. Grudiev, S. Pitman, I. Syratchev
CERN, Geneva, Switzerland
- C. Serpico
Elettra-Sincrotrone Trieste S.C.p.A., Basovizza, Italy
- M. Volpi
The University of Melbourne, Melbourne, Victoria, Australia
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The three X-band test facilities currently at CERN aim at qualifying CLIC structures prototypes but are also exten- sively used to qualify X-band components operation at high power. In order to upgrade one of the facilities from a single test line to a double test line facility, a high power variable splitter and variable phase shifter have been designed and manufactured at CERN. They have been power tested, first in a dedicated test and also in their final configuration, to en- sure stable power operation before installing them together with an accelerating structure. In this paper, we broadly describe the RF and mechanical design, manufacturing and low power measurements agreement with simulations. We report the high power qualification of both components and their suitability to be used in existing and planned X-band facilities.
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DOI • |
reference for this paper
※ https://doi.org/10.18429/JACoW-IPAC2019-WEPRB064
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About • |
paper received ※ 10 May 2019 paper accepted ※ 22 May 2019 issue date ※ 21 June 2019 |
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