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Design and System Integration of the Superconducting Wiggler Magnets for the Compact Linear Collider Damping Rings
To achieve high luminosity at the collision point of the Compact Linear Collider (CLIC) the normalized horizontal and vertical emittances of the electron and positron beams must be reduced to 500 nm and 4 nm before the beams enter the 1.5TeV linear accelerators. An effective way to accomplish ultra-...
Autores principales: | , , , , , , , , , , , , , |
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Lenguaje: | eng |
Publicado: |
2012
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Materias: | |
Acceso en línea: | https://dx.doi.org/10.1103/PhysRevSTAB.15.042401 http://cds.cern.ch/record/1447817 |
_version_ | 1780924830441275392 |
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author | Schoerling, D Antoniou, F Bernhard, A Bragin, A Karppinen, M Maccaferri, R Mezentsev, N Papaphilippou, Y Peiffer, P Rossmanith, R Rumolo, G Russenschuck, S Vobly, P Zolotarev, K |
author_facet | Schoerling, D Antoniou, F Bernhard, A Bragin, A Karppinen, M Maccaferri, R Mezentsev, N Papaphilippou, Y Peiffer, P Rossmanith, R Rumolo, G Russenschuck, S Vobly, P Zolotarev, K |
author_sort | Schoerling, D |
collection | CERN |
description | To achieve high luminosity at the collision point of the Compact Linear Collider (CLIC) the normalized horizontal and vertical emittances of the electron and positron beams must be reduced to 500 nm and 4 nm before the beams enter the 1.5TeV linear accelerators. An effective way to accomplish ultra-low emittances with only small effects on the electron polarization is using damping rings operating at 2.86 GeV equipped with superconducting wiggler magnets. This paper describes a technical design concept for the CLIC damping wigglers. |
id | cern-1447817 |
institution | Organización Europea para la Investigación Nuclear |
language | eng |
publishDate | 2012 |
record_format | invenio |
spelling | cern-14478172023-07-20T15:07:17Zdoi:10.1103/PhysRevSTAB.15.042401http://cds.cern.ch/record/1447817engSchoerling, DAntoniou, FBernhard, ABragin, AKarppinen, MMaccaferri, RMezentsev, NPapaphilippou, YPeiffer, PRossmanith, RRumolo, GRussenschuck, SVobly, PZolotarev, KDesign and System Integration of the Superconducting Wiggler Magnets for the Compact Linear Collider Damping RingsEngineeringAccelerators and Storage RingsTo achieve high luminosity at the collision point of the Compact Linear Collider (CLIC) the normalized horizontal and vertical emittances of the electron and positron beams must be reduced to 500 nm and 4 nm before the beams enter the 1.5TeV linear accelerators. An effective way to accomplish ultra-low emittances with only small effects on the electron polarization is using damping rings operating at 2.86 GeV equipped with superconducting wiggler magnets. This paper describes a technical design concept for the CLIC damping wigglers.CERN-OPEN-2012-013CERN-ATS-2012-068CLIC-Note-942oai:cds.cern.ch:1452624oai:cds.cern.ch:14478172012-05-01 |
spellingShingle | Engineering Accelerators and Storage Rings Schoerling, D Antoniou, F Bernhard, A Bragin, A Karppinen, M Maccaferri, R Mezentsev, N Papaphilippou, Y Peiffer, P Rossmanith, R Rumolo, G Russenschuck, S Vobly, P Zolotarev, K Design and System Integration of the Superconducting Wiggler Magnets for the Compact Linear Collider Damping Rings |
title | Design and System Integration of the Superconducting Wiggler Magnets for the Compact Linear Collider Damping Rings |
title_full | Design and System Integration of the Superconducting Wiggler Magnets for the Compact Linear Collider Damping Rings |
title_fullStr | Design and System Integration of the Superconducting Wiggler Magnets for the Compact Linear Collider Damping Rings |
title_full_unstemmed | Design and System Integration of the Superconducting Wiggler Magnets for the Compact Linear Collider Damping Rings |
title_short | Design and System Integration of the Superconducting Wiggler Magnets for the Compact Linear Collider Damping Rings |
title_sort | design and system integration of the superconducting wiggler magnets for the compact linear collider damping rings |
topic | Engineering Accelerators and Storage Rings |
url | https://dx.doi.org/10.1103/PhysRevSTAB.15.042401 http://cds.cern.ch/record/1447817 |
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