Estimation of orbit change and emittance growth due to random misalignment in long linacs

In linear accelerators, the transverse beam orbit is induced by tilts of accelerating cavities (deviation of accelerating field direction from designed beam direction) and transverse offset of quadrupole magnets. Estimating induced orbit and emittance growth due to such random errors is important fo...

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Main Author: Kiyoshi Kubo
Format: Article
Language:English
Published: American Physical Society 2011-01-01
Series:Physical Review Special Topics. Accelerators and Beams
Online Access:http://doi.org/10.1103/PhysRevSTAB.14.014401
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author Kiyoshi Kubo
author_facet Kiyoshi Kubo
author_sort Kiyoshi Kubo
collection DOAJ
description In linear accelerators, the transverse beam orbit is induced by tilts of accelerating cavities (deviation of accelerating field direction from designed beam direction) and transverse offset of quadrupole magnets. Estimating induced orbit and emittance growth due to such random errors is important for evaluation of performance of linacs, especially where stable and low emittance beam is required, such as linear colliders. Usually, such estimations are performed using tracking simulations, including the Monte Carlo method, which tends to take a long time. Here, a much faster and simpler method of quantitative estimation of beam orbit and emittance growth is reported. This method is valid for very long linacs with many components, where statistical treatment of errors is justified. It is shown that the results from the method agree well with tracking simulations for the ILC (International Linear Collider) main linac.
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spelling doaj.art-a207065dafe84b58a2828b9bee5203b32022-12-22T00:19:26ZengAmerican Physical SocietyPhysical Review Special Topics. Accelerators and Beams1098-44022011-01-0114101440110.1103/PhysRevSTAB.14.014401Estimation of orbit change and emittance growth due to random misalignment in long linacsKiyoshi KuboIn linear accelerators, the transverse beam orbit is induced by tilts of accelerating cavities (deviation of accelerating field direction from designed beam direction) and transverse offset of quadrupole magnets. Estimating induced orbit and emittance growth due to such random errors is important for evaluation of performance of linacs, especially where stable and low emittance beam is required, such as linear colliders. Usually, such estimations are performed using tracking simulations, including the Monte Carlo method, which tends to take a long time. Here, a much faster and simpler method of quantitative estimation of beam orbit and emittance growth is reported. This method is valid for very long linacs with many components, where statistical treatment of errors is justified. It is shown that the results from the method agree well with tracking simulations for the ILC (International Linear Collider) main linac.http://doi.org/10.1103/PhysRevSTAB.14.014401
spellingShingle Kiyoshi Kubo
Estimation of orbit change and emittance growth due to random misalignment in long linacs
Physical Review Special Topics. Accelerators and Beams
title Estimation of orbit change and emittance growth due to random misalignment in long linacs
title_full Estimation of orbit change and emittance growth due to random misalignment in long linacs
title_fullStr Estimation of orbit change and emittance growth due to random misalignment in long linacs
title_full_unstemmed Estimation of orbit change and emittance growth due to random misalignment in long linacs
title_short Estimation of orbit change and emittance growth due to random misalignment in long linacs
title_sort estimation of orbit change and emittance growth due to random misalignment in long linacs
url http://doi.org/10.1103/PhysRevSTAB.14.014401
work_keys_str_mv AT kiyoshikubo estimationoforbitchangeandemittancegrowthduetorandommisalignmentinlonglinacs