Simulation study of electron cloud induced instabilities and emittance growth for the CERN Large Hadron Collider proton beam

The electron cloud may cause transverse single-bunch instabilities of proton beams such as those in the Large Hadron Collider (LHC) and the CERN Super Proton Synchrotron (SPS). We simulate these instabilities and the consequent emittance growth with the code HEADTAIL, which models the turn-by-turn i...

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Main Authors: E. Benedetto, D. Schulte, F. Zimmermann, G. Rumolo
Format: Article
Language:English
Published: American Physical Society 2005-12-01
Series:Physical Review Special Topics. Accelerators and Beams
Online Access:http://doi.org/10.1103/PhysRevSTAB.8.124402
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spelling doaj-7462e0a2a66b427d87b033048aae506d2020-11-24T22:03:11ZengAmerican Physical SocietyPhysical Review Special Topics. Accelerators and Beams1098-44022005-12-0181212440210.1103/PhysRevSTAB.8.124402Simulation study of electron cloud induced instabilities and emittance growth for the CERN Large Hadron Collider proton beamE. BenedettoD. SchulteF. ZimmermannG. RumoloThe electron cloud may cause transverse single-bunch instabilities of proton beams such as those in the Large Hadron Collider (LHC) and the CERN Super Proton Synchrotron (SPS). We simulate these instabilities and the consequent emittance growth with the code HEADTAIL, which models the turn-by-turn interaction between the cloud and the beam. Recently some new features were added to the code, in particular, electric conducting boundary conditions at the chamber wall, transverse feedback, and variable beta functions. The sensitivity to several numerical parameters has been studied by varying the number of interaction points between the bunch and the cloud, the phase advance between them, and the number of macroparticles used to represent the protons and the electrons. We present simulation results for both LHC at injection and SPS with LHC-type beam, for different electron-cloud density levels, chromaticities, and bunch intensities. Two regimes with qualitatively different emittance growth are observed: above the threshold of the transverse mode-coupling (TMC) type of instability there is a rapid blowup of the beam, while below this threshold a slow, long-term, emittance growth remains. The rise time of the TMC instability caused by the electron cloud is compared with results obtained using an equivalent broadband resonator impedance model, demonstrating reasonable agreement.http://doi.org/10.1103/PhysRevSTAB.8.124402
collection DOAJ
language English
format Article
sources DOAJ
author E. Benedetto
D. Schulte
F. Zimmermann
G. Rumolo
spellingShingle E. Benedetto
D. Schulte
F. Zimmermann
G. Rumolo
Simulation study of electron cloud induced instabilities and emittance growth for the CERN Large Hadron Collider proton beam
Physical Review Special Topics. Accelerators and Beams
author_facet E. Benedetto
D. Schulte
F. Zimmermann
G. Rumolo
author_sort E. Benedetto
title Simulation study of electron cloud induced instabilities and emittance growth for the CERN Large Hadron Collider proton beam
title_short Simulation study of electron cloud induced instabilities and emittance growth for the CERN Large Hadron Collider proton beam
title_full Simulation study of electron cloud induced instabilities and emittance growth for the CERN Large Hadron Collider proton beam
title_fullStr Simulation study of electron cloud induced instabilities and emittance growth for the CERN Large Hadron Collider proton beam
title_full_unstemmed Simulation study of electron cloud induced instabilities and emittance growth for the CERN Large Hadron Collider proton beam
title_sort simulation study of electron cloud induced instabilities and emittance growth for the cern large hadron collider proton beam
publisher American Physical Society
series Physical Review Special Topics. Accelerators and Beams
issn 1098-4402
publishDate 2005-12-01
description The electron cloud may cause transverse single-bunch instabilities of proton beams such as those in the Large Hadron Collider (LHC) and the CERN Super Proton Synchrotron (SPS). We simulate these instabilities and the consequent emittance growth with the code HEADTAIL, which models the turn-by-turn interaction between the cloud and the beam. Recently some new features were added to the code, in particular, electric conducting boundary conditions at the chamber wall, transverse feedback, and variable beta functions. The sensitivity to several numerical parameters has been studied by varying the number of interaction points between the bunch and the cloud, the phase advance between them, and the number of macroparticles used to represent the protons and the electrons. We present simulation results for both LHC at injection and SPS with LHC-type beam, for different electron-cloud density levels, chromaticities, and bunch intensities. Two regimes with qualitatively different emittance growth are observed: above the threshold of the transverse mode-coupling (TMC) type of instability there is a rapid blowup of the beam, while below this threshold a slow, long-term, emittance growth remains. The rise time of the TMC instability caused by the electron cloud is compared with results obtained using an equivalent broadband resonator impedance model, demonstrating reasonable agreement.
url http://doi.org/10.1103/PhysRevSTAB.8.124402
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