Update on electron-cloud power deposition for the Large Hadron Collider arc dipoles

We revisit the estimation of the power deposited by the electron cloud (EC) in the arc dipoles of the Large Haydron Collider, by means of simulations. We adopt, as simulation input, a set of electron-related parameters closely resembling those used in recent simulations at CERN [F. Zimmermann, in LT...

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Main Authors: Miguel A. Furman, Vernon H. Chaplin
Format: Article
Language:English
Published: American Physical Society 2006-03-01
Series:Physical Review Special Topics. Accelerators and Beams
Online Access:http://doi.org/10.1103/PhysRevSTAB.9.034403
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spelling doaj-a39f229b4fae4f0bb8234db9871c07dc2020-11-24T22:15:00ZengAmerican Physical SocietyPhysical Review Special Topics. Accelerators and Beams1098-44022006-03-019303440310.1103/PhysRevSTAB.9.034403Update on electron-cloud power deposition for the Large Hadron Collider arc dipolesMiguel A. FurmanVernon H. ChaplinWe revisit the estimation of the power deposited by the electron cloud (EC) in the arc dipoles of the Large Haydron Collider, by means of simulations. We adopt, as simulation input, a set of electron-related parameters closely resembling those used in recent simulations at CERN [F. Zimmermann, in LTC Meeting No. 40, CERN, 2005]. We explore values for the bunch population N_{b} in the range 0.4×10^{11}≤N_{b}≤1.6×10^{11}, peak secondary electron yield δ_{max} in the range 1.0≤δ_{max}≤2.0, and bunch spacing t_{b} either 25 or 75 ns. For t_{b}=25  ns we find that the EC average power deposition per unit length of beam pipe, dP[over ¯]/dz, will exceed the available cooling capacity, which we take to be 1.7   W/m at nominal N_{b} [F. Zimmermann, in LHC MAC Meeting No. 17, 2005], if δ_{max} exceeds ∼1.3, but dP[over ¯]/dz will be comfortably within the cooling capacity if δ_{max}≤1.2. For t_{b}=75  ns dP[over ¯]/dz exceeds the cooling capacity only when δ_{max}>2 and N_{b}>1.5×10^{11} taken in combination. The rediffused component of the secondary electron emission spectrum plays a significant role: if we artificially suppress this component while keeping δ_{max} fixed, dP[over ¯]/dz is roughly cut in half for most values of N_{b} explored here, and in this case we find good agreement with earlier results [F. Zimmermann, in LTC Meeting No. 40, CERN, 2005], as expected. We provide a fairly detailed explanation of the mechanism responsible for such a relatively large effect. We assess the sensitivity of our results to numerical simulation parameters, and to physical parameters such as the photoelectric yield, bunch train length, etc. Owing to the lack of detailed knowledge of the electron emission spectrum, the sensitivity of dP[over ¯]/dz to the rediffused component appears to be the most significant source of uncertainty in our results. Nevertheless, taking our results as a whole, the condition δ_{max}≤1.2 seems to be a conservative requirement for the cooling capacity not to be exceeded.http://doi.org/10.1103/PhysRevSTAB.9.034403
collection DOAJ
language English
format Article
sources DOAJ
author Miguel A. Furman
Vernon H. Chaplin
spellingShingle Miguel A. Furman
Vernon H. Chaplin
Update on electron-cloud power deposition for the Large Hadron Collider arc dipoles
Physical Review Special Topics. Accelerators and Beams
author_facet Miguel A. Furman
Vernon H. Chaplin
author_sort Miguel A. Furman
title Update on electron-cloud power deposition for the Large Hadron Collider arc dipoles
title_short Update on electron-cloud power deposition for the Large Hadron Collider arc dipoles
title_full Update on electron-cloud power deposition for the Large Hadron Collider arc dipoles
title_fullStr Update on electron-cloud power deposition for the Large Hadron Collider arc dipoles
title_full_unstemmed Update on electron-cloud power deposition for the Large Hadron Collider arc dipoles
title_sort update on electron-cloud power deposition for the large hadron collider arc dipoles
publisher American Physical Society
series Physical Review Special Topics. Accelerators and Beams
issn 1098-4402
publishDate 2006-03-01
description We revisit the estimation of the power deposited by the electron cloud (EC) in the arc dipoles of the Large Haydron Collider, by means of simulations. We adopt, as simulation input, a set of electron-related parameters closely resembling those used in recent simulations at CERN [F. Zimmermann, in LTC Meeting No. 40, CERN, 2005]. We explore values for the bunch population N_{b} in the range 0.4×10^{11}≤N_{b}≤1.6×10^{11}, peak secondary electron yield δ_{max} in the range 1.0≤δ_{max}≤2.0, and bunch spacing t_{b} either 25 or 75 ns. For t_{b}=25  ns we find that the EC average power deposition per unit length of beam pipe, dP[over ¯]/dz, will exceed the available cooling capacity, which we take to be 1.7   W/m at nominal N_{b} [F. Zimmermann, in LHC MAC Meeting No. 17, 2005], if δ_{max} exceeds ∼1.3, but dP[over ¯]/dz will be comfortably within the cooling capacity if δ_{max}≤1.2. For t_{b}=75  ns dP[over ¯]/dz exceeds the cooling capacity only when δ_{max}>2 and N_{b}>1.5×10^{11} taken in combination. The rediffused component of the secondary electron emission spectrum plays a significant role: if we artificially suppress this component while keeping δ_{max} fixed, dP[over ¯]/dz is roughly cut in half for most values of N_{b} explored here, and in this case we find good agreement with earlier results [F. Zimmermann, in LTC Meeting No. 40, CERN, 2005], as expected. We provide a fairly detailed explanation of the mechanism responsible for such a relatively large effect. We assess the sensitivity of our results to numerical simulation parameters, and to physical parameters such as the photoelectric yield, bunch train length, etc. Owing to the lack of detailed knowledge of the electron emission spectrum, the sensitivity of dP[over ¯]/dz to the rediffused component appears to be the most significant source of uncertainty in our results. Nevertheless, taking our results as a whole, the condition δ_{max}≤1.2 seems to be a conservative requirement for the cooling capacity not to be exceeded.
url http://doi.org/10.1103/PhysRevSTAB.9.034403
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