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Energy deposition studies for the High-Luminosity Large Hadron Collider inner triplet magnets

A detailed model of the High Luminosity LHC inner triplet region with new large-aperture Nb$_{3}$Sn magnets, field maps, corrector packages, and segmented tungsten inner absorbers was built and implemented into the FLUKA and MARS15 codes. In the optimized configuration, the peak power density averag...

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Detalles Bibliográficos
Autores principales: Mokhov, N.V., Rakhno, I.L., Tropin, I.S., Cerutti, F., Esposito, L.S., Lechner, A.
Lenguaje:eng
Publicado: 2015
Materias:
Acceso en línea:https://dx.doi.org/10.1103/PhysRevSTAB.18.051001
http://cds.cern.ch/record/2006710
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author Mokhov, N.V.
Rakhno, I.L.
Tropin, I.S.
Cerutti, F.
Esposito, L.S.
Lechner, A.
author_facet Mokhov, N.V.
Rakhno, I.L.
Tropin, I.S.
Cerutti, F.
Esposito, L.S.
Lechner, A.
author_sort Mokhov, N.V.
collection CERN
description A detailed model of the High Luminosity LHC inner triplet region with new large-aperture Nb$_{3}$Sn magnets, field maps, corrector packages, and segmented tungsten inner absorbers was built and implemented into the FLUKA and MARS15 codes. In the optimized configuration, the peak power density averaged over the magnet inner cable width is safely below the quench limit. For the integrated luminosity of 3000 fb-1, the peak dose in the innermost magnet insulator ranges from 20 to 35 MGy. Dynamic heat loads to the triplet magnet cold mass are calculated to evaluate the cryogenic capability. In general, FLUKA and MARS results are in a very good agreement.
id cern-2006710
institution Organización Europea para la Investigación Nuclear
language eng
publishDate 2015
record_format invenio
spelling cern-20067102023-03-14T16:30:21Zdoi:10.1103/PhysRevSTAB.18.051001http://cds.cern.ch/record/2006710engMokhov, N.V.Rakhno, I.L.Tropin, I.S.Cerutti, F.Esposito, L.S.Lechner, A.Energy deposition studies for the High-Luminosity Large Hadron Collider inner triplet magnetsAccelerators and Storage RingsA detailed model of the High Luminosity LHC inner triplet region with new large-aperture Nb$_{3}$Sn magnets, field maps, corrector packages, and segmented tungsten inner absorbers was built and implemented into the FLUKA and MARS15 codes. In the optimized configuration, the peak power density averaged over the magnet inner cable width is safely below the quench limit. For the integrated luminosity of 3000 fb-1, the peak dose in the innermost magnet insulator ranges from 20 to 35 MGy. Dynamic heat loads to the triplet magnet cold mass are calculated to evaluate the cryogenic capability. In general, FLUKA and MARS results are in a very good agreement.A detailed model of the high-luminosity LHC inner triplet region with new large-aperture Nb3Sn magnets, field maps, corrector packages, and segmented tungsten inner absorbers was built and implemented into the fluka and mars15 codes. Detailed simulations have been performed coherently with the codes on the impact of particle debris from the 14-TeV center-of-mass pp-collisions on the short- and long-term stability of the inner triplet magnets. After optimizing the absorber configuration, the peak power density averaged over the magnet inner cable width is found to be safely below the quench limit at the luminosity of 5×1034  cm−2 s−1. For the anticipated lifetime integrated luminosity of 3000  fb−1, the peak dose calculated for the innermost magnet insulator ranges from 20 to 35 MGy, a figure close to the commonly accepted limit. Dynamic heat loads to the triplet magnet cold mass are calculated to evaluate the cryogenic capability. fluka and mars results on energy deposition are in very good agreement.A detailed model of the High Luminosity LHC inner triplet region with new large-aperture Nb3Sn magnets, field maps, corrector packages, and segmented tungsten inner absorbers was built and implemented into the FLUKA and MARS15 codes. In the optimized configuration, the peak power density averaged over the magnet inner cable width is safely below the quench limit. For the integrated luminosity of 3000 fb-1, the peak dose in the innermost magnet insulator ranges from 20 to 35 MGy. Dynamic heat loads to the triplet magnet cold mass are calculated to evaluate the cryogenic capability. In general, FLUKA and MARS results are in a very good agreement.arXiv:1504.00594FERMILAB-PUB-15-095-APCFERMILAB-PUB-15-095-APCoai:cds.cern.ch:20067102015-04-02
spellingShingle Accelerators and Storage Rings
Mokhov, N.V.
Rakhno, I.L.
Tropin, I.S.
Cerutti, F.
Esposito, L.S.
Lechner, A.
Energy deposition studies for the High-Luminosity Large Hadron Collider inner triplet magnets
title Energy deposition studies for the High-Luminosity Large Hadron Collider inner triplet magnets
title_full Energy deposition studies for the High-Luminosity Large Hadron Collider inner triplet magnets
title_fullStr Energy deposition studies for the High-Luminosity Large Hadron Collider inner triplet magnets
title_full_unstemmed Energy deposition studies for the High-Luminosity Large Hadron Collider inner triplet magnets
title_short Energy deposition studies for the High-Luminosity Large Hadron Collider inner triplet magnets
title_sort energy deposition studies for the high-luminosity large hadron collider inner triplet magnets
topic Accelerators and Storage Rings
url https://dx.doi.org/10.1103/PhysRevSTAB.18.051001
http://cds.cern.ch/record/2006710
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AT rakhnoil energydepositionstudiesforthehighluminositylargehadroncolliderinnertripletmagnets
AT tropinis energydepositionstudiesforthehighluminositylargehadroncolliderinnertripletmagnets
AT ceruttif energydepositionstudiesforthehighluminositylargehadroncolliderinnertripletmagnets
AT espositols energydepositionstudiesforthehighluminositylargehadroncolliderinnertripletmagnets
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