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Dynamics of the interaction of dust particles with the LHC beam

Micrometer-sized dust particles present in the Large Hadron Collider (LHC) beam pipe are believed to have caused many thousands of sporadic beam loss events around the LHC. These so-called unidentified falling objects (UFOs) have been under continuous study since the start of high intensity beam ope...

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Autores principales: Lindstrom, B, Bélanger, P, Gorzawski, A, Kral, J, Lechner, A, Salvachua, B, Schmidt, R, Siemko, A, Vaananen, M, Valuch, D, Wiesner, C, Wollmann, D, Zamantzas, C
Lenguaje:eng
Publicado: 2020
Materias:
Acceso en línea:https://dx.doi.org/10.1103/PhysRevAccelBeams.23.124501
http://cds.cern.ch/record/2750010
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author Lindstrom, B
Bélanger, P
Gorzawski, A
Kral, J
Lechner, A
Salvachua, B
Schmidt, R
Siemko, A
Vaananen, M
Valuch, D
Wiesner, C
Wollmann, D
Zamantzas, C
author_facet Lindstrom, B
Bélanger, P
Gorzawski, A
Kral, J
Lechner, A
Salvachua, B
Schmidt, R
Siemko, A
Vaananen, M
Valuch, D
Wiesner, C
Wollmann, D
Zamantzas, C
author_sort Lindstrom, B
collection CERN
description Micrometer-sized dust particles present in the Large Hadron Collider (LHC) beam pipe are believed to have caused many thousands of sporadic beam loss events around the LHC. These so-called unidentified falling objects (UFOs) have been under continuous study since the start of high intensity beam operation in the LHC due to their impact on the LHC availability: 139 beam dumps and 12 magnet quenches during Run II (2015–2018) alone. To mitigate the impact of UFOs on future accelerators such as the High Luminosity LHC and the Future Circular Collider, it is fundamental to foster a better understanding of these beam loss events. In this paper, key observations made since the start of LHC operation are summarized and the prevailing UFO hypothesis is confronted by a compilation of observations acquired during Run II. In particular, it is shown that UFOs must carry an initial negative charge before entering the proton beam, or that they are by some other means accelerated toward the beam not only by gravity. A simulation model for the dynamics of the dust particles and their interaction with the beam was developed over the years. This model is improved and validated by measurements. It is however also shown that a subset of observed beam losses, which contain a positive time profile skewness, cannot be explained by it.
id oai-inspirehep.net-1839777
institution Organización Europea para la Investigación Nuclear
language eng
publishDate 2020
record_format invenio
spelling oai-inspirehep.net-18397772021-01-22T22:04:26Zdoi:10.1103/PhysRevAccelBeams.23.124501http://cds.cern.ch/record/2750010engLindstrom, BBélanger, PGorzawski, AKral, JLechner, ASalvachua, BSchmidt, RSiemko, AVaananen, MValuch, DWiesner, CWollmann, DZamantzas, CDynamics of the interaction of dust particles with the LHC beamAccelerators and Storage RingsMicrometer-sized dust particles present in the Large Hadron Collider (LHC) beam pipe are believed to have caused many thousands of sporadic beam loss events around the LHC. These so-called unidentified falling objects (UFOs) have been under continuous study since the start of high intensity beam operation in the LHC due to their impact on the LHC availability: 139 beam dumps and 12 magnet quenches during Run II (2015–2018) alone. To mitigate the impact of UFOs on future accelerators such as the High Luminosity LHC and the Future Circular Collider, it is fundamental to foster a better understanding of these beam loss events. In this paper, key observations made since the start of LHC operation are summarized and the prevailing UFO hypothesis is confronted by a compilation of observations acquired during Run II. In particular, it is shown that UFOs must carry an initial negative charge before entering the proton beam, or that they are by some other means accelerated toward the beam not only by gravity. A simulation model for the dynamics of the dust particles and their interaction with the beam was developed over the years. This model is improved and validated by measurements. It is however also shown that a subset of observed beam losses, which contain a positive time profile skewness, cannot be explained by it.oai:inspirehep.net:18397772020
spellingShingle Accelerators and Storage Rings
Lindstrom, B
Bélanger, P
Gorzawski, A
Kral, J
Lechner, A
Salvachua, B
Schmidt, R
Siemko, A
Vaananen, M
Valuch, D
Wiesner, C
Wollmann, D
Zamantzas, C
Dynamics of the interaction of dust particles with the LHC beam
title Dynamics of the interaction of dust particles with the LHC beam
title_full Dynamics of the interaction of dust particles with the LHC beam
title_fullStr Dynamics of the interaction of dust particles with the LHC beam
title_full_unstemmed Dynamics of the interaction of dust particles with the LHC beam
title_short Dynamics of the interaction of dust particles with the LHC beam
title_sort dynamics of the interaction of dust particles with the lhc beam
topic Accelerators and Storage Rings
url https://dx.doi.org/10.1103/PhysRevAccelBeams.23.124501
http://cds.cern.ch/record/2750010
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