Can we predict luminosity?

In these proceedings, a luminosity model based on the main components (intrabeam scattering, synchrotron radiation , elastic scattering and luminosity burn-oil) responsible for the LHC luminosity evolution, is compared with data from the 2016 Run of LHC. Based 011 a bunch-by-bunch and fill-by-fill a...

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Detalles Bibliográficos
Autores principales: Antoniou, F, Hostettler, M, Iadarola, G, Papadopoulou, S, Papaphilippou, Y, Pellegrini, D, Trad, G
Lenguaje:eng
Publicado: CERN 2017
Materias:
Accelerators and Storage Rings
Acceso en línea:http://cds.cern.ch/record/2293678
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author Antoniou, F
Hostettler, M
Iadarola, G
Papadopoulou, S
Papaphilippou, Y
Pellegrini, D
Trad, G
author_facet Antoniou, F
Hostettler, M
Iadarola, G
Papadopoulou, S
Papaphilippou, Y
Pellegrini, D
Trad, G
author_sort Antoniou, F
collection CERN
description In these proceedings, a luminosity model based on the main components (intrabeam scattering, synchrotron radiation , elastic scattering and luminosity burn-oil) responsible for the LHC luminosity evolution, is compared with data from the 2016 Run of LHC. Based 011 a bunch-by-bunch and fill-by-fill analysis, the data are compared to the model predictions and possible sources of luminosity degradation are discussed. The impact of the degradation mechanisms on the integrated luminosity is also presented.
id oai-inspirehep.net-1635435
institution Organización Europea para la Investigación Nuclear
language eng
publishDate 2017
publisher CERN
record_format invenio
spelling oai-inspirehep.net-16354352019-09-30T06:29:59Zhttp://cds.cern.ch/record/2293678engAntoniou, FHostettler, MIadarola, GPapadopoulou, SPapaphilippou, YPellegrini, DTrad, GCan we predict luminosity?Accelerators and Storage RingsIn these proceedings, a luminosity model based on the main components (intrabeam scattering, synchrotron radiation , elastic scattering and luminosity burn-oil) responsible for the LHC luminosity evolution, is compared with data from the 2016 Run of LHC. Based 011 a bunch-by-bunch and fill-by-fill analysis, the data are compared to the model predictions and possible sources of luminosity degradation are discussed. The impact of the degradation mechanisms on the integrated luminosity is also presented.CERNoai:inspirehep.net:16354352017
spellingShingle Accelerators and Storage Rings
Antoniou, F
Hostettler, M
Iadarola, G
Papadopoulou, S
Papaphilippou, Y
Pellegrini, D
Trad, G
Can we predict luminosity?
title Can we predict luminosity?
title_full Can we predict luminosity?
title_fullStr Can we predict luminosity?
title_full_unstemmed Can we predict luminosity?
title_short Can we predict luminosity?
title_sort can we predict luminosity?
topic Accelerators and Storage Rings
url http://cds.cern.ch/record/2293678
work_keys_str_mv AT antoniouf canwepredictluminosity
AT hostettlerm canwepredictluminosity
AT iadarolag canwepredictluminosity
AT papadopoulous canwepredictluminosity
AT papaphilippouy canwepredictluminosity
AT pellegrinid canwepredictluminosity
AT tradg canwepredictluminosity

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