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dc.date.accessioned 2019-12-05T17:40:51Z
dc.date.available 2019-12-05T17:40:51Z
dc.date.issued 2016
dc.identifier.uri http://sedici.unlp.edu.ar/handle/10915/86920
dc.description.abstract This paper discusses various observations on beam-induced and cosmic-ray backgrounds in the ATLAS detector during the LHC 2012 proton-proton run. Building on published results based on 2011 data, the correlations between background and residual pressure of the beam vacuum are revisited. Ghost charge evolution over 2012 and its role for backgrounds are evaluated. New methods to monitor ghost charge with beam-gas rates are presented and observations of LHC abort gap population by ghost charge are discussed in detail. Fake jets from colliding bunches and from ghost charge are analysed with improved methods, showing that ghost charge in individual radio-frequency buckets of the LHC can be resolved. Some results of two short periods of dedicated cosmic-ray background data-taking are shown; in particular cosmic-ray muon induced fake jet rates are compared to Monte Carlo simulations and to the fake jet rates from beam background. A thorough analysis of a particular LHC fill, where abnormally high background was observed, is presented. Correlations between backgrounds and beam intensity losses in special fills with very high β∗ are studied. en
dc.language en es
dc.subject Beam-intensity monitors es
dc.subject Beam-line instrumentation (beam position and profile monitors es
dc.subject Bunch length monitors) es
dc.subject Data analysis es
dc.subject Performance of high energy physics detectors es
dc.title Beam-induced and cosmic-ray backgrounds observed in the ATLAS detector during the LHC 2012 proton-proton running period en
dc.type Articulo es
sedici.identifier.other doi:10.1088/1748-0221/11/05/P05013 es
sedici.identifier.other eid:2-s2.0-85009065117 es
sedici.identifier.issn 1748-0221 es
sedici.creator.person Alconada Verzini, María Josefina es
sedici.creator.person Alonso, Francisco es
sedici.creator.person Arduh, Francisco Anuar es
sedici.creator.person Dova, María Teresa es
sedici.creator.person Monticelli, Fernando Gabriel es
sedici.creator.person Wahlberg, Hernán Pablo es
sedici.creator.corporate The ATLAS Collaboration es
sedici.description.note La lista completa de autores que integran el documento puede consultarse en el archivo es
sedici.subject.materias Física es
sedici.description.fulltext true es
mods.originInfo.place Instituto de Física La Plata es
sedici.subtype Articulo es
sedici.rights.license Creative Commons Attribution 3.0 Unported (CC BY 3.0)
sedici.rights.uri http://creativecommons.org/licenses/by/3.0/
sedici.description.peerReview peer-review es
sedici.relation.journalTitle Journal of Instrumentation es
sedici.relation.journalVolumeAndIssue vol. 11, no. 5 es
sedici.rights.sherpa * Color: green * Pre-print del autor: can * Post-print del autor: can * Versión de editor/PDF:cannot * Condiciones: >>Pre-print on author's personal website, repository, non-commercial scientific social network, arXiv or non-commercial website >>Pre-print can not be updated after submission >>Post-print on author's personal website or Arxiv immediately >>Post-print on institutional website, institutional repository, subject-based repository, bioRxiv, PubMed Central, non-commercial scientific social network or third party eprint servers after 12 months embargo >>Publisher's version/PDF cannot be used >>Published source must be acknowledged with citation >>Must link to publisher version with DOI >>Set statements to accompany different versions (see policy) >>Post-print is not permitted on commercial scientific social networks e.g. ResearchGate, Mendely and Academia.edu >>Articles can not be deposited under an open access license or creative commons license >>Authors may make a closed deposit of post-print on a non-commercial repository within three months of date of acceptance. * Link a Sherpa: http://sherpa.ac.uk/romeo/issn/1748-0221/es/


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Creative Commons Attribution 3.0 Unported (CC BY 3.0) Excepto donde se diga explícitamente, este item se publica bajo la siguiente licencia Creative Commons Attribution 3.0 Unported (CC BY 3.0)