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dc.contributor.authorAbratenko, P.
dc.contributor.authorBueno Villar, Antonio 
dc.contributor.authorGarcía Gámez, Diego 
dc.contributor.authorNicolás Arnaldos, Francisco Javier 
dc.contributor.authorPelegrina Gutiérrez, Luis
dc.contributor.authorSáncehz Castillo, Alejandro
dc.contributor.authorSánchez Lucas, Patricia
dc.contributor.authorVázquez Ramos, Alicia
dc.contributor.authorZamorano García, Bruno 
dc.contributor.authorSBND Collaboration
dc.date.accessioned2024-11-18T09:41:03Z
dc.date.available2024-11-18T09:41:03Z
dc.date.issued2024-10-10
dc.identifier.citationAbratenko, P. & Bueno Villar, A. & SNDB Collaboration. et. al. Eur. Phys. J. C (2024) 84:1046. [https://doi.org/10.1140/epjc/s10052-024-13306-3]es_ES
dc.identifier.urihttps://hdl.handle.net/10481/96993
dc.description.abstractSBND is the near detector of the Short-Baseline Neutrino program at Fermilab. Its location near to theBooster Neutrino Beam source and relatively large mass will allow the study of neutrino interactions on argon with unprecedented statistics. This paper describes the expected performance of the SBND photon detection system, using a simulated sample of beam neutrinos and cosmogenic particles. Its design is a dual readout concept combining a system of 120 photomultiplier tubes, used for triggering, with a system of 192 X-ARAPUCA devices, located behind the anode wire planes. Furthermore, covering the cathode plane with highly-reflective panels coated with a wavelength-shifting compound recovers part of the light emitted towards the cathode, where no optical detectors exist.We show how this new design provides a high light yield and a more uniform detection efficiency, an excellent timing resolution and an independent 3D-position reconstruction using only the scintillation light. Finally, the whole reconstruction chain is applied to recover the temporal structure of the beam spill, which is resolved with a resolution on the order of nanoseconds.es_ES
dc.description.sponsorshipThe U.S. Department of Energy, Office of Science, Office of High Energy Physicses_ES
dc.description.sponsorshipThe U.S. National Science Foundationes_ES
dc.description.sponsorshipThe Science and Technology Facilities Council (STFC), part ofUnitedKingdom Research and Innovation, The Royal Society of the United Kingdom, and the UK Research and Innovation (UKRI) Future Leaders Fellowshipes_ES
dc.description.sponsorshipThe Swiss National Science Foundationes_ES
dc.description.sponsorshipThe Spanish Ministerio de Ciencia e Innovación (MICIN/ AEI/ 10.13039/ 501100011033) under grants No PRE2019-090468, PID2019-104676GB-C31 and C32, RYC2022-036471-I, and Comunidad deMadrid (2019-T2/TIC-13649)es_ES
dc.description.sponsorshipThe European Union’s Horizon 2020 research and innovation programme under GA no 101004761 and the Marie Sklodowska-Curie Grant agreements nos. 822185 and 892933es_ES
dc.description.sponsorshipThe São Paulo Research Foundation 1098 (FAPESP), the National Council of Scientific and Technological Development (CNPq) and Ministry of Science, Technology and Innovations-MCTI of Braziles_ES
dc.description.sponsorshipLos Alamos National Laboratory for LDRD fundinges_ES
dc.description.sponsorshipFermilab ismanaged by Fermi Research Alliance, LLC (FRA), acting under Contract no. DE-AC02-07CH11359es_ES
dc.language.isoenges_ES
dc.publisherSpringer Naturees_ES
dc.rightsAtribución 4.0 Internacional*
dc.rights.urihttp://creativecommons.org/licenses/by/4.0/*
dc.titleScintillation light in SBND: simulation, reconstruction, and expected performance of the photon detection systemes_ES
dc.typejournal articlees_ES
dc.relation.projectIDinfo:eu-repo/grantAgreement/EC/H2020/101004761es_ES
dc.relation.projectIDinfo:eu-repo/grantAgreement/EC/MSC/822185es_ES
dc.relation.projectIDinfo:eu-repo/grantAgreement/EC/MSC/892933es_ES
dc.rights.accessRightsopen accesses_ES
dc.identifier.doi10.1140/epjc/s10052-024-13306-3
dc.type.hasVersionVoRes_ES


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