Search for photons above 1018  eV by simultaneously measuring the atmospheric depth and the muon content of air showers at the Pierre Auger Observatory

dc.citation.titlePhysical Review D
dc.citation.volume110
dc.creatorBinet, V.
dc.creatorMicheletti, M. I.
dc.creatorThe Pierre Auger collaboration
dc.date.accessioned2025-03-20T12:33:41Z
dc.date.available2025-03-20T12:33:41Z
dc.date.issued2024-09-25
dc.description.abstractThe Pierre Auger Observatory is the most sensitive instrument to detect photons with energies above 1⁢017  eV. It measures extensive air showers generated by ultrahigh energy cosmic rays using a hybrid technique that exploits the combination of a fluorescence detector with a ground array of particle detectors. The signatures of a photon-induced air shower are a larger atmospheric depth of the shower maximum (𝑋max) and a steeper lateral distribution function, along with a lower number of muons with respect to the bulk of hadron-induced cascades. In this work, a new analysis technique in the energy interval between 1 and 30 EeV (1  EeV=1⁢018  eV) has been developed by combining the fluorescence detector-based measurement of 𝑋max with the specific features of the surface detector signal through a parameter related to the air shower muon content, derived from the universality of the air shower development. No evidence of a statistically significant signal due to photon primaries was found using data collected in about 12 years of operation. Thus, upper bounds to the integral photon flux have been set using a detailed calculation of the detector exposure, in combination with a data-driven background estimation. The derived 95% confidence level upper limits are 0.0403, 0.01113, 0.0035, 0.0023, and 0.0021  km−2 sr−1 yr−1 above 1, 2, 3, 5, and 10 EeV, respectively, leading to the most stringent upper limits on the photon flux in the EeV range. Compared with past results, the upper limits were improved by about 40% for the lowest energy threshold and by a factor 3 above 3 EeV, where no candidates were found and the expected background is negligible. The presented limits can be used to probe the assumptions on chemical composition of ultrahigh energy cosmic rays and allow for the constraint of the mass and lifetime phase space of super-heavy dark matter particles.
dc.description.filFil: Binet, V. Universidad Nacional de Rosario. Facultad de Ciencias Bioquímicas y Farmacéuticas. Instituto de Física de Rosario (IFIR-CONICET); Argentina.
dc.description.filFil: Micheletti, M. I. Universidad Nacional de Rosario. Facultad de Ciencias Bioquímicas y Farmacéuticas. Instituto de Física de Rosario (IFIR-CONICET); Argentina.
dc.description.sponsorshipArgentina. Comisión Nacional de Energía Atómica (CNEA)
dc.description.sponsorshipAgencia Nacional de Promoción de la Investigación, el Desarrollo Tecnológico y la Innovación (Agencia I+D+i)
dc.description.sponsorshipConsejo Nacional de Investigaciones Científicas y Técnicas (CONICET)
dc.description.sponsorshipGobierno de la Provincia de Mendoza
dc.description.sponsorshipMunicipalidad de Malargüe
dc.description.sponsorshipNDM Holdings and Valle Las Leñas
dc.description.sponsorshipAustralian Research Council
dc.description.sponsorshipFonds de la Recherche Scientifique (FNRS)
dc.description.sponsorshipResearch Foundation Flanders (FWO)
dc.description.sponsorshipMarie Curie Action of the European Union: Grant No. 101107047
dc.description.sponsorshipConselho Nacional de Desenvolvimento Científico e Tecnológico (CNPq)
dc.description.sponsorshipFinanciadora de Estudos e Projetos (FINEP)
dc.description.sponsorshipFundação de Amparo à Pesquisa do Estado de Rio de Janeiro (FAPERJ)
dc.description.sponsorshipSão Paulo Research Foundation (FAPESP): Grants No. 2019/10151-2, No. 2010/07359-6, and No. 1999/05404-3
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dc.description.sponsorshipCzech Academy of Sciences: LQ100102401
dc.description.sponsorshipCentre National de la Recherche Scientifique (CNRS)
dc.description.sponsorshipCentre National de la Recherche Scientifique (CNRS). Centre de Calcul de l’IN2P3 (CC-IN2P3)
dc.description.sponsorshipCentre National de la Recherche Scientifique (CNRS). Département Physique Nucléaire et Corpusculaire (PNC-IN2P3)
dc.description.sponsorshipCentre National de la Recherche Scientifique (CNRS). Institut National des Sciences de l'Univers (INSU). Département Sciences de l'Univers (SDU)
dc.description.sponsorshipConseil régional d'Île-de-France
dc.description.sponsorshipInstitut Lagrange de Paris (ILP): Grant No. LABEX ANR-10-LABX-63
dc.description.sponsorshipInvestissements d’Avenir Programme: Grant No. ANR-11-IDEX-0004-02
dc.description.sponsorshipBundesministerium für Bildung und Forschung (BMBF)
dc.description.sponsorshipDeutsche Forschungsgemeinschaft (DFG)
dc.description.sponsorshipFinanzministerium Baden-Württemberg; Helmholtz Alliance for Astroparticle Physics (HAP)
dc.description.sponsorshipHelmholtz-Gemeinschaft Deutscher Forschungszentren (HGF)
dc.description.sponsorshipMinisterium für Kultur und Wissenschaft des Landes Nordrhein-Westfalen (MKW NRW)
dc.description.sponsorshipMinisterium für Wissenschaft, Forschung und Kunst des Landes Baden-Württemberg
dc.description.sponsorshipIstituto Nazionale di Fisica Nucleare (INFN)
dc.description.sponsorshipIstituto Nazionale di Astrofisica (INAF)
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dc.description.sponsorshipItalian Center for SuperComputing (ICSC). Centro Nazionale di Ricerca in High Performance Computing, Big Data and Quantum Computing
dc.description.sponsorshipEuropean Union NextGenerationEU: reference code CN_00000013
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dc.description.sponsorshipUniversidad Nacional Autónoma de México (UNAM)
dc.description.sponsorshipUniversidad Nacional Autónoma de México (UNAM). Dirección General de Asuntos del Personal Académico (DGAPA). Programa de Apoyo a Proyectos de Investigación e Innovación Tecnológica (PAPIIT)
dc.description.sponsorshipNetherlands. Ministry of Education, Culture and Science
dc.description.sponsorshipNetherlands Organization for Scientific Research (NWO)
dc.description.sponsorshipDutch national e-infrastructure with the support of SURF Cooperative
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dc.description.sponsorshipPortugal. Ministério da Educação, Ciência e Inovação. Fundação para a Ciência e a Tecnologia (FCT). Programa Operacional Factores de Competitividade (COMPETE)
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dc.description.sponsorshipEuropean Commission. Marie Skłodowska-Curie Actions (MSCA)
dc.description.sponsorshipEuropean Commission. European Regional Development Fund (ERDF)
dc.description.sponsorshipU.S. Department of Energy (DOE): Contracts No. DE-AC02-07CH11359, No. DE-FR02-04ER41300, No. DE-FG02-99ER41107, No. DE-SC0011689
dc.description.sponsorshipU.S. National Science Foundation (NSF): Grant No. 0450696
dc.description.sponsorshipThe Grainger Foundation
dc.description.sponsorshipEuropean Commission. International Research Staff Exchange Scheme (IRSES-MSCA)
dc.description.sponsorshipEuropean Commission. European Particle physics Latin America NETwork (EPLANET-MSCA)
dc.description.sponsorshipOrganización de las Naciones Unidas para la Educación, la Ciencia y la Cultura (UNESCO)
dc.description.versionpeerreviewed
dc.format.extent1-21
dc.identifier.citationAbdul Halim, A., Abreu, P., Aglietta, M., Allekotte, I., Almeida Cheminant, K., Almela, A., Aloisio, R., Alvarez-Muñiz, J., Ammerman Yebra, J., Anastasi, G. A., Anchordoqui, L., Andrada, B., Andrade Dourado, L., Andringa, S., Apollonio, L., Aramo, C., Araújo Ferreira, P. R., Arnone, E., Arteaga Velázquez, J. C.,... Zavrtanik, M. (2024). Search for photons above 1018  eV by simultaneously measuring the atmospheric depth and the muon content of air showers at the Pierre Auger Observatory. Physical Review D, 110(6). https://doi.org/10.1103/PhysRevD.110.062005
dc.identifier.e-issn2470-0029
dc.identifier.issn2470-0010
dc.identifier.urihttps://hdl.handle.net/2133/29087
dc.language.isoen
dc.publisherAmerican Physical Society
dc.relation.publisherversionhttps://doi.org/10.1103/PhysRevD.110.062005
dc.relation.publisherversionhttps://journals.aps.org/prd/abstract/10.1103/PhysRevD.110.062005
dc.rightsopenAccess
dc.rights.holderBinet, V.
dc.rights.holderMicheletti, M. I.
dc.rights.holderThe Pierre Auger collaboration
dc.rights.holderUniversidad Nacional de Rosario. Facultad de Ciencias Bioquímicas y Farmacéuticas
dc.rights.textAttribution 4.0 International
dc.rights.urihttp://creativecommons.org/licenses/by/4.0/
dc.subjectCosmic ray composition & spectra
dc.subjectCosmic ray propagation
dc.subjectCosmic ray sources
dc.subjectCosmic rays & astroparticles
dc.subjectParticle dark matter
dc.subjectCosmic ray & astroparticle detectors
dc.titleSearch for photons above 1018  eV by simultaneously measuring the atmospheric depth and the muon content of air showers at the Pierre Auger Observatory
dc.typearticulo
dc.type.collectionarticulo
dc.type.versionpublishedVersion

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