Aviso: para depositar documentos, por favor, inicia sesión e identifícate con tu cuenta de correo institucional de la UCM con el botón MI CUENTA UCM. No emplees la opción AUTENTICACIÓN CON CONTRASEÑA
 

Ultrahigh Energy Neutrinos at the Pierre Auger Observatory

Simple item page
dc.contributor.authorArganda, E.
dc.contributor.authorArqueros Martínez, Fernando
dc.contributor.authorBlanco Ramos, Francisco
dc.contributor.authorGarcía Pinto, Diego
dc.contributor.authorMinaya Flores, Ignacio Andrés
dc.contributor.authorOrtiz Ramis, Montserrat
dc.contributor.authorRosado Vélez, Jaime
dc.contributor.authorVázquez Peñas, José Ramón
dc.date.accessioned2023-06-19T14:55:49Z
dc.date.available2023-06-19T14:55:49Z
dc.date.issued2013
dc.description© 2013 Hindawi Publishing Corporation. The successful installation, commissioning, and operation of the Pierre Auger Observatory would not have been possible without the strong commitment and effort from the technical and administrative staff in Malargue. The authors are very grateful to the following agencies and organizations for financial support: Comision Nacional de Energia Atomica, Fundacion Antorchas, Gobierno De La Provincia de Mendoza, Municipalidad de Malargue, NDM Holdings and Valle Las Lenas, in gratitude for their continuing cooperation over land access, Argentina; the Australian Research Council; Conselho Nacional de Desenvolvimento Cientifico e Tecnologico (CNPq), Financiadora de Estudos e Projetos (FINEP), Fundacao de Amparo a Pesquisa do Estado de Rio de Janeiro (FAPERJ), Fundacao de Amparo a Pesquisa do Estado de Sao Paulo (FAPESP), Ministerio de Ciencia e Tecnologia (MCT), Brazil; AVCR AV0Z10100502 and AV0Z10100522, GAAV KJB100100904, MSMT-CR LA08016, LG11044, MEB111003, MSM0021620859, LA08015, and TACR TA01010517, Czech Republic; Centre de Calcul IN2P3/CNRS, Centre National de la Recherche Scientifique (CNRS), Conseil Regional Ile-deFrance, Departement Physique Nucleaire et Corpusculaire (PNC-IN2P3/CNRS), Departement Sciences de l'Univers (SDU-INSU/CNRS), France; Bundesministerium fur Bildung und Forschung (BMBF), Deutsche Forschungsgemeinschaft (DFG), Finanzministerium Baden-Wurttemberg, Helmholtz-Gemeinschaft Deutscher Forschungszentren (HGF), Ministerium fur Wissenschaft und Forschung, Nordrhein-Westfalen, Ministerium fur Wissenschaft, Forschung und Kunst, Baden-Wurttemberg, Germany; Istituto Nazionale di Fisica Nucleare (INFN), Ministero dell'Istruzione, dell'Universita e della Ricerca (MIUR), Italy; Consejo Nacional de Ciencia y Tecnologia (CONACYT), Mexico; Ministerie van Onderwijs, Cultuur en Wetenschap, Nederlandse Organisatie voor Wetenschappelijk Onderzoek (NWO), Stichting voor Fundamenteel Onderzoek der Materie (FOM), The Netherlands; Ministry of Science and Higher Education, Grants no. N N202 200239 and N N202 2038, Poland; Fundacao para a Ciencia e a Tecnologia, Portugal; Ministry for Higher Education, Science, and Technology, Slovenian Research Agency, Slovenia; Comunidad de Madrid, Consejeria de Educacion de la Comunidad de Castilla La Mancha, FEDER funds, Ministerio de Ciencia e Innovacion and Consolider-Ingenio 2010 (CPAN), Xunta de Galicia, Spain; Science and Technology Facilities Council, UK; Department of Energy, Contract nos. DE-AC02-07CH11359 and DE-FR02-04ER41300, National Science Foundation, Grant no. 0450696, The Grainger Foundation, USA; NAFOSTED, Vietnam; ALFA-EC/HELEN and UNESCO.
dc.description.abstractThe observation of ultrahigh energy neutrinos (UHE nu s) has become a priority in experimental astroparticle physics. UHE nu s can be detected with a variety of techniques. In particular, neutrinos can interact in the atmosphere (downward-going nu) or in the Earth crust (Earth-skimming nu), producing air showers that can be observed with arrays of detectors at the ground. With the surface detector array of the Pierre Auger Observatory we can detect these types of cascades. The distinguishing signature for neutrino events is the presence of very inclined showers produced close to the ground (i.e., after having traversed a large amount of atmosphere). In this work we review the procedure and criteria established to search for UHE nu s in the data collected with the ground array of the Pierre Auger Observatory. This includes Earth-skimming as well as downward-going neutrinos. No neutrino candidates have been found, which allows us to place competitive limits to the diffuse flux of UHE nu s in the EeV range and above.
dc.description.departmentDepto. de Estructura de la Materia, Física Térmica y Electrónica
dc.description.facultyFac. de Ciencias Físicas
dc.description.refereedTRUE
dc.description.sponsorshipAVCR, Czech Republic
dc.description.sponsorshipGAAV, Czech Republic
dc.description.sponsorshipMSMT-CR, Czech Republic
dc.description.sponsorshipTACR, Czech Republic
dc.description.sponsorshipCentre de Calcul IN2P3/CNRS
dc.description.sponsorshipCentre National de la Recherche Scientifique (CNRS), France
dc.description.sponsorshipConseil Regional Ile-de-France
dc.description.sponsorshipDepartement Physique Nucleaire et Corpusculaire (PNC-IN2P3/CNRS)
dc.description.sponsorshipDepartement Sciences de l'Univers (SDU-INSU/CNRS), France
dc.description.sponsorshipBundesministerium fur Bildung und Forschung (BMBF)
dc.description.sponsorshipDeutsche Forschungsgemeinschaft (DFG)
dc.description.sponsorshipFinanzministerium Baden-Wurttemberg, Germany
dc.description.sponsorshipHelmholtz-Gemeinschaft Deutscher Forschungszentren (HGF)
dc.description.sponsorshipMinisterium fur Wissenschaft und Forschung Nordrhein-Westfalen
dc.description.sponsorshipMinisterium fur Wissenschaft Forschung
dc.description.sponsorshipKunst Baden-Wurttemberg, Germany
dc.description.sponsorshipIstituto Nazionale di Fisica Nucleare (INFN)
dc.description.sponsorshipMinistero dell'Istruzione, dell'Universita e della Ricerca (MIUR), Italy
dc.description.sponsorshipMinisterie van Onderwijs, Cultuur en Wetenschap, Netherlands
dc.description.sponsorshipNederlandse Organisatie voor Wetenschappelijk Onderzoek (NWO)
dc.description.sponsorshipStichting voor Fundamenteel Onderzoek der Materie (FOM), The Netherlands
dc.description.sponsorshipMinistry of Science and Higher Education, Poland
dc.description.sponsorshipFundacao para a Ciencia e a Tecnologia, Portugal
dc.description.sponsorshipMinistry for Higher Education, Science, and Technology, Slovenian
dc.description.sponsorshipResearch Agency, Slovenia
dc.description.sponsorshipComunidad de Madrid, Spain
dc.description.sponsorshipConsejeria de Educacion de la Comunidad de Castilla La Mancha, Spain
dc.description.sponsorshipFEDER funds, Spain
dc.description.sponsorshipMinisterio de Ciencia e Innovacion and Consolider-Ingenio 2010 (CPAN)
dc.description.sponsorshipXunta de Galicia, Spain
dc.description.sponsorshipScience and Technology Facilities Council, UK
dc.description.sponsorshipALFA-EC/HELEN
dc.description.sponsorshipUNESCO
dc.description.statuspub
dc.eprint.idhttps://eprints.ucm.es/id/eprint/32661
dc.identifier.doi10.1155/2013/708680
dc.identifier.issn1687-7357
dc.identifier.officialurlhttp://dx.doi.org/10.1155/2013/708680
dc.identifier.relatedurlhttp://www.hindawi.com/
dc.identifier.urihttps://hdl.handle.net/20.500.14352/34828
dc.journal.titleAdvances in high energy physics
dc.language.isoeng
dc.publisherHindawi Publishing Corporation
dc.relation.projectIDAV0Z10100502
dc.relation.projectIDAV0Z10100522
dc.relation.projectIDKJB100100904
dc.relation.projectIDLA08016
dc.relation.projectIDLG11044
dc.relation.projectIDMEB111003
dc.relation.projectIDMSM0021620859
dc.relation.projectIDLA08015
dc.relation.projectIDTA01010517
dc.relation.projectIDN N202 200239
dc.relation.projectIDN N202 2038
dc.rightsAtribución 3.0 España
dc.rights.accessRightsopen access
dc.rights.urihttps://creativecommons.org/licenses/by/3.0/es/
dc.subject.cdu539.1
dc.subject.keywordCosmic-rays
dc.subject.keywordAir-showers
dc.subject.keywordTau-neutrinos
dc.subject.keywordFlux
dc.subject.keywordSpectrum
dc.subject.keywordSearch
dc.subject.keywordArray
dc.subject.keywordLimit.
dc.subject.ucmFísica nuclear
dc.subject.unesco2207 Física Atómica y Nuclear
dc.titleUltrahigh Energy Neutrinos at the Pierre Auger Observatory
dc.typejournal article
dcterms.references[1] M. Nagano and A. A. Watson, “Observations and implications of the ultrahigh-energy cosmic rays,” Reviews of Modern Physics, vol. 72, no. 3, pp. 689–732, 2000. [2] K. Kotera and A. Olinto, “The astrophysics of ultrahigh-energy cosmic rays,” Annual Review of Astronomy and Astrophysics, vol. 49, pp. 119–153, 2010. [3] F. Halzen and D. Hooper, “High-energy neutrino astronomy: the cosmic ray connection,” Reports on Progress in Physics, vol. 65, no. 7, p. 1025, 2002. [4] J. K. Becker, “High-energy neutrinos in the context of multimessenger astrophysics,” Physics Reports, vol. 458, no. 4-5, pp. 173–246, 2008. [5] P. Bhattacharjee and G. Sigl, “Origin and propagation of extremely high-energy cosmic rays,” Physics Reports, vol. 327, no. 3-4, pp. 109–247, 2000. [6] K. Greisen, “End to the cosmic-ray spectrum?” Physical Review Letters, vol. 16, pp. 748 750, 1966. [7] G. T. Zatsepin and V. A. Kuzmin, “Upper limit of the spectrum of cosmic rays,” Pis’ma v Zhurnal Eksperimental noi i Teoreticheskoi Fiziki, vol. 4, p. 114, 1966, English translation in: JETP Letters, vol. 4, p. 78, 1966. [8] V. S. Berezinsky and G. T. Zatsepin, “Cosmic rays at ultra high energies (neutrino?),” Physics Letters B, vol. 28, no. 6, pp. 423–424, 1969. [9] R. U. Abbasi, T. Abu-Zayyad, M. Allen et al., “First Observation of the Greisen-Zatsepin-Kuzmin Suppression,” Physical Review Letters, vol. 100, no. 10, article 101101, 5 pages, 2008. [10] J. Abraham, P. Abreu, M. Aglietta et al., “Observation of the suppression of the flux of cosmic rays above 4×1019 eV,” Physical Review Letters, vol. 101, no. 6, article 061101, 7 pages, 2008. [11] J. Abraham, P. Abreu, M. Aglietta et al., “Measurement of the energy spectrum of cosmic rays above 1018 eV using the pierre auger observatory,” Physical Letters B, vol. 685, no. 4-5, pp. 239–246, 2010.
dspace.entity.typePublication
relation.isAuthorOfPublicatione6fd6d50-2946-45a9-a515-273dddff2091
relation.isAuthorOfPublicationfd97b031-5b10-40ab-beb5-8f192e632ca3
relation.isAuthorOfPublication7c75d106-b698-42ee-bfea-fe4a2b11b7f8
relation.isAuthorOfPublication8385de5d-023a-4c39-8d07-80f84fe48bcd
relation.isAuthorOfPublication32033072-414c-4448-b44b-98a6bd3e9321
relation.isAuthorOfPublication.latestForDiscoverye6fd6d50-2946-45a9-a515-273dddff2091

Download

Original bundle

Now showing 1 - 1 of 1
Thumbnail Image
Name:
arqueros23libre+CC.pdf
Size:
3.98 MB
Format:
Adobe Portable Document Format
downoload Download

Collections

Artículos