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Bounds on the density of sources of ultra-high energy cosmic rays from the Pierre Auger Observatory

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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.accessioned2023-06-19T14:55:37Z
dc.date.available2023-06-19T14:55:37Z
dc.date.issued2013-05
dc.description© Iop Publishing Ltd 2013. Autoría conjunta: Pierre Auger Collaboration. Artículo firmado por mas de 500 autores. We are very grateful to the following agencies and organizations for financial support,: Comision Nacional de Energia Atomica, Fundacion Antorchas, Gobierno De La, Provincia de Ailendoza. Municipalidad de Malargile. INDM floldings 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), Fundacdo de Amparo a Pesquisa do Est ado de Rio de Janeiro (FAP HRJ), Fundacdo de Amparo Pesquisa do Estado de Sdo Paulo (FAPESP), Ministerio de Ciencia e Tecnologia (IVICT), Brazil; AVCR AVOZ10100502 and AVOZ10100522, GAAV KJB100100904, AISMT-CR LA08016, LG11044, 1VIEB111003, MSAI0021620859, LA08015, TACR TA01010517 and GA U.K. 119810, Czech Republic; Centre de Calcul I-N2P3/CNRS, Centre National de la -Recherche Scientifique ((1 NRS), Conseil Regional Ile-de-France,Conseil Régional Ile-de-France Département Physique Nucléaire et Corpusculaire (PNC-IN2P3/CNRS) Département Sciences de l'Univers (SDU-INSU/CNRS), France; Bundesministerium fur Bildung und Forschung (BMBF), Deutsche Forschungsgemeinschaft (DITG), Finanzministerium Baden-Wurttemberg, flelmholtz-Gemeinschaft Deutscher Forschungszentren Ministerium fur Wissenschaft und Forschung, Nordrhein-Westfalen, Ministerimn fur Wissenschaft, Forschung und Kunst, Baden-WUrttemberg, Germany; Istituto Nazion ale di Fisica Nucleare (INFN), Ministero dell'Istruzione, delhLniversita e della Ricerca (MIUR), Italy: Consejo Nacional de Ciencia y Tecnologia (CONACYT), Mexico; Ministerie van Onden s Cultuur on NVetenschap Nederlandse Organisatie voor Wetenschappelijk Onderzoek (NWO), Stichting voor Rmdamenteel Onderzoek der Materie (FOM), Netherlands; Ministry of Science and Higher Education, Grant Nos. N N202 200239 and N N202 207238, Poland; Portuguese national funds and FEDER funds within COMPETE - Programa Operacional Factores de Competitividade through Fundacao para a Ciencia e a Tecnologia, Portugal; Romanian Authority for Scientific Research ANCS, CNDI-UEFISETD1 partnership projects nr.20/2012 and nr.194/2012, project nr.1 /ASPERA2/20I2 ERA-NET and PN-IIRU-PD-2011-3-0145-17, Romania; Ministry for Higher Education, Science, and 'Technology, Slovenian Research Agency, Slovenia; Comunidad de Madrid, FEDER funds, Ministerio de Ciencia e Innovacion and Consolider-Ingenio 2010 (( PAN), X unta de Galicia Spain; Science and Technology Facilities Council, United kingdom; Department of Luergy, Contract Nos. DE-ACO2-07(11-111359, DE-FR02-04E1(41300, DE-FG02-99E1(41107, National Science Foundation, Grant No. 0450696, The Grainger Foundation U.S.A.; NAFOSTED, Vietnam; Marie Curie-IRSES/HPLANET, European Particle Physics Latin American Network, European Union 7th Frarneworlc Program. Grant No. IIRSES-2009-GA-246806; and UNESCO.
dc.description.abstractWe derive lower bounds on the density of sources of ultra-high energy cosmic rays from the lack of significant clustering in the arrival directions of the highest energy events detected at the Pierre Auger Observatory. The density of uniformly distributed sources of equal intrinsic intensity was found to be larger than similar to (0.06 - 5) x 10(-4) Mpc(-3) at 95% CL, depending on the magnitude of the magnetic defections. Similar bounds, in the range (0.2 - 7) x 10(-4) Mpc(-3), were obtained for sources following the local matter distribution.
dc.description.departmentDepto. de Estructura de la Materia, Física Térmica y Electrónica
dc.description.facultyFac. de Ciencias Físicas
dc.description.refereedTRUE
dc.description.sponsorshipUnión Europea. FP7
dc.description.sponsorshipCentre de Calcul IN2P3/CNRS
dc.description.sponsorshipCentre National de la -Recherche Scientifique (CNRS)
dc.description.sponsorshipConseil Regional Ile-de-France
dc.description.sponsorshipDépartement Physique Nucléaire et Corpusculaire (PNC-IN2P3/CNRS)
dc.description.sponsorshipDépartement Sciences de l'Univers (SDU-INSU/CNRS).
dc.description.sponsorshipBundesministerium fur Bildung und Forschung (BMBF)
dc.description.sponsorshipDeutsche Forschungsgemeinschaft (DITG)
dc.description.sponsorshipFinanzministerium Baden-Wurttemberg
dc.description.sponsorshipHelmholtz-Gemeinschaft Deutscher Forschungszentren (HGF)
dc.description.sponsorshipMinisterium für Wissenschaft und Forschung, Nordrhein-Westfalen
dc.description.sponsorshipMinisterimn fur Wissenschaft, Forschung und Kunst, Baden-Württemberg
dc.description.sponsorshipIstituto Nazion ale di Fisica Nucleare (INFN)
dc.description.sponsorshipMinistero dell'Istruzione, delhLniversita e della Ricerca (MIUR)
dc.description.sponsorshipMinisterie van Onden s Cultuur en Wetenschap
dc.description.sponsorshipNederlandse Organisatie voor Wetenschappelijk Onderzoek (NWO)
dc.description.sponsorshipStichting voor Fundamenteel Onderzoek der Materie (FOM), Netherlands
dc.description.sponsorshipMinistry of Science and Higher Education, Poland
dc.description.sponsorshipFundacao para a Ciencia e a Tecnologia
dc.description.sponsorshipFEDER funds within COMPETE - Programa Operacional Factores de Competitividade
dc.description.sponsorshipRomanian Authority for Scientific Research ANCS
dc.description.sponsorshipCNDI-UEFISETDI
dc.description.sponsorshipMinistry for Higher Education, Science, and Technology
dc.description.sponsorshipSlovenian Research Agency
dc.description.sponsorshipMinisterio de Ciencia e Innovacion and Consolider-Ingenio 2010 ( CPAN)
dc.description.sponsorshipComunidad de Madrid, FEDER funds
dc.description.sponsorshipXunta de Galicia, Spain
dc.description.sponsorshipScience and Technology Facilities Council, United Kingdom
dc.description.sponsorshipUNESCO
dc.description.statuspub
dc.eprint.idhttps://eprints.ucm.es/id/eprint/32509
dc.identifier.doi10.1088/1475-7516/2013/05/009
dc.identifier.issn1475-7516
dc.identifier.officialurlhttp://dx.doi.org/10.1088/1475-7516/2013/05/009
dc.identifier.relatedurlhttp://iopscience.iop.org/
dc.identifier.relatedurlhttp://arxiv.org/abs/1305.1576
dc.identifier.urihttps://hdl.handle.net/20.500.14352/34811
dc.issue.number5
dc.journal.titleJournal of Cosmology and Astroparticle Physics
dc.language.isoeng
dc.publisherIOP Publishing Ltd
dc.relation.projectIDPIRSES-2009-GA (246806)
dc.relation.projectIDAVCR AVOZ10100502
dc.relation.projectIDAVOZ10100522
dc.relation.projectIDGAAV KJB100100904
dc.relation.projectIDAISMT-CR LA08016
dc.relation.projectIDLG11044, 1VIEB111003
dc.relation.projectIDMSAI0021620859
dc.relation.projectIDLA08015
dc.relation.projectIDTACR TA01010517
dc.relation.projectIDGA U.K. 119810
dc.relation.projectIDN N202 200239
dc.relation.projectIDN N202 207238
dc.relation.projectID20/2012
dc.relation.projectID194/2012
dc.relation.projectID1 /ASPERA2/20I2 ERA-NET
dc.relation.projectIDPN-IIRU-PD-2011-3-0145-17
dc.rights.accessRightsopen access
dc.subject.cdu539.1
dc.subject.keywordLuminosity function
dc.subject.keywordSpectrum
dc.subject.keywordNumber
dc.subject.keywordDetector
dc.subject.ucmFísica nuclear
dc.subject.unesco2207 Física Atómica y Nuclear
dc.titleBounds on the density of sources of ultra-high energy cosmic rays from the Pierre Auger Observatory
dc.typejournal article
dcterms.references[1] K. Greisen, Phys. Rev. Lett. 16 (1966) 748; G. T. Zatsepin and V. A. Kuz’min, JETP Lett. 4 (1966) 78. [2] R. U. Abbasi et al. (HiRes Collaboration), Phys. Rev. Lett. 100 (2008) 101101. [3] J. Abraham et al. (The Pierre Auger Collaboration), Phys. Rev. Lett. 100 (2008) 211101; J. Abraham et al. (The Pierre Auger Collaboration), Phys. Lett. B 685 (2010) 239. [4] C. S. Kochanek et al., Astrophys. J. 560 (2001) 566. [5] A. T. Steffen et al., Astrophys. J. Lett. 596 (2003) L3; S. Sazonov et al., Astron. and Astrophys. J. 462 (2007) 57; J. Tueller et al., Astrophys. J. 681 (2008) 113. [6] R. G. Carlberg et al., Astrophys. J. Lett. 479 (1997) L19. [7] K. Dolag et al. JCAP 0501 (2005) 009. [8] E. Armengaud, G. Sigl and F. Miniati, Phys. Rev. D 72 (2005) 043009. [9] J. Abraham et al. (The Pierre Auger Collaboration), Phys. Rev. Lett. 104 (2010) 091101. [10] P. Facal San Luis for the Pierre Auger Collaboration, Proc. 32nd ICRC (2011) [arXiv:1107.4804]. [11] D. Garcia-Pinto for the Pierre Auger Collaboration, Proc. 32nd ICRC (2011) [arXiv:1107.4804]. [12] R. U. Abbasi et al. (HiRes Collaboration), Phys. Rev. Lett. 104 (2010) 161101. [13] C. Jui et al. (TA Collaboration) Proc. APS DPF Meeting [arXiv:1110.0133]. [14] S. L. Dubovsky, P. G. Tinyakov and I. I. Tkachev, Phys. Rev. Lett. 85 (2000) 1154. [15] Z. Fodor and S. D. Katz, Phys. Rev. D 63 (2000) 23002. [16] H. Yoshiguchi et al., Astrophys. J. 586 (2003) 1211. [17] P. Blasi and S. De Marco, Astrop. Phys. 20 (2004) 559. [18] G. Sigl, F. Miniati and T. A. Enßlin, Phys. Rev. D 70 (2004) 043007. [19] M. Kachelriess and D. Semikoz, Astrop. Phys. 23 (2005) 486. [20] A. Cuoco et al., Astrophys. J. 702 (2009) 825. [21] H. Takami and K. Sato, Astrop. Phys. 30 (2009) 306. [22] T. Abu-Zayyad et al. (TA Collaboration), Astrophys. J. 757 (2012) 26. [23] J. P. Huchra et al., Astrophys. J. Suppl. 199 (2012) 26. [24] M. de Domenico for the Pierre Auger Collaboration, Proc. 32nd ICRC (2011) [arXiv:1107.4805]. [25] J. Abraham et al. (The Pierre Auger Collaboration), NIM A 523 (2004) 50. [26] I. Allekotte et al. (The Pierre Auger Collaboration), NIM A 586 (2008) 409. [27] J. Abraham et al. (The Pierre Auger Collaboration), NIM A 620 (2010) 227. [28] C. Bonifazi, for The Pierre Auger Collaboration, Nucl. Phys. B (Proc. Suppl.) 190 (2009) 20. [29] R. Pesce, for The Pierre Auger Collaboration, Proc. 32nd ICRC (2011) [arXiv:1107.4809]. [30] K.-H. Kampert et al., [arXiv:1206.3132]. [31] G. Cowan, Review of Particle Physics, Phys. Rev. D 86, 010001 (2012) 390. [32] D. Harari, S. Mollerach and E. Roulet, JCAP 11(2006)012. [33] P. Abreu et al. (Pierre Auger Collaboration), Astropart. Phys. 34 (2010) 314. [34] B. T. Soifer et al., Astrophys. J. Lett. 303 (1986) L41.
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