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Features of the Energy Spectrum of Cosmic Rays above 2.5 × 10(18) eV Using the Pierre Auger Observatory

dc.contributor.authorAab, A.
dc.contributor.authorBueno Villar, Antonio 
dc.date.accessioned2020-10-30T07:07:56Z
dc.date.available2020-10-30T07:07:56Z
dc.date.issued2020-09-16
dc.identifier.citationAab, A., Abreu, P., Aglietta, M., Albury, J. M., Allekotte, I., Almela, A., ... & Anchordoqui, L. (2020). Features of the Energy Spectrum of Cosmic Rays above 2.5× 10 18 eV Using the Pierre Auger Observatory. Physical Review Letters, 125(12), 121106. [doi:10.1103/PhysRevLett.125.121106]es_ES
dc.identifier.urihttp://hdl.handle.net/10481/63960
dc.description.abstract2.51 0.03ðstatÞ 0.05ðsystÞ to 3.05 0.05ðstatÞ 0.10ðsystÞ, evolving to 5.1 0.3ðstatÞ 0.1ðsystÞ beyond 5 × 1019 eV, while no significant dependence of spectral features on the declination is seen in the accessible range. These features of the spectrum can be reproduced in models with energy-dependent mass composition. The energy density in cosmic rays above 5×1018 eV is ½5.66 0.03ðstatÞ 1.40ðsystÞ × 1053 ergMpc−3es_ES
dc.description.sponsorshipFundacao de Amparo a Pesquisa do Estado de Sao Paulo (FAPESP) 2019/10151-2 2010/07359-6 1999/05404-3es_ES
dc.description.sponsorshipCzech Republic Grant MSMT CR LTT18004 LM2015038 LM2018102 CZ.02.1.01/0.0/0.0/16_013/0001402 CZ.02.1.01/0.0/0.0/18_046/0016010 CZ.02.1.01/0.0/0.0/17_049/0008422es_ES
dc.description.sponsorshipFrench National Research Agency (ANR) LABEX ANR-10-LABX-63 ANR11-IDEX-0004-02es_ES
dc.description.sponsorshipConsejo Nacional de Ciencia y Tecnologia (CONACyT) 167733es_ES
dc.description.sponsorshipSURF Cooperativees_ES
dc.description.sponsorshipPoland-Ministry of Science and Higher Education DIR/WK/2018/11es_ES
dc.description.sponsorshipNational Science Center, Poland National Science Centre, Poland 2013/08/M/ST9/00322 2016/23/B/ST9/01635 HARMONIA 5-2013/10/M/ST9/00062 UMO-2016/22/M/ST9/00198es_ES
dc.description.sponsorshipPortugal-Portuguese national funds within Programa Operacional Factores de Competitividade through Fundacao para a Ciencia e a Tecnologia (COMPETE)es_ES
dc.description.sponsorshipFEDER funds within Programa Operacional Factores de Competitividade through Fundacao para a Ciencia e a Tecnologia (COMPETE)es_ES
dc.description.sponsorshipProgram Nucleu within MCI within PNCDI III PN19150201/16N/2019 PN19060102 PN-III-P1-1.2-PCCDI-2017-0839/19PCCDI/2018es_ES
dc.description.sponsorshipSlovenia-Slovenian Research Agency P1-0031 P1-0385 I00033 N1-0111es_ES
dc.description.sponsorshipSpain-Ministerio de Economía, Industria y Competitividad FPA2017-85114-P FPA2017-85197-Pes_ES
dc.description.sponsorshipXunta de Galicia ED431C 2017/07es_ES
dc.description.sponsorshipJunta de Andalucía SOMM17/6104/UGRes_ES
dc.description.sponsorshipFeder Funds, RENATA Red Nacional Tematica de Astroparticulas FPA2015-68783-REDTes_ES
dc.description.sponsorshipMaria de Maeztu Unit of Excellence MDM-2016-0692es_ES
dc.description.sponsorshipUnited States Department of Energy (DOE) DE-AC0207CH11359 DE-FR02-04ER41300 DE-FG0299ER41107 DE-SC0011689es_ES
dc.description.sponsorshipNational Science Foundation (NSF) 0450696es_ES
dc.language.isoenges_ES
dc.publisherAmer Physical Soces_ES
dc.rightsAtribución-NoComercial-SinDerivadas 3.0 España*
dc.rights.urihttp://creativecommons.org/licenses/by-nc-nd/3.0/es/*
dc.titleFeatures of the Energy Spectrum of Cosmic Rays above 2.5 × 10(18) eV Using the Pierre Auger Observatoryes_ES
dc.typeinfo:eu-repo/semantics/articlees_ES
dc.rights.accessRightsinfo:eu-repo/semantics/openAccesses_ES
dc.identifier.doi10.1103/PhysRevLett.125.121106
dc.type.hasVersioninfo:eu-repo/semantics/publishedVersiones_ES


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