Home > Publications database > Active galactic nuclei jets as the origin of ultrahigh-energy cosmic rays and perspectives for the detection of astrophysical source neutrinos at EeV energies > print

001     457130
005     20250724175407.0
024 7 _ |a 10.1103/PhysRevLett.126.191101
|2 doi
024 7 _ |a Rodrigues:2020pli
|2 INSPIRETeX
024 7 _ |a inspire:1787069
|2 inspire
024 7 _ |a 0031-9007
|2 ISSN
024 7 _ |a 1079-7114
|2 ISSN
024 7 _ |a 1092-0145
|2 ISSN
024 7 _ |a arXiv:2003.08392
|2 arXiv
024 7 _ |a 10.3204/PUBDB-2021-01868
|2 datacite_doi
024 7 _ |a altmetric:77921946
|2 altmetric
024 7 _ |a pmid:34047601
|2 pmid
024 7 _ |a WOS:000652838300004
|2 WOS
024 7 _ |a openalex:W3162846926
|2 openalex
037 _ _ |a PUBDB-2021-01868
041 _ _ |a English
082 _ _ |a 530
088 _ _ |a DESY-20-095
|2 DESY
088 _ _ |a arXiv:2003.08392
|2 arXiv
100 1 _ |a de Sousa Ferreira Rodrigues, Xavier
|0 P:(DE-H253)PIP1028911
|b 0
|e Corresponding author
|u desy
245 _ _ |a Active galactic nuclei jets as the origin of ultrahigh-energy cosmic rays and perspectives for the detection of astrophysical source neutrinos at EeV energies
260 _ _ |a College Park, Md.
|c 2021
|b APS
336 7 _ |a article
|2 DRIVER
336 7 _ |a Output Types/Journal article
|2 DataCite
336 7 _ |a Journal Article
|b journal
|m journal
|0 PUB:(DE-HGF)16
|s 1622457034_32466
|2 PUB:(DE-HGF)
336 7 _ |a ARTICLE
|2 BibTeX
336 7 _ |a JOURNAL_ARTICLE
|2 ORCID
336 7 _ |a Journal Article
|0 0
|2 EndNote
500 _ _ |a Phys. Rev. Lett. 126, 191101 (2021). Manuscript accepted for publication in Phys. Rev. Lett
520 _ _ |a We demonstrate that a population of active galactic nuclei (AGN) can describe the observed spectrum of ultra-high-energy cosmic rays (UHECRs) at and above the ankle, and that the dominant contribution comes from low-luminosity BL Lacertae objects. An additional, subdominant contribution from high-luminosity AGN is needed to improve the description of the composition observables, leading to a substantial neutrino flux that peaks at exaelectronvolt (EeV) energies. We also find that different properties for the low- and high-luminosity AGN populations are required; a possibly similar baryonic loading can already be excluded from current IceCube Neutrino Observatory observations. We also show that the flux of neutrinos emitted from within the sources should outshine the cosmogenic neutrinos produced during the propagation of UHECRs. This result has profound implications for the ultra-high-energy (∼EeV) neutrino experiments, since additional search strategies can be used for source neutrinos compared to cosmogenic neutrinos, such as stacking searches, flare analyses, and multimessenger follow-ups.
536 _ _ |a 613 - Matter and Radiation from the Universe (POF4-613)
|0 G:(DE-HGF)POF4-613
|c POF4-613
|x 0
|f POF IV
536 _ _ |a NEUCOS - Neutrinos and the origin of the cosmic rays (646623)
|0 G:(EU-Grant)646623
|c 646623
|x 1
|f ERC-2014-CoG
588 _ _ |a Dataset connected to CrossRef, INSPIRE, Journals: bib-pubdb1.desy.de
650 _ 7 |a cosmic radiation: UHE
|2 INSPIRE
650 _ 7 |a cosmic radiation: spectrum
|2 INSPIRE
650 _ 7 |a neutrino: flux
|2 INSPIRE
650 _ 7 |a neutrino: energy: high
|2 INSPIRE
650 _ 7 |a blazar
|2 INSPIRE
650 _ 7 |a messenger
|2 INSPIRE
650 _ 7 |a propagation
|2 INSPIRE
650 _ 7 |a stacking
|2 INSPIRE
650 _ 7 |a Gravitation and Astrophysics
|2 autogen
693 _ _ |0 EXP:(DE-H253)IceCube-20150101
|5 EXP:(DE-H253)IceCube-20150101
|e IceCube South Pole Neutrino Observatory
|x 0
693 _ _ |0 EXP:(DE-MLZ)NOSPEC-20140101
|5 EXP:(DE-MLZ)NOSPEC-20140101
|e No specific instrument
|x 1
700 1 _ |a Heinze, Jonas
|0 P:(DE-H253)PIP1025586
|b 1
|u desy
700 1 _ |a Palladino, Andrea
|0 P:(DE-H253)PIP1082506
|b 2
700 1 _ |a van Vliet, Arjen
|0 P:(DE-HGF)0
|b 3
700 1 _ |a Winter, Walter
|0 P:(DE-H253)PIP1021242
|b 4
773 _ _ |a 10.1103/PhysRevLett.126.191101
|g Vol. 126, no. 19, p. 191101
|0 PERI:(DE-600)1472655-5
|n 19
|p 191101 (1-6)
|t Physical review letters
|v 126
|y 2021
|x 0031-9007
787 0 _ |a de Sousa Ferreira Rodrigues, Xavier et.al.
|d 2021
|i IsParent
|0 PUBDB-2020-03344
|r arXiv:2003.08392 ; DESY-20-095
|t AGN jets as the origin of UHECRs and perspectives for the detection of EeV astrophysical neutrinos
856 4 _ |u https://bib-pubdb1.desy.de/record/457130/files/Admin-Rodrigues.pdf
856 4 _ |x pdfa
|u https://bib-pubdb1.desy.de/record/457130/files/Admin-Rodrigues.pdf?subformat=pdfa
856 4 _ |y OpenAccess
|u https://bib-pubdb1.desy.de/record/457130/files/PRL126%282021%29191101.pdf
856 4 _ |y OpenAccess
|x pdfa
|u https://bib-pubdb1.desy.de/record/457130/files/PRL126%282021%29191101.pdf?subformat=pdfa
909 C O |o oai:bib-pubdb1.desy.de:457130
|p openaire
|p open_access
|p OpenAPC
|p driver
|p VDB
|p ec_fundedresources
|p openCost
|p dnbdelivery
910 1 _ |a Deutsches Elektronen-Synchrotron
|0 I:(DE-588b)2008985-5
|k DESY
|b 0
|6 P:(DE-H253)PIP1028911
910 1 _ |a Deutsches Elektronen-Synchrotron
|0 I:(DE-588b)2008985-5
|k DESY
|b 1
|6 P:(DE-H253)PIP1025586
910 1 _ |a Deutsches Elektronen-Synchrotron
|0 I:(DE-588b)2008985-5
|k DESY
|b 2
|6 P:(DE-H253)PIP1082506
910 1 _ |a Deutsches Elektronen-Synchrotron
|0 I:(DE-588b)2008985-5
|k DESY
|b 3
|6 P:(DE-HGF)0
910 1 _ |a Deutsches Elektronen-Synchrotron
|0 I:(DE-588b)2008985-5
|k DESY
|b 4
|6 P:(DE-H253)PIP1021242
913 0 _ |a DE-HGF
|b Forschungsbereich Materie
|l Materie und Universum
|1 G:(DE-HGF)POF3-610
|0 G:(DE-HGF)POF3-613
|3 G:(DE-HGF)POF3
|2 G:(DE-HGF)POF3-600
|4 G:(DE-HGF)POF
|v Matter and Radiation from the Universe
|x 0
913 1 _ |a DE-HGF
|b Forschungsbereich Materie
|l Matter and the Universe
|1 G:(DE-HGF)POF4-610
|0 G:(DE-HGF)POF4-613
|3 G:(DE-HGF)POF4
|2 G:(DE-HGF)POF4-600
|4 G:(DE-HGF)POF
|v Matter and Radiation from the Universe
|x 0
914 1 _ |y 2021
915 _ _ |a DBCoverage
|0 StatID:(DE-HGF)0200
|2 StatID
|b SCOPUS
|d 2021-02-02
915 _ _ |a DBCoverage
|0 StatID:(DE-HGF)0160
|2 StatID
|b Essential Science Indicators
|d 2021-02-02
915 _ _ |a DBCoverage
|0 StatID:(DE-HGF)1230
|2 StatID
|b Current Contents - Electronics and Telecommunications Collection
|d 2021-02-02
915 _ _ |a DBCoverage
|0 StatID:(DE-HGF)0600
|2 StatID
|b Ebsco Academic Search
|d 2021-02-02
915 _ _ |a American Physical Society Transfer of Copyright Agreement
|0 LIC:(DE-HGF)APS-112012
|2 HGFVOC
915 _ _ |a DBCoverage
|0 StatID:(DE-HGF)1150
|2 StatID
|b Current Contents - Physical, Chemical and Earth Sciences
|d 2021-02-02
915 _ _ |a Peer Review
|0 StatID:(DE-HGF)0030
|2 StatID
|b ASC
|d 2021-02-02
915 _ _ |a WoS
|0 StatID:(DE-HGF)0113
|2 StatID
|b Science Citation Index Expanded
|d 2021-02-02
915 _ _ |a DBCoverage
|0 StatID:(DE-HGF)0150
|2 StatID
|b Web of Science Core Collection
|d 2021-02-02
915 _ _ |a OpenAccess
|0 StatID:(DE-HGF)0510
|2 StatID
915 _ _ |a DBCoverage
|0 StatID:(DE-HGF)0571
|2 StatID
|b SCOAP3 sponsored Journal
|d 2021-02-02
915 _ _ |a JCR
|0 StatID:(DE-HGF)0100
|2 StatID
|b PHYS REV LETT : 2019
|d 2021-02-02
915 _ _ |a DBCoverage
|0 StatID:(DE-HGF)0300
|2 StatID
|b Medline
|d 2021-02-02
915 _ _ |a IF >= 5
|0 StatID:(DE-HGF)9905
|2 StatID
|b PHYS REV LETT : 2019
|d 2021-02-02
915 _ _ |a Nationallizenz
|0 StatID:(DE-HGF)0420
|2 StatID
|d 2021-02-02
|w ger
915 _ _ |a DBCoverage
|0 StatID:(DE-HGF)0199
|2 StatID
|b Clarivate Analytics Master Journal List
|d 2021-02-02
920 1 _ |0 I:(DE-H253)Z_THAT-20210408
|k Z_THAT
|l Theoretische Astroteilchenphysik
|x 0
920 1 _ |0 I:(DE-H253)ZEU-ICE-20160806
|k ZEU-ICE
|l Neutrinoteleskop
|x 1
920 1 _ |0 I:(DE-H253)Z_NA-20210408
|k Z_NA
|l Neutrinoastronomie / Kosmologie
|x 2
980 _ _ |a journal
980 _ _ |a VDB
980 _ _ |a UNRESTRICTED
980 _ _ |a I:(DE-H253)Z_THAT-20210408
980 _ _ |a I:(DE-H253)ZEU-ICE-20160806
980 _ _ |a I:(DE-H253)Z_NA-20210408
980 _ _ |a APC
980 1 _ |a APC
980 1 _ |a FullTexts

LibraryCollectionCLSMajorCLSMinorLanguageAuthor
Marc 21