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Search for ultrarelativistic magnetic monopoles with the Pierre Auger observatory

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    SYSNO ASEP0468802
    Document TypeJ - Journal Article
    R&D Document TypeJournal Article
    Subsidiary JČlánek ve WOS
    TitleSearch for ultrarelativistic magnetic monopoles with the Pierre Auger observatory
    Author(s) Aab, A. (DE)
    Abreu, A. (PT)
    Aglietta, M. (IT)
    Blažek, Jiří (FZU-D) ORCID, RID
    Boháčová, Martina (FZU-D) RID, ORCID
    Chudoba, Jiří (FZU-D) RID, ORCID
    Ebr, Jan (FZU-D) RID, ORCID
    Mandát, Dušan (FZU-D) RID, ORCID
    Palatka, Miroslav (FZU-D) RID, ORCID, SAI
    Pech, Miroslav (FZU-D) RID, ORCID
    Prouza, Michael (FZU-D) RID, ORCID
    Řídký, Jan (FZU-D) RID, ORCID
    Schovánek, Petr (FZU-D) RID, ORCID
    Trávníček, Petr (FZU-D) RID, ORCID
    Vícha, Jakub (FZU-D) RID, ORCID
    Number of authors413
    Article number082002
    Source TitlePhysical Review D. - : American Physical Society - ISSN 2470-0010
    Roč. 94, č. 8 (2016), s. 1-12
    Number of pages12 s.
    Languageeng - English
    CountryUS - United States
    KeywordsPierre Auger Observatory ; detector ; cosmic rays
    Subject RIVBF - Elementary Particles and High Energy Physics
    OECD categoryParticles and field physics
    R&D ProjectsLG15014 GA MŠMT - Ministry of Education, Youth and Sports (MEYS)
    GA14-17501S GA ČR - Czech Science Foundation (CSF)
    Research InfrastructureAUGER-CZ - 90038 - Fyzikální ústav AV ČR, v. v. i.
    Method of publishingLimited access
    Institutional supportFZU-D - RVO:68378271
    UT WOS000384474700002
    EID SCOPUS84994423094
    DOI10.1103/PhysRevD.94.082002
    AnnotationWe present a search for ultrarelativistic magnetic monopoles with the Pierre Auger observatory. Such particles, possibly a relic of phase transitions in the early Universe, would deposit a large amount of energy along their path through the atmosphere, comparable to that of ultrahigh-energy cosmic rays (UHECRs). The air-shower profile of a magnetic monopole can be effectively distinguished by the fluorescence detector from that of standard UHECRs. No candidate was found in the data collected between 2004 and 2012, with an expected background of less than 0.1 event from UHECRs. The corresponding 90% confidence level (C.L.) upper limits on the flux of ultrarelativistic magnetic monopoles range from 10(-1)9 (cm(2) sr s)(-1) for a Lorentz factor gamma = 10(9) to 2.5 x 10(-21) (cm(2) sr s)(-1) for gamma = 10(12). These results-the first obtained with a UHECR detector-improve previously published limits by up to an order of magnitude.
    WorkplaceInstitute of Physics
    ContactKristina Potocká, potocka@fzu.cz, Tel.: 220 318 579
    Year of Publishing2021
    Electronic addresshttps://doi.org/10.1103/PhysRevD.94.082002
Number of the records: 1  

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