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2022-10-14Zeitschriftenartikel DOI: 10.18452/26423
Searching for High-energy Neutrino Emission from Galaxy Clusters with IceCube
dc.contributor.authorAbbasi, R.
dc.contributor.authorAckermann, M.
dc.contributor.authorAdams, J.
dc.contributor.authorAguilar, J. A.
dc.contributor.authorAhlers, M.
dc.contributor.authorAhrens, M.
dc.contributor.authorAlameddine, J. M.
dc.contributor.authorAlves, A. A.
dc.contributor.authorAmin, N. M.
dc.contributor.authorAndeen, K.
dc.contributor.authorAnderson, T.
dc.contributor.authorAnton, G.
dc.contributor.authorArgüelles, C.
dc.contributor.authorAshida, Y.
dc.contributor.authorAthanasiadou, S.
dc.contributor.authorAxani, S.
dc.contributor.authorBai, X.
dc.contributor.authorV., A. Balagopal
dc.contributor.authorBaricevic, M.
dc.contributor.authorBarwick, S. W.
dc.contributor.authorBasu, V.
dc.contributor.authorBay, R.
dc.contributor.authorBeatty, J. J.
dc.contributor.authorBecker, K.-H.
dc.contributor.authorTjus, J. Becker
dc.contributor.authorBeise, J.
dc.contributor.authorBellenghi, C.
dc.contributor.authorBenda, S.
dc.contributor.authorBenZvi, S.
dc.contributor.authorBerley, D.
dc.contributor.authorBernardini, E.
dc.contributor.authorBorowka, J.
dc.contributor.authorBöser, S.
dc.contributor.authorBotner, O.
dc.contributor.authorBöttcher, J.
dc.contributor.authorBourbeau, E.
dc.contributor.authorBradascio, F.
dc.contributor.authorBraun, J.
dc.contributor.authorBrinson, B.
dc.contributor.authorBron, S.
dc.contributor.authorBrostean-Kaiser, J.
dc.contributor.authorBurley, R. T.
dc.contributor.authorBusse, R. S.
dc.contributor.authorCampana, M. A.
dc.contributor.authorCarnie-Bronca, E. G.
dc.contributor.authorChen, C.
dc.contributor.authorChen, Z.
dc.contributor.authorChirkin, D.
dc.contributor.authorChoi, K.
dc.contributor.authorClark, B. A.
dc.contributor.authorClark, K.
dc.contributor.authorClassen, L.
dc.contributor.authorColeman, A.
dc.contributor.authorCollin, G. H.
dc.contributor.authorConnolly, A.
dc.contributor.authorConrad, J. M.
dc.contributor.authorCoppin, P.
dc.contributor.authorCorrea, P.
dc.contributor.authorCowen, D. F.
dc.contributor.authorGallagher, J.
dc.contributor.authorGanster, E.
dc.contributor.authorGarcia, A.
dc.contributor.authorGarrappa, S.
dc.contributor.authorGerhardt, L.
dc.contributor.authorGhadimi, A.
dc.contributor.authorGlaser, C.
dc.contributor.authorGlauch, T.
dc.contributor.authorGlüsenkamp, T.
dc.contributor.authorGoehlke, N.
dc.contributor.authorGonzalez, J. G.
dc.contributor.authorGoswami, S.
dc.contributor.authorGrant, D.
dc.contributor.authorGrégoire, T.
dc.contributor.authorGriswold, S.
dc.contributor.authorGünther, C.
dc.contributor.authorGutjahr, P.
dc.contributor.authorHaack, C.
dc.contributor.authorHallgren, A.
dc.contributor.authorHalliday, R.
dc.contributor.authorHalve, L.
dc.contributor.authorHalzen, F.
dc.contributor.authorHamdaoui, H.
dc.contributor.authorMinh, M. Ha
dc.contributor.authorHanson, K.
dc.contributor.authorHardin, J.
dc.contributor.authorHarnisch, A. A.
dc.contributor.authorHaungs, A.
dc.contributor.authorHelbing, K.
dc.contributor.authorHellrung, J.
dc.contributor.authorHenningsen, F.
dc.contributor.authorHettinger, E. C.
dc.contributor.authorHeuermann, L.
dc.contributor.authorHickford, S.
dc.contributor.authorHignight, J.
dc.contributor.authorHill, C.
dc.contributor.authorHill, G. C.
dc.contributor.authorWiebusch, C. H.
dc.contributor.authorWilley, N.
dc.contributor.authorWilliams, D. R.
dc.contributor.authorWolf, M.
dc.date.accessioned2023-04-21T09:58:14Z
dc.date.available2023-04-21T09:58:14Z
dc.date.issued2022-10-14none
dc.date.updated2022-10-19T02:43:36Z
dc.identifier.issn2041-8205
dc.identifier.urihttp://edoc.hu-berlin.de/18452/27103
dc.description.abstractGalaxy clusters have the potential to accelerate cosmic rays (CRs) to ultrahigh energies via accretion shocks or embedded CR acceleration sites. The CRs with energies below the Hillas condition will be confined within the cluster and eventually interact with the intracluster medium gas to produce secondary neutrinos and gamma rays. Using 9.5 yr of muon neutrino track events from the IceCube Neutrino Observatory, we report the results of a stacking analysis of 1094 galaxy clusters with masses ≳1014 M ⊙ and redshifts between 0.01 and ∼1 detected by the Planck mission via the Sunyaev–Zel’dovich effect. We find no evidence for significant neutrino emission and report upper limits on the cumulative unresolved neutrino flux from massive galaxy clusters after accounting for the completeness of the catalog up to a redshift of 2, assuming three different weighting scenarios for the stacking and three different power-law spectra. Weighting the sources according to mass and distance, we set upper limits at a 90% confidence level that constrain the flux of neutrinos from massive galaxy clusters (≳1014 M ⊙) to be no more than 4.6% of the diffuse IceCube observations at 100 TeV, assuming an unbroken E −2.5 power-law spectrum.eng
dc.description.sponsorshipNational Science Foundation (NSF)https://doi.org/10.13039/100000001
dc.language.isoengnone
dc.publisherHumboldt-Universität zu Berlin
dc.rights(CC BY 4.0) Attribution 4.0 Internationalger
dc.rights.urihttps://creativecommons.org/licenses/by/4.0/
dc.subjectNeutrino astronomyeng
dc.subjectHigh-redshift galaxy clusterseng
dc.subject.ddc520 Astronomie und zugeordnete Wissenschaftennone
dc.titleSearching for High-energy Neutrino Emission from Galaxy Clusters with IceCubenone
dc.typearticle
dc.identifier.urnurn:nbn:de:kobv:11-110-18452/27103-2
dc.identifier.doihttp://dx.doi.org/10.18452/26423
dc.type.versionpublishedVersionnone
local.edoc.pages10none
local.edoc.type-nameZeitschriftenartikel
local.edoc.container-typeperiodical
local.edoc.container-type-nameZeitschrift
dc.description.versionPeer Reviewednone
dc.identifier.eissn2041-8213
dcterms.bibliographicCitation.doi10.3847/2041-8213/ac966bnone
dcterms.bibliographicCitation.journaltitleThe astrophysical journalnone
dcterms.bibliographicCitation.volume938none
dcterms.bibliographicCitation.issue2none
dcterms.bibliographicCitation.articlenumberL11none
dcterms.bibliographicCitation.originalpublishernameInstitute of Physics Publ.none
dcterms.bibliographicCitation.originalpublisherplaceLondonnone
bua.departmentMathematisch-Naturwissenschaftliche Fakultätnone

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