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Light at the end of the shower: An all-flavour neutrino point-source search with the ANTA PDF

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UvA-DARE (Digital Academic Repository) Light at the end of the shower: An all-flavour neutrino point-source search with the ANTARES neutrino telescope Michael, T. Publication date 2016 Document Version Final published version Link to publication Citation for published version (APA): Michael, T. (2016). Light at the end of the shower: An all-flavour neutrino point-source search with the ANTARES neutrino telescope. [Thesis, fully internal, Universiteit van Amsterdam]. General rights It is not permitted to download or to forward/distribute the text or part of it without the consent of the author(s) and/or copyright holder(s), other than for strictly personal, individual use, unless the work is under an open content license (like Creative Commons). Disclaimer/Complaints regulations If you believe that digital publication of certain material infringes any of your rights or (privacy) interests, please let the Library know, stating your reasons. In case of a legitimate complaint, the Library will make the material inaccessible and/or remove it from the website. Please Ask the Library: https://uba.uva.nl/en/contact, or a letter to: Library of the University of Amsterdam, Secretariat, Singel 425, 1012 WP Amsterdam, The Netherlands. You will be contacted as soon as possible. UvA-DARE is a service provided by the library of the University of Amsterdam (https://dare.uva.nl) Download date:06 Feb 2023 L i g Invitation h t a to attend the t t Tino Michael public defence of h e my PhD dissertation E Light at the End of the Shower n d o f An all-flavour Neutrino Point-Source Search Light at t h e with the ANTARES Neutrino Telescope the End of S h o w the Shower e r Friday, 13. May 2016 at 10:00 in the Agnietenkapel T i n o M i c h a e l Tino Michael Light at the End of the Shower An all-flavour Neutrino Point-Source Search with the ANTARES Neutrino Telescope Light at the End of the Shower An all-flavour Neutrino Point-Source Search with the ANTARES Neutrino Telescope ACADEMISCH PROEFSCHRIFT terverkrijgingvandegraadvandoctor aandeUniversiteitvanAmsterdam opgezagvandeRectorMagnificus prof. dr. D.C.vandenBoom tenoverstaanvaneendoorhetCollege voorPromotiesingesteldecommissie, inhetopenbaarteverdedigenindeAgnietenkapel opvrijdag13mei2016,te10:00uur door Tino Michael geborenteCottbus,Duitsland Promotiecommissie Promotor: prof. dr. P.M.Kooijman UniversiteitvanAmsterdam Copromotor: dr. A.J.Heijboer Nikhef Overigeleden: prof. dr. ir. E.N.Koffeman UniversiteitvanAmsterdam dr. R.Bruijn UniversiteitvanAmsterdam prof. dr. F.L.Linde UniversiteitvanAmsterdam prof. dr. ir. P.J.deJong UniversiteitvanAmsterdam dr. D.F.E.Samtleben UniversiteitLeiden prof. dr. ing. B.vanEijk UniversiteitTwente dr. C.Finley StockholmUniversity FaculteitderNatuurwetenschappen,WiskundeenInformatica TinoMichael2016,CC-BY-SA LightattheEndoftheShower SetinLatexusingLinuxLibertine CoverImage: Toulonbeachduringsunsettaken2013bytheauthorduringanon-siteshift. TheworkdescribedinthisthesisispartoftheresearchprogramoftheSticht- ingvoorFundamenteelonderzoekderMaterie(FOM),whichispartoftheNed- erlandseorganisatievoorWetenschappelijkOnderzoek (NWO). Theresearchwasfundedbythevidiproject“ExploringtheCosmoswithNeu- trinos”grantedtoA.J.HeijboerandwascarriedoutattheNationaalInstituut voorSubatomaireFysica(Nikhef)inAmsterdam,theNetherlands. Contents 1 Introduction 1 2 NeutrinoAstronomy 5 2.1 NeutrinosandtheStandardModel . . . . . . . . . . . . . . . . 5 2.2 CosmicRays . . . . . . . . . . . . . . . . . . . . . . . . . . . . 6 2.2.1 CosmicParticleAcceleration . . . . . . . . . . . . . . 7 2.2.2 GalacticAccelerators . . . . . . . . . . . . . . . . . . . 8 2.2.3 ExtragalacticAccelerators . . . . . . . . . . . . . . . . 10 2.2.4 TheGZK-Cutoff . . . . . . . . . . . . . . . . . . . . . . 11 2.3 NeutrinoProductionatAstrophysicalAccelerationSites . . . 11 2.3.1 NeutrinoOscillationanditsImplications . . . . . . . . 13 2.3.2 TheIceCubeSignal . . . . . . . . . . . . . . . . . . . . 14 3 TheANTARESExperiment 17 3.1 DetectionPrinciple . . . . . . . . . . . . . . . . . . . . . . . . 17 3.1.1 NeutrinoInteractions . . . . . . . . . . . . . . . . . . . 18 3.1.2 CherenkovRadiation . . . . . . . . . . . . . . . . . . . 22 3.2 TheANTARESDetector . . . . . . . . . . . . . . . . . . . . . 22 3.2.1 DetectorLayout . . . . . . . . . . . . . . . . . . . . . . 23 3.2.2 DataAcquisition . . . . . . . . . . . . . . . . . . . . . 26 3.2.3 Trigger . . . . . . . . . . . . . . . . . . . . . . . . . . . 26 3.2.4 Calibration . . . . . . . . . . . . . . . . . . . . . . . . 27 3.2.5 Background . . . . . . . . . . . . . . . . . . . . . . . . 29 3.2.6 Visibility . . . . . . . . . . . . . . . . . . . . . . . . . . 31 3.3 Simulation . . . . . . . . . . . . . . . . . . . . . . . . . . . . . 31 3.3.1 EventGeneration . . . . . . . . . . . . . . . . . . . . . 32 3.3.2 PhotonTracking . . . . . . . . . . . . . . . . . . . . . 33 3.3.3 DetectorResponse . . . . . . . . . . . . . . . . . . . . 33 3.4 MuonTrackReconstruction . . . . . . . . . . . . . . . . . . . 34 4 OutlookonKM3NeT 39 4.1 TheKM3NeTNeutrinoObservatory . . . . . . . . . . . . . . . 39 i 4.2 ThePPM-DOM . . . . . . . . . . . . . . . . . . . . . . . . . . 40 4.2.1 FirstDeep-SeaRuns . . . . . . . . . . . . . . . . . . . 40 4.2.2 AtmosphericMuons . . . . . . . . . . . . . . . . . . . 46 5 AShowerReconstructionforANTARES 51 5.1 ShowerEventTopology . . . . . . . . . . . . . . . . . . . . . . 51 5.2 PositionReconstruction . . . . . . . . . . . . . . . . . . . . . . 53 5.3 DirectionReconstruction . . . . . . . . . . . . . . . . . . . . . 56 5.3.1 TheSignalTerm . . . . . . . . . . . . . . . . . . . . . 58 5.3.2 Thenon-hitTerm . . . . . . . . . . . . . . . . . . . . . 58 5.3.3 TheBackgroundTerm . . . . . . . . . . . . . . . . . . 59 5.3.4 Implementation . . . . . . . . . . . . . . . . . . . . . . 60 5.3.5 ErrorEstimator . . . . . . . . . . . . . . . . . . . . . . 60 5.4 Performance . . . . . . . . . . . . . . . . . . . . . . . . . . . . 61 5.4.1 Position . . . . . . . . . . . . . . . . . . . . . . . . . . 61 5.4.2 Direction . . . . . . . . . . . . . . . . . . . . . . . . . 63 5.4.3 Energy . . . . . . . . . . . . . . . . . . . . . . . . . . . 63 5.4.4 AngularResolutionmeasuredinData . . . . . . . . . 63 6 EventSelection 67 6.1 RunSelection . . . . . . . . . . . . . . . . . . . . . . . . . . . 67 6.2 SelectionofMuonTracks . . . . . . . . . . . . . . . . . . . . . 69 6.3 SelectionofShowerEvents . . . . . . . . . . . . . . . . . . . . 69 6.4 Data/MonteCarloComparison . . . . . . . . . . . . . . . . . 73 7 Point-SourceSearch 77 7.1 Likelihood-Functions . . . . . . . . . . . . . . . . . . . . . . . 77 7.2 SearchMethod . . . . . . . . . . . . . . . . . . . . . . . . . . . 79 7.2.1 Acceptance . . . . . . . . . . . . . . . . . . . . . . . . 79 7.2.2 PointSpreadFunction . . . . . . . . . . . . . . . . . . 82 7.2.3 BackgroundRate . . . . . . . . . . . . . . . . . . . . . 83 7.2.4 NumberofselectedHits . . . . . . . . . . . . . . . . . 83 7.2.5 ImplementationoftheLikelihoodFunction . . . . . . 83 7.3 PseudoExperiments . . . . . . . . . . . . . . . . . . . . . . . . 85 7.3.1 AbsolutePointingAccuracy . . . . . . . . . . . . . . . 86 7.3.2 AngularResolutionUncertainty . . . . . . . . . . . . . 86 7.3.3 AcceptanceUncertainty . . . . . . . . . . . . . . . . . 87 7.3.4 BackgroundUncertainty . . . . . . . . . . . . . . . . . 88 7.4 DiscoveryPotentialandSensitivity . . . . . . . . . . . . . . . 88 7.4.1 FullSkySearch . . . . . . . . . . . . . . . . . . . . . . 89 ii 7.4.2 CandidateListSearch . . . . . . . . . . . . . . . . . . 90 7.4.3 SearcharoundtheGalacticCentre . . . . . . . . . . . 91 8 Results 93 8.1 FullSkySearch. . . . . . . . . . . . . . . . . . . . . . . . . . . 93 8.2 CandidateList . . . . . . . . . . . . . . . . . . . . . . . . . . . 98 8.3 TheGalacticCentre . . . . . . . . . . . . . . . . . . . . . . . . 102 Summary 107 Samenvatting 113 Zusammenfassung 119 Acknowledgements 125 iii

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The ultimate purpose of the monument is still a mystery but it has been pro- posed that many . The ANTARES detector is the largest deep sea neutrino observatory to date. One advantage of by the detector's sensor modules. the blue and UV range where water is also most transmissive. 3.2 The
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