Table Of ContentUvA-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].
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Download date:06 Feb 2023
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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
Description: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