Neutron Backgrounds in Dark Maer Experiments · Measurement and Analysis of WIMP Detecon...
Transcript of Neutron Backgrounds in Dark Maer Experiments · Measurement and Analysis of WIMP Detecon...
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NeutronBackgroundsinDarkMa3erExperiments
AndreasBiekertPhysics290E
October26,2016
Background:h3ps://upload.wikimedia.org/wikipedia
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• Electronrecoil(ER)eventshavemuchlargercountratethannuclearrecoil(NR)events.
• PossibletodiscriminatebetweenERandNR.
• NeutronNReventscanmimicWIMPsignal.
BackgroundsandSignalDiscriminaPon
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BlueeventsfromERcalibraPon(133Ba)andGreeneventsfromNRcalibraPon(252Cf)inCDMSZIPdetector.From[1]
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UnderstandingNeutronBackgroundsinExperiments
• Neutronbackgroundscanbeverysite,detector,andenvironmentspecific.
• Canbedifficulttomeasureaccurately.• UnderstandingcomesfromcarefulconsideraPonof:– Theory(relevantsources,distribuPons,etc.)– SimulaPon(commonlywithGEANTand/orFLUKA)– Measurements(ratecounPng)
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MainSourcesofNeutrons
• Lowenergyneutronsfrom(α,n)reacPonsandspontaneousfissioninsurroundingrockanddetectorcomponents
• HighenergyneutronsfrommuoninteracPonsinsurroundingrockanddetectorcomponents
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(α,n)reacPons
• 238U,235U,and232Thdecaychainsproduceα’s.
• Differentisotopeshavedifferentenergycutoffsfor(α,n)reacPons
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238U:From:h3ps://upload.wikimedia.org/wikipedia/
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(α,n)reacPons
• 238U,235U,and232Thdecaychainsproduceα’s.
• Differentisotopeshavedifferentenergycutoffsfor(α,n)reacPons
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235U:From:h3ps://upload.wikimedia.org/wikipedia/
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(α,n)reacPons
• 238U,235U,and232Thdecaychainsproduceα’s.
• Differentisotopeshavedifferentenergycutoffsfor(α,n)reacPons
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232Th:From:h3ps://upload.wikimedia.org/wikipedia/
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DecayChainRelevancetoNeutronBackgrounds
From[2]
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CRESSTGranSassoNeutronBackgroundAnalysis(From[2])
• ExperimentmovedfromHallAtoHallCbetweengeneraPons.
• Prompteddetailedneutronbackgroundstudy.
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Right:h3p://www.nature.com/polopoly_fs/7.4565.1337781034!/image/gran-sasso-graphic-on-page.jpg_gen/derivaPves/landscape_630/gran-sasso-graphic-on-page.jpgLek:h3ps://www.mppmu.mpg.de/english/cresst_image4.gif
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CRESSTGranSasso(α,n)SimulaPons
• BackgroundratesspecifictorockfoundaroundHallAatGranSasso• ContribuPonlevelsoffaker~1mofrock/concrete
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SpontaneousFission
• Nucleusdecaysintotwodaughternucleiand2-3neutrons.
• Possibleinprincipleforourfriends238U,235U,and232Th.
• InpracPce,onlyappreciablecontribuPonisfrom238U.
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CRESSTGranSassoTotalNeutronFluxComparison
• CarefulsimulaPonscanreproduceexperimentaldata(measurementperformedinhallA)
• SignificanceofwatercontenttoneutronfluxraisesquesPonsaboutannualmodulaPonofsignalseenbyDAMA– DAMA’ssignalpersistsandnotconclusivelyexplained
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PassiveShielding
• Usuallymadeof:– Wax– Hydrocarbon(Polyethylene,scinPllator,etc.)
– Water• A3enuatesneutronfluxfromexternalsources.
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EffectofwaxshieldingaroundearlyCDMSexperimentatStanfordUndergroundFacility.Leadshielddesignedtoreduceϒfluxindetector.From[3]
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CDMSStanfordUndergroundFacilityNeutronBackgroundAnalysis
• Imagesfrom[4]• Experiment(CDMSI)conductedatmuchshallowerdepth.• BackgroundanalysisonneutronsoriginaPngfrommuon
interacPons.
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NeutronproducPonprocessesbymuons
• Muoncapturefollowedbyneutronemission.Fallsoffaker300meterwaterequivalent
• DirectmuonspallaPonejectsneutron
• NeutronsproducPonbyhadronsfrommuon-generatednuclearshowers
• Neutronsproducedbygammasinmuon-generatedelectromagnePcshowers
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MuonInteracPonsinDetectorComponents
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• Passiveshieldingworksonneutronsgeneratedbymuonsexternaltothedetector(forthemostpart).
• MuonscangenerateneutronsinsidedetectorbyinteracPngwithdetectorcomponents.
Leadshielding: CopperCrysotat:Plotsfrom[3]
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MuonInteracPonsinDetectorComponents
• PlotshowsneutronfluxresulPngfromdifferentmuoninteracPonprocesses(280GeVmuons).
• DifferentdetectorcomponentshavedifferentsensiPviPes.
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From[5]
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AcPveVetoLayer• Modernexperimentshave
vetolayersaroundexperiments.– LUXusedwaterwithPMTsthatmonitorforCherenkovradiaPonfrommuons.
– CDMSIIusedplasPcscinPllatorforsimilarpurpose
• Vetolayerscanalsodetectsomehighenergy(“punch-through”)neutronsfromexternalmuoninteracPons
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Lek:LUXwatershield.From[6]
Right:CDMSIIplasPcscinPllatorveto.From[1]
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AddiPonalStrategies
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• VetoingNReventswithmulPplesca3eringsinthedetector– WIMPsnotlikelytomulPplesca3erinthedetector
• VetoingNReventswithaccompanyingERevents– ThesearetheresultofneutrondeepinelasPcsca3ering
• Cleanerandcleanerdetectormaterials
SimulaPonofneutronsca3eringmulPplicityinagenericliquidxenondetectordeepunderground.From[7]
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LUXNeutronBackgrounds[8]• Neutronsourcesarepreviouslydiscussed(α,n)andspontaneousfissionprocessesoccurringin:– PMTs– AccumulaPonof210Pbdaughtersondetectorsurfaces(negligible)
– Cryostats(30%ofbaselinePMTesPmate)• Punch-throughneutronsfrommuoninteracPonsinrock(30%ofbaselinePMTesPmate)
• FinalesPmatetranslatesto3x10-4NReventsperdaypassingallcuts
• NReventssubdominantbackground
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CDMSIINeutronBackground[1]
• Unvetoedmuon-inducedNReventsforrun– 0.214±0.0081(stat.)±0.0086(syst.)forGedetectors– 0.129±0.0058(stat.)±0.0033(syst.)forSidetectors
• Detectorcomponent-generatedneutroneventsforrunalsomuchlessthan1.
• NRbackgroundenPrelysubdominant.
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NewExperiment–NuclearEmulsion(From[9])
• Authorsassumepassivescreeningtechniquesforexternallygeneratedneutrons.
• DetailedcalculaPons,simulaPons,andacPvitymeasurementstoesPmateintrinsicneutronbackground
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References[1]S.M.Fallows.MeasurementofNuclearRecoilsintheCDMSIIDarkMa8erSearch.PhDthesis,UniversityofMinnesota,December2014.[2]H.R.T.Wulandari.StudyOnNeutron-InducedBackgroundintheDarkMa8erExperimentCRESST.PhDthesis,InsPtutfürAstro-TeilchenphysikderTechnischenUniversitätMünchen,July2003.[3]A.D.Silva,etal.Neutronbackgroundforadarkma3erexperimentatashallowdepthsite.NuclearInstrumentsandMethodsinPhysicsResearchA,354:553–559,August1995.[4]T.Perera.TheLimiDngBackgroundinaDarkMa8erSearchatShallowDepth.PhDthesis,CaseWesternReserveUniversity,January2002.[5]H.M.Araùjo,etal.Muon-inducedneutronproducPonanddetecPonwithGEANT4andFLUKA.NuclearInstrumentsandMethodsinPhysicsResearchSecPonA:Accelerators,Spectrometers,DetectorsandAssociatedEquipment,545(1-2):398–411,June2005.[6]S.Fiorucci.TheLUXdarkma3ersearch.DarknessVisible:DarkMa3erinAstrophysicsandParPclePhysics,August2010.[7]M.J.Carson,etal.Neutronbackgroundinlarge-scalexenondetectorsfordarkma3ersearches.AstroparPclePhysics,21(6):667–687,Sep2004.[8]D.C.Malling.MeasurementandAnalysisofWIMPDetecDonBackgrounds,andCharacterizaDonandPerformanceoftheLargeUndergroundXenonDarkMa8erSearchExperiment.PhDthesis,BrownUniversity,May2014.[9]A.Alexandrov,etal.IntrinsicneutronbackgroundofnuclearemulsionsfordirecPonaldarkma3ersearches.arXiv,June2016.
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OtherSourcesP.Sorensen.SensiPvityandbackgroundsoftheluxdarkma3ersearch.APSAprilMeePng,2008.T.Classen.TheLUXWIMPdetector.24thPacificCoastGravityMeePng,March2008.K.Ni.DevelopmentofaLiquidXenonTimeProjecDonChamberfortheXENONDarkMa8erSearch.PhDthesis,ColumbiaUniversity,2006.M.J.Carson,etal.Vetoperformanceforlarge-scalexenondarkma3erdetectors.NuclearInstrumentsandMeth-odsinPhysicsResearchSecPonA:Accelerators,Spectrometers,DetectorsandAssociatedEquipment,548(3):418–426,August2005.
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