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ParticleDetectionHowtoseetheinvisible

RobertHarr

WhatIsDetection?• Howcanwe“see”asubatomicparticle?

o Byitsinteractionswithordinarymatter.

• Whatkindofinteractionsdoesasubatomicparticlehavewithordinarymatter?o Ordinarymatteriscomposedofatoms.Interactionscanoccurwiththe:• bulkmaterial,• molecularbonds,• atomicelectrons,and• nuclei.

o Theatomicpictureisveryuseful!13 May 2016 R. Harr 2

AGeneralPurposeDetector

13 May 2016 R. Harr 3

Detection• Requirescreatingameasurablesignal:

o somethingthatcanbeseenbyeyeo anelectricsignalthatcanberegisteredo achemicalchangetosomethingthatcanbemadevisibleafterachemicalreaction

• Wenormallyconsiderthedetectormaterialtobeatresto incidentparticleonfixedtargetgeometry

13 May 2016 R. Harr 4

WheretoBegin?• Somanypossibledetectormaterials:o gas,liquid,solido atomicormolecularo HtoU

• Andsomanypossiblesignals:o heat,light,electric

• Canwesimplifythis?

13 May 2016 R. Harr 5

• Therearehundredsofparticles:o leptons,quarkso bosons:γ,W,Z,Ho combinationsofquarks:mesonsandbaryons

o deuterons,alphas,...o newparticles:axions,SUSY,darkmatter,...

• Canwewinnowthislistdown?

WhichParticles?• Whichparticlesaredirectlydetectable?

o Thosethatlivelongenoughtotraversedetectormaterial

• Enumeratethem(it’sasmallnumber):o photonγo electronandpositrone±

o muonandanti-muonµ±

o chargedpions π±

o chargedkaons K±

o protonandanti-protonp±

o neutronsn andanti-neutronsn,andneutralkaon K0

o afewofthestrangebaryons,inspecialcaseso somespeculativeparticleslikedarkmatterormag.monopoles

13 May 2016 R. Harr 6

hadrons

WhatAboutOtherParticles?• Detectionofallotherparticlesisviatheirdecayproducts,forexample:o K0Sà π+π−

o D+(s) à φ π+ à K+K-π+ (seeplot)

o Z0 à e+e-,µ+µ-,bb• b quarksareseenasjetswithadisplacedvertex• jetsareacollectionofdetectableparticlesinanarrowcone

oW± à e±νe ,µ±νµ• neutrinosaren’tseensomuchasinferredfromanimbalanceofmomentumperpendiculartothecollisionaxisreferredtoasmissingtransverseenergyorMET.

13 May 2016 R. Harr 7

WhatCanBeMeasured?• Firstistodetectthataparticleispresent.

o Forlowenergyphotons,darkmatter,and[lowenergy]neutrinos,thatisaboutallthatcanbemeasured

• Forotherparticleswewouldliketoknow:o chargeo typeofparticle(mass)o energyandmomentumo spin(?!)

• Thesearedeterminedfromthewayparticlesinteractwithamacroscopicdetector(matter).

13 May 2016 R. Harr 8

TheInteractions• Thebasicinteractionscanbefurthersubdividedintoasurprisinglyshortlist.

• Iwillnotdiscussinteractionsthateffectmolecularbonds.o Thesearenotusedinelectronicdetectorssincechemicalprocessingisneeded(uptonow).

o Thesecomeintoplaywithphotographicemulsionsandsometypesofplasticdetectors.

o Otherfamousexample:RayDavis’solarneutrinoexpt.o Consultreferencesifyouneedmoreinformation.

13 May 2016 R. Harr 9

Interactions(cont’d)1. Interactionswith(orrequiring)atomicnuclei-

- maybefamiliarfrommodernphysicscourses:

a) Pairproductionb) Bremstrahlungc) Nuclear(hadronic)interaction

• Thefirstappliestophotons,thesecondtoelectrons(mostly),andthelasttohadrons.

13 May 2016 R. Harr 10

Interactions(cont’d)2. Interactionswithatomicelectronsarewidely

used:a) ComptonScatteringb) Photoelectriceffectc) Ionizationofatomsd) Excitationofatoms

• Thefirsttwoapplyonlytophotons,thelasttwoapplytoallparticles.

13 May 2016 R. Harr 11

Interactions(cont’d)3. Interactionswithbulkmaterialmaybethe

leastfamiliar:a) Cerenkovradiationb) Transitionradiation

• Iwillnotbeabletocoverthesetoday.o Checkthebackupslidesforsomeinformationonthese.o AgoodintroductioncanbefoundinJackson’sClassicalElectrodynamics.

13 May 2016 R. Harr 12

ThePhysicsofDetection

13 May 2016 R. Harr 13

14

InteractionswithElectrons• Interactionswithatomicelectronsmaybethesinglemostimportantdetectionprocessforparticleexperiments.o Primaryprocessfor“tracking” particleso Alsoimportantforproducinglargenumbersoffreeelectronsforadetectablecurrent.

13 May 2016 R. Harr 14

15

ThePhotoelectricEffectFamiliarfromModernPhysicsclass.Einstein’sexplanationrequiresquantizedenergyforphotons.

Energyofliberatedelectronsdependsonthefrequencyoflight(photons).

Rateofelectrons(current)dependsontheintensityofthelight(rateofincidentphotons).

Photomultipliertubesusethephotoelectriceffecttoconvertincomingphotonstoelectrons(singlephotondetection).Silicondetectors(strips,pixels,CCD’s)usethephotoelectriceffecttocreateanelectron-holepair.13 May 2016 R. Harr 15

16

ComptonScatteringAsecondtypeofphoton-matterinteraction.Usuallyappearswhendiscussingrelativity.

Importantforintermediateenergyphotons.

Incidentphotonlosesenergywhenejectinganelectronfromanatom.

Processisimportantto“breakdown” ahighenergyphotonintoelectrons.Theenergyofthephotondeterminesthefinalnumberofelectronsproduced.(Seecalorimetry)

13 May 2016 R. Harr 16

The Bethe-BlochFormula• Semi-classicalcalculationofenergyloss

• Notethecompetitionbetweenln(β2γ2)and–β2o Causesaminimumintheenergylosso MinimumenergylossscalesroughlyasZ/Aofthematerial.

• 4MeVcm2/gforHtoabout1MeVcm2/gforheavyelementso Minimumenergylosswhenβγ ≈3to3.5o Dependsonkinematics,independentofparticletype

• δ termrepresentsdensityeffect13 May 2016 R. Harr 17

�dE

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2

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A

1

b2

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2

ln

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c

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18

Energy Loss

13 May 2016 R. Harr 18

DependenceonMaterialEnergylossdependsonthetypeofmaterialandparticle.AtomswithhigherZhavelessenergylossperg/cm2

Buttheirhigherdensity(g/cm3)morethanmakesupforthis.

13 May 2016 R. Harr 19

ScintillationManymaterialsemitlightwhenatomsormoleculesareexcitedbyachargedparticlepassingnearbyEmittedlightiscalledscintillationScintillatingmediumusuallytransparentLight(onetoa fewphotons)detectedbyaphotomultiplier

13 May 2016 R. Harr 20

InteractionswithNuclei• Twotypesofinteractionarepossible

o Electromagnetico Strong

• Detailsareinthebackupslides

13 May 2016 R. Harr 21

(1)Electromagnetic• Mostlysinglephotonexchange

o elasticinteractions

• Whenalightobject(particle)scatterselasticallyfromaheavyobject(nucleus):o littlelossofenergyo canchangedirectionsignificantly

• thinkoftheRutherfordscatteringexperiment• mostscatteringissmallangle• largenumberofsmallanglescatterscanbetreatedstatistically

13 May 2016 R. Harr 22

23

PairProductionAthirdtypeofphoton-matterinteraction.Exampleofconversionofenergyintomass.

Importantforhighenergyphotons.

Incidentphotonconvertsintoanelectron-positronpair.

Processisimportantto“breakdown” ahighenergyphotonintoelectrons.Theenergyofthephotondeterminesthefinalnumberofelectronsproduced.(Seecalorimetry.)

Presenceofmatterisrequiredtoconserveenergy-momentum.

13 May 2016 R. Harr 23

24

BremstrahlungAGermanwordfor“brakingradiation”.

Importantforhighenergyelectrons.

Incidentelectronemitsaphoton(usuallyx-ray),whenacceleratedintheelectricfieldofanucleus.

Processisimportantto“breakdown” ahighenergyelectronintolowenergyelectrons.Theenergyoftheincidentelectrondeterminesthefinalnumberofelectronsproduced.(Seecalorimetry.)

13 May 2016 R. Harr 24

25

SynchrotronRadiationLikeBremstrahlung,butaccelerationduetoa

magneticfield.

13 May 2016 R. Harr 25

(2)StrongInteractionsImportantformeasuringtheenergyofprotons,neutrons,pions,andkaons(calorimetry).

13 May 2016 R. Harr 26

ATypicalDetector

13 May 2016 R. Harr 27

BuildinganExperimentIdeallywewanttoidentifyeverything(particletype,charge,spin,pointoforigin,momentumatpointoforigin)emergingfromacollisioninordertoreconstructexactlywhatoccurred.

Webuildadetectorthatcomesasclosetoachievingthisgoalasmoneyallows.

Interestingcollisionscontainshortlivedparticles(top,bottom,orcharmquarks,WorZbosons,Higgsparticles,oradeconfined quarkstate)thatcannotbedirectlyseen,andmustbeinferredfromtheproductstheyleavebehind.

13 May 2016 R. Harr 28

CollideParticles

• atveryhighenergiesandconvertenergyintomass(i.e.otherparticles)

13 May 2016 R. Harr 29

DetectorLayout• Colliderdetectorshaveconvergedonastandardconfiguration.Movingoutwardfromthecollisionwehave:o precisiontrackingo trackingtomeasurecurvatureinasolenoidal magneticfield

o Cerenkovdetector,TOF,transitionradiationdet.(optional)o electromagneticcalorimetero hadronic calorimetero muondetector(alwaysoutermost)

13 May 2016 R. Harr 30

AGeneralPurposeDetector

13 May 2016 R. Harr 31

Tracking• measuretheorigin(vertex)ofchargedtracks• measurethemomentumofchargedtracks• requires:

o amagneticfieldofsufficientstrengthandextent(tomeasureradiusofcurvature)

o largevolumetracking(drivenbycost)o highprecisionmeasurementsnearthecollisionpt.o possiblysomeparticleID(dE/dx,TOF,Cerenkov,TRD)

13 May 2016 R. Harr 32

MeasuringMomentum• Inauniformmagneticfield

o p cosλ =0.3zBRo whereB isinTesla,R inmeters,z inmultiplesoftheprotoncharge,p inGeV/c.

• Theuncertaintyonp comesfrom2sources:i. resolutionoftrackpositionmeasurementsii. multiplescatteringofmaterialinthedetectoro Thesecondsourceleadsustousethinsilicondetectorsorgaseousdetectors

13 May 2016 R. Harr 33

Calorimetry• Measuretheenergyinchargedandneutralparticles

• Hadronsinteractdifferentlyfromphotonsandelectrons.EMcalorimeterplacedbeforehadronic calorimeter

13 May 2016 R. Harr 34

MeasuringEnergy• Converttheenergyofhighenergyparticlesinton lowenergyparticleso n ~E/E0 whereE0 istheaverageenergytoproducealowenergyparticle.

o ThenumberofparticlesisstochasticquantitywithPoissonfluctuationsà wewillmeasuren ± √n particles

o ThemeasuredenergyisE ± √E,sotherelativemeasurementuncertaintyis1/√E

13 May 2016 R. Harr 35

PhotonDetection• Detectingphotonsisimportantinmanysituations:astronomy,calorimetry,TOF,...

• Commondetectorsareo photomultipliers

• fastsignals,highsensitivity,lowgranularityo CCDs

• highgranularity,timeintegrating

13 May 2016 R. Harr 36

CCD• Thesensorsfordigitalcameras• Semiconductordevices,usuallysilicon• CanbecustomizedforsensitivityinIR,visible,orUV.

13 May 2016 R. Harr 37

MuonDetector• Muons are200timesheavierthanelectrons.• Muons bremstrahl with(200)2 smallerprobability

• Theresultisthattheycanpassthroughmuchmorematerialwithoutinteractingthanotherchargedparticles.

• Muondetectorisbasicallyachargedparticletrackerlocatedbehindlotsofmaterial.

13 May 2016 R. Harr 38

13 May 2016 R. Harr 39

Backup

13 May 2016 R. Harr 40

(1)Electromagnetic(cont’d)• MultipleCoulombscattering(MCS)

o yieldsaroughlyGaussiandistributionofscatteringangles

o X0 iscalledtheradiationlengthofthematerial• characterizeselectromagneticinteractionswithnucleiinamaterial

o Scatteringindependentofparticletype(excepte-)

13 May 2016 R. Harr 41

P (q)dq =1p

2pq0eq2/2q2

0dq

q0 =13.6MeV

bpc

z

rx

X0

1+0.038ln

✓x

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42

TransitionRadiationRadiationproducedwhenahighlyrelativisticelectronpassesthroughmaterialswithdifferentindicesofrefraction.

13 May 2016 R. Harr 42

CerenkovRadiationEmittedwhenaparticleexceedsthespeedoflightinamediumLiketheshockwavefromasupersonicplaneConeangleisrelatedtoparticlevelocity

13 May 2016 R. Harr 43

ElectromagneticShowers• Tomeasuretheenergyofanincomingparticle

o Convertasinglehigh-energyparticleintomanylow-energyparticles,andcountthenumberofparticles.

o Theconversioniscalledashower.o pairproduction:1photonà 2electronso Comptonscattering:1photonà 1photon+1electrono bremstrahlung:1electronà 1electron+1photon

• AftertraversingdistanceXofamedium,theaverageenergyofanelectron/photonis:

13 May 2016 R. Harr 44

hEi = E0e�X/X0

Hadronic Showers• Sameideaasforelectromagneticshowers

o incomingparticleisahadrono interactionswithmaterialcharacterizedbyinteractionlengthλI

o radiationlengths<<interactionlengthso therefore,electromagneticcalorimetersprecedehadroniccalorimetersinadetector

13 May 2016 R. Harr 45

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