PHZ 7357, Fall 20171HW1
PHZ7357,Fall2017,HW1DueSeptember15,at5:10pm
Name
1) YouarerepeatingC.Andersonexperimentandobtainedapicturefromthecloudchamber(ontheright).Thecloudchamberisdividedinhalfbythe6mmthickleadplate.Chargedparticletrackiscrossingthechamberandtheleadplate.ThewholesetupisintheuniformH=1.5Teslamagneticfieldpointingfromyou.
H=1.5T
a) Explainhowyoufindthesignoftheparticle’scharge.b) Measuremomentumoftheparticleinthetopandthebottom
partsofthechamber(neglectlosesinthecloudchamber).Motivateyourmeasurementmethod.CompareyourresultwiththeresultobtainedbyAnderson(findlinktohisarticleinthecoursedairy).
c) Useparticle’smomentummeasuredbyAnderson.Assumingthattheionizationlossesinleadare!"
!#~ %&'𝑀𝑒𝑉𝑔,%𝑐𝑚/estimate
theparticle’smassM.d) ArguewhytherealmassoftheparticlemcanbelessthanM.e) Arguewhyparticle’schargecannotbegreaterthan2e.f) Estimateenergylossinleadwhenm<<M.
PHZ 7357, Fall 20172HW1
Name
2. DrawlowestorderFeynmandiagramfortheprocessofphotonsplitting𝛾 + 𝑍, 𝐴 → 𝛾 + 𝛾.Estimateratioofcross-sectionsforphotonsplittingontungsten(W)andhydrogen(H)targets.
3. DrawthelowestorderFeynmandiagramsfortheprocess𝜈7 + 𝑒, → 𝜈7 + 𝑒,
4. DrawthelowestorderFeynmandiagramfortheprocess𝑒8 +𝑒, → 𝛾 + 𝛾.Estimatetherangeoftheforcewhen𝑒8𝑎𝑛𝑑𝑒,areatrest
5. Whatisthedominantreactionthatproducessolarneutrinos?Calculatethemaximumenergyofneutrinosproducedbythisreaction.
6. ExplainhowcanthetotalfluxofneutrinosproducedintheSunbemeasuredonEarth bySNOexperiment.ListthemainneutrinointeractionprocessesdetectedbySNO.Calculatetheneutrinoenergythresholdforeachprocess.
7. CalculatetheoscillationlengthL13andL12forelectronantineutrinoswithenergy3MeV.Whyisthetwo-componentmixingmodelagoodapproximationforneutrinooscillationsatdistanceof1kmand200km?Woulditbeareasonableapproximationfordistanceof10km?
PHZ 7357, Fall 20173HW1
PHZ 7357, Fall 20174HW1
DiracEquation• HofmassiveparticlehasanextratermbmwhichmixestwoWeyl
equations-Y=YR+YL – 4-componentspinors
Expanding
s
PHZ 7357, Fall 20175HW1
ProbabilityDensityandCurrent
S�⃗� =𝑞𝑚𝑆 = 2
𝑞2𝑚 �⃗� → −𝑔
𝑞𝑒 𝜇E�⃗�
µm – magneton
g-factor=2forDiracparticle,ge~2,gp=2.79– protonisnotpoint-like
PHZ 7357, Fall 20176HW1
theDiracgMatrices
PHZ 7357, Fall 20177HW1
Pauli-DiracRepresentation
• this4-vectorcurrentisusedforderivationoftheLorentzinvariantmatrixelementforthefundamentalinteractions.