QMGreensite_merged

(bbancia) #1

6.3. THEENERGYOFENERGYEIGENSTATES 95


state”). Energyeigenstatesofhigherenergiesareknownas”excitedstates.”The
factthatthegroundstateenergyoftheparticleinthetubeE 1 isgreaterthanzero
isanotherexampleoftheUncertaintyPrincipleatwork. Sincethethe particleis
confinedinaregionoflengthL,itmeansthat∆x≤L,andtherefore


∆p>

̄h
2 L

(6.61)


Assuming

=0,thiswouldgivealowerboundtotheenergyofroughly


E≈


(∆p)^2
2 m

>


̄h^2
8 mL^2

(6.62)


andthislowerboundisinfact smaller,bysome numerical factors, than thetrue
groundstateenergyE 1 givenin(6.59),inagreementwiththeUncertaintyPrinciple.
Notethatthedependenceonh, ̄m,LofthelowerboundisthesameasthatofE 1.
Again, itisnotaquestion of ”theobservationdisturbing theobserved.” Thereis
simplynophysicalstateofaparticleinatubewhichhasanenergylowerthanE 1.
Energyeigenstatesarestationarystates,inthesensethatthetime-dependenceof
thewavefunctionisentirelycontainedinanoverallphasefactor


ψα(x,t)=φα(x)e−iEαt/ ̄h (6.63)

andthisphasecancelsoutwhencomputingexpectationvaluesofanyfunctionofx
andp,e.g.


<x> =


dxψα∗(x,t)xψα(x,t)

=


dxφ∗α(x)xφα(x)

<p> =


dxψα∗(x,t)p ̃ψα(x,t)

=


dxφ∗α(x)p ̃φα(x) (6.64)

Therefore


∂t<x> = 0

<−

∂V


∂x

> = 0 (6.65)


wherethesecondequationfollowsfrom∂t

=0,andEhrenfest’sPrinciple.Note
that theseequations aresimilar to thecorresponding expressionsfor astationary
stateinclassicalmechanics:theparticleisstatic,so


∂tx= 0 (6.66)
Free download pdf