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12.1. THESCALEOFTHEWORLD 201


normalizationgivesN=(2a 0 )−^1 /^2 ,andtherefore


φ 200 =

1



8 πa^30

(
1 −

r
2 a 0

)
e−r/^2 a^0 (12.51)

Ingeneral,thewavefunctionforprincipalquantumnumberhastheform

φnlm=(polynomialinroforder≤n-1)×e−r/na^0 Ylm(θ,φ) (12.52)

Apolynomialcangothroughzero,soingeneraltheprobabilitydistributioninthe
radialdirectionhas”bumps”,whosepositionsdependonbothnandl.Inparticular,
ifweareonlyinterestedintheprobabilityoffindinganelectronbetweenradiir 1 and
r 2 ,then


prob(r 1 <r<r 2 ) =

∫r 2

r 1

drr^2


dΩφ∗nlmφnlm

=

∫r 2

r 1

drr^2 Rnl^2 (r)

=

∫r 2

r 1

drP(r) (12.53)

wherewedefinetheradialprobabilitydensity


P(r) = r^2 R^2 nl(r)
= ((2n-thorderpolynomialinr)×e−^2 r/na^0 (12.54)

AsketchofP(r)vs. risshowninFig. [12.2],foranumberof low-lyingenergy
eigenstates.


12.1 The Scale of the World


Weknowthatthevolumeofagramofwaterisonecubiccentimeter. Whyisn’tthe
volumeinsteadonecubickilometer,oronecubicparsec?
Ifyouburnaloginafireplace,enoughenergyisreleasedtowarmtheroom. If
youburninsteadastickofdynamite,theenergyreleasedwilldestroytheroom,and
probablythe restofthehouse. Butneitherthelognorthe dynamitewillrelease
enoughenergytoflattenacity,orvaporizetheplanet. Whynot?
Quantummechanicsanswers thesequestions, givenasinput themasses of the
electronandproton,andtheelectroncharge. Infact,thesolutionoftheHydrogen
atomprovidesuswithrough,order-of-magnitudeestimatesforthevolumeofamole
ofsolid anything,andtheenergyreleasedbyburningamoleofanything. Thisis

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