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In view ofProblem 5.1, we can correct for the motion of the nucleus in hydrogen by simply replacing the electron mass with the reduced mass.

(a) Find (to two significant digits) the percent error in the binding energy of hydrogen (Equation 4.77) introduced by our use of m instead of μ.

E1=-m2h2e24π'2=-13.6eV(4.77).

(b) Find the separation in wavelength between the red Balmer lines n=3n=2for hydrogen and deuterium (whose nucleus contains a neutron as well as the proton).

(c) Find the binding energy of positronium (in which the proton is replaced by a positron—positrons have the same mass as electrons, but opposite charge).

(d) Suppose you wanted to confirm the existence of muonic hydrogen, in which the electron is replaced by a muon (same charge, but 206.77 times heavier). Where (i.e. at what wavelength) would you look for the “Lyman-α” line n=2n=1?.

Short Answer

Expert verified

(a) The percent error is 0.054%

(b)λ=9.109×10-312(1.673×10-27)(6.563×10-7)m=1.79×10-10m.

(c)μ=(13.6/2)eV=6.8eV.

(d)λ=6.54×10-10m.

Step by step solution

01

(a) Finding the percent error in the binding energy of hydrogen,

From Eq. 4.77,

E1=-me2h2e4π'2=-13eV (4.77).

E1is proportional to mass, so E1E1=mμ=m-μμ=mm+MmM-MM=mM

The fractional error is the ratio of the electron mass(m) to the proton mass(M):

9.109×10-31kg1.673×10-27kg=5.44×10-4

. The percent error is 0.054% (pretty small).

02

(b) Finding the separation in wavelength between the red Balmer lines(n=3→n=2) 

From Eq. 4.94, R is proportional to m, so

R=m4πch3e24π'2=1.097×107m-1 (4.94).

1+λ1+λ=RR=μμ=-1-λ2λ1-λ=-λλ.

So (in magnitude)role="math" localid="1656065390250" λ/λ=μ/μ.Butμ=mM/m+M., where m = electron mass,

and M = nuclear mass.

μ=m2mpm+2mp-mmpm+mp=mmpm+mpm+2mp2m+2mp-m-2mp.=m2mpm+mpm+2mp=mμm+2mpλλ=μμ=mm+2mpm2mpsoλ=m2mpλh,whereisthehydrogenwavelength.1λ=R14-19=536Rλ=365R=3651.097×107m=6.563×10-7m.λ=9.109×10-3121.673×10-276.563×10-7m=1.79×10-10m.

03

(c) Finding the binding energy of positronium,

μ=mmm+m=m2,sotheenergyishalfwhatitwouldbeforhydrogen:13.6/2eV=6.8eV.
04

(d) The “Lyman-α” line (n=2→n=1)is at,

μ=mpmμmpmμ;Rμ,soRischangedbyafactormpmμmp+mμ-mpmemp+me=mμmpmememp+mμ,ascomparedwithhydrogen.Forhydrogen,1/λ=R1-1/4=34Rλ=4/31.097×107m=1.215×10-7m,andλ1/R,soformuonichydrogentheLyman-alphalineisatλ=mμmpmememp+mμ1.215×10-7m=1206.771.673×10-27+206.77×9.109×10-311.673×10-27+9.109×10-311.215×10-7m=6.54×10-10m.

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Most popular questions from this chapter

Find the average energy per free electron (Etot/Nd), as a fraction of the

Fermi energy. Answer:(3/5)EF

Typically, the interaction potential depends only on the vectorr=r1-r2between

the two particles. In that case the Schrodinger equation seperates, if we change variables from r1,r2andR=(m1r1+m2r2)I(m1+m2)(the center of mass).

(a)Show that

localid="1655976113066" r1=R+(μ/m1)r,r2=R-(μ/m)r,and1=(μ/m)R+r,2=(μ/m1)R-r,where

localid="1655976264171" μ=m1m2m1+m2(5.15).

is the reduced mass of the system

(b) Show that the (time-independent) Schrödinger equation (5.7) becomes

-h22m112ψ-h22m222ψ+=-h22(m1+m2)R2ψ-h22μr2ψ+V(r)ψ=.(5.7).

(c) Separate the variables, letting ψ(R,r)=ψR(R)ψr(r)Note that ψRsatisfies the

one-particle Schrödinger equation, with the total mass (m1+m2)in place of m, potential zero, and energy ERwhile ψrsatisfies the one-particle Schrödinger equation with the reduced mass in place of m, potential V(r) , and energy localid="1655977092786" Er. The total energy is the sum: E=ER+Er. What this tells us is that the center of mass moves like a free particle, and the relative motion (that is, the motion of particle 2 with respect to particle 1) is the same as if we had a single particle with the reduced mass, subject to the potential V. Exactly the same decomposition occurs in classical mechanics; it reduces the two-body problem to an equivalent one-body problem.

(a) Using Equations 5.59 and 5.63, show that the wave function for a particle in the periodic delta-function potential can be written in the form

ψ(X)=C[sinkx+e-ikasina-x]0xa

(b) There is an exception; At the top of a band where z is an integer multiple ofπyielsψ(x)=0 yields .

Find the correct wave function for the case. Note what happens toψeach delta function.

a) Hund’s first rule says that, consistent with the Pauli principle, the state with the highest total spin (S) will have the lowest energy. What would this predict in the case of the excited states of helium?

(b) Hund’s second rule says that, for a given spin, the state with the highest total orbital angular momentum (L) , consistent with overall antisymmetrization, will have the lowest energy. Why doesn’t carbon haveL=2? Note that the “top of the ladder”(ML=L)is symmetric.

(c) Hund’s third rule says that if a subshell(n,l)is no more than half filled,
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(d) Use Hund’s rules, together with the fact that a symmetric spin state must go with an antisymmetric position state (and vice versa) to resolve the carbon and nitrogen ambiguities in Problem 5.12(b). Hint: Always go to the “top of the ladder” to figure out the symmetry of a state.

Find the energy at the bottom of the first allowed band, for the caseβ=10 , correct to three significant digits. For the sake of argument, assume αa=1eV.

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