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Show that the spontaneous emission rate (Equation 9.56) for a transition from n,lton',l' in hydrogen is

e2ω2l23πo0hc3˙×{l+12l+1ifl'=l+1l2l-1ifl'=l-1

where

l=0r3Rnl(r)Rn'J'(r)dr

(The atom starts out with a specific value of m, and it goes toamyof the state’s mconsistent with the selection rules:m'=m+1,m or m -1 . Notice that the answer is independent of m .) Hint: First calculate all the nonzero matrix elements of x,y,and z between role="math" localid="1658313179553" |n|m>andn'l'm'>for the case . From these, determine the quantity

|n'.1+1.m+1rn|m|2+|n'.1+1,mr|nm|2+|n'.1+1,m-1r|nm|2

Then do the same forl'=l-1.

Short Answer

Expert verified

Hence showed that A=q2ll-12ω033o0πhc3˙l+12l+1and A=q2ll-12ω033o0πhc3˙l+12l-1.

Step by step solution

01

Define Spontaneous emission rate.

The spontaneous emission rate for a charge q, in a starting stateψa>decaying to the state is given by,

A=ω03||230πhc3… (1)

Here, the matrix element of the diploe moment,=q<ψbrψa>… (2)

The hydrogen wave function is given by, ψnlm=Rn(r)Ylm(θ,ϕ)… (3) Here,Rnis a radial function and Ylmis a spherical hormonic.

02

Obtain the transition using the integrals of spherical harmonics.

The transitions are allowed from a state nlm>only for ll±1and mm,m±1for the hydrogen atom (the selection rule). Suppose that the starting state is nlm>and finishing state is n'l'm'>.

For l'=l+1, work out the transition rates to all possible final values of m', for m'=m+1and m'=m-1.

Use the integrals of spherical harmonics to get:

02x0πYlmθϕY00θϕYl-mθϕdθdϕ=14π02x0πYlmθϕY10θϕYl+1-mθϕdθdϕ=34π(l+m+1)(l-m+1)(2l+1)(2l+3)02x0πYlmθϕY10θϕYl-1-(m+1)θϕdθdϕ=38π(l+m+1)(l-m+2)(2l+1)(2l+3)02x0πYlmθϕY10θϕYl-1-(m+1)θϕdθdϕ=38π(l-m)(l-m-1)(2l-1)(2l+1)And02x0πYl1m1θϕYl2m2θϕYl2-m2θϕdθdϕ=0,m1+m2m3

03

Find <ψbxψa>,<ψbyψa>and <ψb|z|ψa> .

In spherical coordinates, the values are:

x=rsin(θ)cosϕy=rsin(θ)sinϕz=rcosθ

In terms of the spherical harmonics as:

x+iy=rsinθeiϕ=-r8π3Y11x-iy=r8π3Y1-1z=r8π3Y10

The only non-zero matrix elements by using equation (4) are:

localid="1658318624067" n,l+1,mznlm=1l,11l+1,m4π3Y10om˙=ll+14π302π0πYlvnθϕY10θϕYl+1mθϕdθdϕ=ll+1(l+m+1)(l-m+1)(2l+1)(2l+3) ……(5)

localid="1658376948601" a¨=-ll+18π302π0πYtmθϕ˙Y11θϕYl+1-(m+1)θϕdθdϕ=-ll+1(l+m+1)(l+m+2)(2l+1)(2l+3)......(6)=nlmx+iyn,l+1,m-1*=-ll+18π302π0πYl+1m-1θφ˙Y11θϕ˙Yl-mθϕ˙dθdϕ=-ll+1(l+1-(m-1)(l+1-(m-1)-1)(2(l+1)(2(l+1)+1)=-ll+1(l-m+2)(l-m+1)(2l+1)(2l+3)...(7)

Here,localid="1658376877539" a˙=n',l+1+m+1x+iynlm°=n',l+1+m-1x-iynlm. And also,.

ll+1=0r3Rnl(r)Rn(l+1)(r)dr.

To separate x and y, in (6) and (7), note that:

localid="1658376981160" n',l+1+m-1x-iynlm=ll+18π302π0πYl+1m-1θφ˙Y11θϕ˙Yl-mθϕ˙dθdϕ=0

As it is zero, add it to (6) and subtracted also from (6), so separate x and y to get:

localid="1658378320569" n',l+1+m+1xnlm=-12lln(l+m+1)(l+m+2)(2l+1)(2l+3) ……. (8)

localid="1658378337745" n',l+1+m+1ynlm=-12ll1(l+m+1)(l+m+2)(2l+1)(2l+3) ……. (9)

By adding it to (7) and also subtracted from (7), so separate and to get:

localid="1658378363128" n',l+1+m-1xnlm=-12lL+1(l-m+1)(l-m+2)(2l+1)(2l+3) ……. (10)

localid="1658378375668" n',l+1+m-1ynlm=-12ll+1(l-m+2)(l-m+1)(2l+1)(2l+3) ……. (11)

04

Find the value of A.

Put all these results together into the square modules of the dipole moment to get:

P2q2=n',l+1,mznlm2+n',l+1,m+1xnlm2+n',l+1,m+1ynlm2+n',l+1,m-1xnlm2+n',l+1,m-1ynlm2

Substitute from (8), (9), (10) and (11) into this equation to get:

2=q2ll+12(l+m+1)(l-m+1)+12(l+m+1)(l+m+2)+(l-m+1)(2l+1)(2l+3)=q2ll+12l+12l+1

Substitute into (1) to get:

role="math" localid="1658382762842" A=q2ll+12ω03300πhc3˙l+12l+1

05

Find the non-zero matrix element.

Follow the same method for l'=l-1.

n'l-1,mznlm=n',l,mzn,l-1,m*=ll-1(l+m)(l-m)(2l-1)(2l+1) ……. (12)

role="math" localid="1658381942976" n'l-1,m-1x-iynlm=nlmx+iyn',l-1,m-1=-ll-1(l+m-1)(l+m)(2l-1)(2l+1)....(13)n'l-1,m+1x+iynlm=-ll-1(l-m-1)(l-m)(2l-1)(2l+1).......(14)

Separate and to get:

n'l-1,m-1xnlm=-12ll-1(l+m-1)(l+m)(2l-1)(2l+1)....(15)n'l-1,m-1ynlm=-12ll-1(l+m-1)(l+m)(2l-1)(2l+1).......(16)

n'l-1,m+1xnlm=-12ll-1(l-m-1)(l-m)(2l-1)(2l+1)....(17)n'l-1,m-1ynlm=-12ll-1(l-m-1)(l-m)(2l-1)(2l+1).......(18)

Put all these results to get the dipole moment:

role="math" localid="1658382683044" 2=q2ll+12(l+1)(l-m)+12(l+m-1)(l+m)+(l-m-1)(l-m)(2l-1)(2l+1)=q2ll-12l2l-1

Substitute into (1) we get:

A=q2ll-12ω033o˙0πhc3l2l-1

Hence proved.

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Most popular questions from this chapter

The first term in Equation 9.25 comes from the eiωt/2, and the second from e-iωt/2.. Thus dropping the first term is formally equivalent to writing H^=(V/2)e-iωt, which is to say,

cbl-ihvba0tcos(ωt')eiω0t'dt'=-iVba2h0tej(ω0+ω)t'+ej(ω0-ω)t'dt'=--iVba2hej(ω0+ω)t'-1ω0+ω+ej(ω0-ω)t'-1ω0-ω(9.25).Hba'=Vba2e-iωt,Hab'=Vab2eiωt(9.29).

(The latter is required to make the Hamiltonian matrix hermitian—or, if you prefer, to pick out the dominant term in the formula analogous to Equation 9.25 forca(t). ) Rabi noticed that if you make this so-called rotating wave approximation at the beginning of the calculation, Equation 9.13 can be solved exactly, with no need for perturbation theory, and no assumption about the strength of the field.

c.a=-ihHab'e-iω0tcb,c.b=-ihHba'e-iω0tca,

(a) Solve Equation 9.13 in the rotating wave approximation (Equation 9.29), for the usual initial conditions: ca(0)=1,cb(0)=0. Express your results (ca(t)andcb(t))in terms of the Rabi flopping frequency,

ωr=12(ω-ω0)2+(Vab/h)2 (9.30).

(b) Determine the transition probability,Pab(t), and show that it never exceeds 1. Confirm that.

ca(t)2+cb(t)2=1.

(c) Check that Pab(t)reduces to the perturbation theory result (Equation 9.28) when the perturbation is “small,” and state precisely what small means in this context, as a constraint on V.

Pab(t)=cb(t)2Vab2hsin2ω0-ωt/2ω0-ω2(9.28)

(d) At what time does the system first return to its initial state?


Suppose you don’t assume Haa=Hbb=0

(a) Find ca(t)and cb(t) in first-order perturbation theory, for the case

.show that , to first order in .

(b) There is a nicer way to handle this problem. Let

.

Show that

where

So the equations for are identical in structure to Equation 11.17 (with an extra

(c) Use the method in part (b) to obtain in first-order
perturbation theory, and compare your answer to (a). Comment on any discrepancies.

We have encountered stimulated emission, (stimulated) absorption, and spontaneous emission. How come there is no such thing as spontaneous absorption?

Suppose the perturbation takes the form of a delta function (in time):

H^'=U^δ(t);

Assume thatUaa=Ubb=0,andletUab=Uba+=αif ca(-)=1and cb(-)=0,

find ca(t)andcb(t),and check that lc(t)l2+lcb(t)l2=1. What is the net probability(Pabfort) that a transition occurs? Hint: You might want to treat the delta function as the limit of a sequence of rectangles.

Answer:Pab=sin2(|α|lh)

Magnetic resonance. A spin-1/2 particle with gyromagnetic ratio γ at rest in a static magnetic fieldB0k^ precesses at the Larmor frequencyω0=γB0 (Example 4.3). Now we turn on a small transverse radiofrequency (rf) field,Brf[cos(ωt)ı^sin(ωt)j^]$, so that the total field is

role="math" localid="1659004119542" B=Brfcos(ωt)ı^Brfsin(ωt)j^+B0k^

(a) Construct the 2×2Hamiltonian matrix (Equation 4.158) for this system.

(b) If χ(t)=(a(t)b(t))is the spin state at time t, show that

a˙=i2(Ωeiωtb+ω0a):   b˙=i2(Ωeiωtaω0b)

where ΩγBrfis related to the strength of the rf field.

(c) Check that the general solution fora(t) andb(t) in terms of their initial valuesa0 andb0 is

role="math" localid="1659004637631" a(t)={a0cos(ω't/2)+iω'[a0(ω0ω)+b0Ω]sin(ω't/2)}eiωt/2b(t)={b0cos(ω't/2)+iω'[b0(ωω0)+a0Ω]sin(ω't/2)}eiωt/2

Where

ω'(ωω0)2+Ω2

(d) If the particle starts out with spin up (i.e. a0=1,b0=0,), find the probability of a transition to spin down, as a function of time. Answer:P(t)={Ω2/[(ωω0)2+Ω2]}sin2(ω't/2)

(e) Sketch the resonance curve,

role="math" localid="1659004767993" P(ω)=Ω2(ωω0)2+Ω2,

as a function of the driving frequencyω (for fixed ω0andΩ ). Note that the maximum occurs atω=ω0 Find the "full width at half maximum,"Δω

(f) Since ω0=γB0we can use the experimentally observed resonance to determine the magnetic dipole moment of the particle. In a nuclear magnetic resonance (nmr) experiment the factor of the proton is to be measured, using a static field of 10,000 gauss and an rf field of amplitude gauss. What will the resonant frequency be? (See Section for the magnetic moment of the proton.) Find the width of the resonance curve. (Give your answers in Hz.)

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