An electron in the n=3,l=0,m=0state of hydrogen decays by a sequence of (electric dipole) transitions to the ground state.

(a) What decay routes are open to it? Specify them in the following way:

|300|nlm|n'l'm'|100.

(b) If you had a bottle full of atoms in this state, what fraction of them would decay via each route?

(c) What is the lifetime of this state? Hint: Once it’s made the first transition, it’s no longer in the state |300\rangle∣300⟩, so only the first step in each sequence is relevant in computing the lifetime.

Short Answer

Expert verified

(a)(|300|200and|300|1100)

(b)|21±1|r|300|2=2|21±1|x|300|2=K2/3

(c)  τ=1R=1.58×107s

Step by step solution

01

(a) Specifying the decay routes.

(|300|200and|300|1100violateΔl=±1rule.)

02

(b) Fraction of decay via each route. 

From Eq. 11.76:

{ifm'=m,   thenn'l'm'|x|nlm=n'l'm'|y|nlm=0ifm'=m±1,thenn'l'm'|x|nlm=±i(n'l'm'|y|nlmandn'l'm'|z|nlm=0(11.76).

210|r|300=210|z|300k^21±1|r|300=21±1|x|300i^+21±1|y|300j^

±21±1|x|300=i21±1|y|.Thus|210|r|300|2=|210|z|300|2   and   |21±1|r|300|2=2|21±1|x|300|2

So there are really just two matrix elements to calculate.

ψ21m=R21Y1m,   ψ300=R30Y00.From Table 4.3:

Y10Y00cosθsinθdθdϕ=34π14π0πcos2θsinθdθ02πdϕ=34π(cos3θ3)|0π(2π)=32(23)=13

(Y1±1)*Y00sin2θcosϕdθdϕ=38π14π0πsin3θdθ02πcosϕeiϕdϕ=14π32(43)[02πcos2ϕdϕi02πcosϕsinϕdϕ]=1π6(π0)=16

From Table 4.7:

K0R21R30r3dr=124a3/2227a3/20raer/2a[123ra+227(ra)2]er/3ar3dr=192a3a40(123u+227u2)u4e5u/6du=a92[4!(65)5235!(65)6+2276!(65)7]

=a924!6556(52365+22763)=a924!6556=2734562a

So,

21±1|x|300=R21(Y1±1)*(rsinθcosϕ)R30Y00r2sinθdrdθdϕ=K(16)

210|z|300=R21Y10(rcosθ)R30Y00r2sinθdrdθdϕ=K(13)

|210|r|300|2=|210|z|300|2=K2/3;|21±1|r|300|2=2|21±1|x|300|2=K2/3

Evidently the three transition rates are equal, and hence 1/3 go by each route.

03

(c) Lifetime of the state

For each mode,

A=ω3e2|r|23πϵ0c3here,ω=E3E2=1(E19E14)=536E1,

so the total decay rate is

R=3(536E1)3e23πϵ0c313(2734562a)2=6(25)9(E1mc2)2(ca)

=6(25)9(13.60.511×106)2(3×1080.529×1010)/s=6.32×106/sτ=1R=1.58×107s

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Most popular questions from this chapter

Solve Equation 9.13 to second order in perturbation theory, for the general case ca(0)=a,cb(0)=bca=-ihH'abe-0tcb,cb=-ihH'bae-0tca

(9.13).

Prove the commutation relation in Equation 9.74. Hint: First show that

[L2,z]=2ih(xLy-yLx-ihz)

Use this, and the fact that localid="1657963185161" r.L=r.(r×p)=0, to demonstrate that

[L2,[L2,z]]=2h2(zL2+L2z)

The generalization from z to r is trivial.

A particle starts out (at time t=0 ) in the Nth state of the infinite square well. Now the “floor” of the well rises temporarily (maybe water leaks in, and then drains out again), so that the potential inside is uniform but time dependent:V0(t),withV0(0)=V0(T)=0.

(a) Solve for the exact cm(t), using Equation 11.116, and show that the wave function changes phase, but no transitions occur. Find the phase change, role="math" localid="1658378247097" ϕ(T), in terms of the function V0(t)

(b) Analyze the same problem in first-order perturbation theory, and compare your answers. Compare your answers.
Comment: The same result holds whenever the perturbation simply adds a constant (constant in x, that is, not in to the potential; it has nothing to do with the infinite square well, as such. Compare Problem 1.8.

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.)

Develop time-dependent perturbation theory for a multi-level system, starting with the generalization of Equations 9.1 and 9.2:

H^0ψn=Enψn,   ψnψm=δnm (9.79)

At time t = 0 we turn on a perturbation H'(t)so that the total Hamiltonian is

H^=H^0+H^'(t)(9.80).

(a) Generalize Equation 9.6 to read

Ψ(t)=ca(t)ψaeiEat/+cb(t)ψbeiEbt/(9.81).

and show that

c˙m=incnHmn'ei(EmEn)t/ (9.82).

Where

Hmn'ψm|H^'|ψn (9.83).

(b) If the system starts out in the state ψN, show that (in first-order perturbation theory)

cN(t)1i0tHNN'(t')dt'(9.84).

and

cm(t)i0tHmN'(t')ei(EmEN)t'/dt',   (mN)(9.85).

(c) For example, supposeH^'is constant (except that it was turned on at t = 0 , and switched off again at some later time . Find the probability of transition from state N to state M (MN),as a function of T. Answer:

4|HMN'|2sin2[(ENEM)T/2](ENEM)2 (9.86).

(d) Now supposeH^'is a sinusoidal function of timeH^'=Vcos(ωt): Making the usual assumptions, show that transitions occur only to states with energy EM=EN±, and the transition probability is

PNM=|VMN|2sin2[(ENEM±ω)T/2](ENEM±ω)2 (9.87).

(e) Suppose a multi-level system is immersed in incoherent electromagnetic radiation. Using Section 9.2.3 as a guide, show that the transition rate for stimulated emission is given by the same formula (Equation 9.47) as for a two-level system.

Rba=π3ϵ02||2ρ(ω0)Rb (9.47).

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