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.

Short Answer

Expert verified

a)cmt2=cm02,andtherearenotransitions.ΦT=-1ħ0TV0tdt

(b)By the First-Order perturbation theory

cNt=eiΦt,cmt=0

Step by step solution

01

Step 1: First-Order perturbation theory

The first-Order perturbation equation includes all the terms in the Schrodinger equation Hψ=Eψthat represent the first order approximations to H,ψ,E,This equation can be obtained by truncating H,ψ,E,after the first order terms.

02

Step 2: (a) Solving for 

Equation 9.82

c˙m=-iħncnH'mneiEm-Ent/ħ

Here,

H'mn=ψmVotψn=δmnV0tc˙m=-iħncnH'mneiEm-Ent/ħc˙m=-iħcmV0t;dcmcm=-iħV0tdtIncm=-iħV0t'dt'+constantccmt=cm0e-iħ0tV0t'dt'

……. (11.116)

.Let,

Φt=-1ħ0tV0t'dt;cmt=eiΦcm0

Hence,

cmt2=cm02,andtherearenotransitions.ΦT=-1ħ0TV0tdt

03

Step 3: (b) Analyzing the problem in the first order perturbation theory

cNt1-iħ0tV0t'dt=1+iΦcmt=-iħ0tδmNV0t'eiEm-ENt'/ħdt=0mNcmt-iħ0tH'mNt'eiEm-ENt'/ħdt',(mN)

The exact answer is cNt=eiΦt,cmt=0, and they are consistent since, eiΦ1+i to first order.

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Most popular questions from this chapter

Solve Equation 9.13 for the case of a time-independent perturbation, assumingthatandcheck that

. Comment: Ostensibly, this system oscillates between “” Doesn’t this contradict my general assertion that no transitions occur for time-independent perturbations? No, but the reason is rather subtle: In this are not, and never were, Eigen states of the Hamiltonian—a measurement of the energy never yields. In time-dependent perturbation theory we typically contemplate turning on the perturbation for a while, and then turning it off again, in order to examine the system. At the beginning, and at the end,are Eigen states of the exact Hamiltonian, and only in this context does it make sense to say that the system underwent a transition from one to the other. For the present problem, then, assume that the perturbation was turned on at time t = 0, and off again at time T —this doesn’t affect the calculations, but it allows for a more sensible interpretation of the result.

ca=-ihHabeigtcb,cb=-ihHbaeigtca …(9.13).

A hydrogen atom is placed in a (time-dependent) electric fieldE=E(t)k.calculateallfourmatrixelementsHij,oftheperturbationH,=eEzbetween the ground state (n = 1 ) the (quadruply degenerate) first excited states (n = 2 ) . Also showthatHii,=0 for all five states. Note: There is only one integral to be done here, if you exploit oddness with respect to z; only one of the n = 2 states is “accessible” from the ground state by a perturbation of this form, and therefore the system functions as a two-state configuration—assuming transitions to higher excited states can be ignored.

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.

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).

In Equation 9.31 assumed that the atom is so small (in comparison to the wavelength of light) that spatial variations in the field can be ignored. The true electric field would be E(r,t)=E0cos(krωt).

If the atom is centered at the origin, thenkr1 over the relevant volume,|k|=2π/λ sokr~r/λ1) and that's why we could afford to drop this term. Suppose we keep the first-order correction:

E(r,t)=E0[cos(ωt)+(kr)sin(ωt)].

The first term gives rise to the allowed (electric dipole) transitions we considered in the text; the second leads to so-called forbidden (magnetic dipole and electric quadrupole) transitions (higher powers of k.rlead to even more "forbidden" transitions, associated with higher multipole moments).

(a) Obtain the spontaneous emission rate for forbidden transitions (don't bother to average over polarization and propagation directions, though this should really be done to complete the calculation). Answer:role="math" localid="1659008133999" Rba=q2ω5πϵ0c5|a|(n^r)(k^r)|b|2.

(b) Show that for a one-dimensional oscillator the forbidden transitions go from leveln to levelrole="math" localid="1659008239387" n-2 and the transition rate (suitably averaged over n^andk^) isR=q2ω3n(n1)15πϵ0m2c5.

(Note: Hereω is the frequency of the photon, not the oscillator.) Find the ratio of the "forbidden" rate to the "allowed" rate, and comment on the terminology.

(c) Show that the2S1S transition in hydrogen is not possible even by a "forbidden" transition. (As it turns out, this is true for all the higher multipoles as well; the dominant decay is in fact by two-photon emission, and the lifetime it is about a tenth of a second

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