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)

Short Answer

Expert verified

ca(t)=1,t<0cos(αlh),t<0,cb(t)=0,t<0-iα+αsin(αlh),t>0,Pab=b2=sin(αlh),

Step by step solution

01

Concept.

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

H+=Uδ(t)

Where perturbation to the Hamiltonian in a two state system is switched on at r = 0 and then off again at some later time t=l-. The safest approach is to represent the delta function as:

H'={U\l-0<t<l-0otherwise

02

Finding  ca(t) and cb(t)

ca(-ϵ)=1=-α+ei(ω0-ω)ϵ/2A[(ω+ω0)+(ω-ω0)]=-2ωα+/α*e(i(ω0-ω)ϵ/2)A,soA.=-α+2ωei(ω0-ω)/2ca(t)=12ωe-iω0(t+ϵ)/2)[(ω+ω0)eiω(t+ϵ)/2+(ω-ω0)e-iω(t+ϵ)/2]=e-iω0(t+ϵ)/2cosω(t+)2+iω0ωsinω(t+)2cb(t)=-α+2ωeiω0(t-ϵ)/2eiω0(t+ϵ)/2)-e-iω0(t+ϵ)/2)=-iα+ωeiω0(t+ϵ)/2)sinω(t+)2.This is a tricky problem, and I thank Prof. Onuttom Narayan for showing me the correct solution. The safest approach is to represent the delta function as a sequence of rectangles:

δ0(t)={(1/2),-<t<0,otherwise}

Then Eq.11.17

t<-:ca(t)=1,cb(t)=0t>:ca(t)=a,cb(t)=b-<t<:ca=-iα2he-iω0tcbcb=-iα2he-iω0tcaca=-ihHab'e-ω0tcb,ca=-ihHba'e-ω0tcb,(11.17)

In the interval -<t<

d2cbdt2=-iα+2hiω0eiω0tca+eiω0tiα+2he-iω0tcb=-iα+2hiω0i2hα+dcbdt-iα2hcb=iω0dcadt-α2(2h)2cb

Thus cbsatisfies a homogeneous linear differential equation with constant coefficients:

d2cbdt2-iω0

Try a solution of the form cb(t)=eλt

λ2-iω0λ+α2(2h)2=0λ=iω0±iω02-α2/h22orλ=02±2,whereω02-α2/h2.

The general solution is

cb(t)=eiω0t/2(Aeiω0t/2+Beiω0t/2)Butcb(-)=0Ae0t/2+Be0t/2=0B=-Ae0So,cb(t)=Ae0t/2(e0t/2-e-(+t/2))

Meanwhile

localid="1655973144761" ca(t)=2ihα+e-iω0tca=2ihα+e-iω0t/2Aiω02(eiωt/2-e-iω(iω0t/2))+iω2(eiωt/2-e-iω(iω0t/2))=-hα+e-iω0t/2A(ω+ω0)eiωt/2+(ω-ω0)e-iωt/2

But

ca(-ϵ)=1=-α+ei(ω0-ω)ϵ/2A[(ω+ω0)+(ω-ω0)]=-2ωα+/α*e(i(ω0-ω)ϵ/2)A,soA.=-α+2ωei(ω0-ω)/2ca(t)=12ωe-iω0(t+ϵ)/2)[(ω+ω0)eiω(t+ϵ)/2+(ω-ω0)e-iω(t+ϵ)/2]=e-iω0(t+ϵ)/2cosω(t+)2+iω0ωsinω(t+)2cb(t)=-α+2ωeiω0(t-ϵ)/2eiω0(t+ϵ)/2)-e-iω0(t+ϵ)/2)=-iα+ωeiω0(t+ϵ)/2)sinω(t+)2.

Thus

localid="1655977472500" α=cα()=e-iω0cosω+iω0ωsinω,b=cb()=-iα+hωsinωThisisfortherectangularpulse;itremainstotakethelimit0;ωα/hsoαcosαh+iω0hαsinαhcosαh,b-+αsinαhandweconcludethatforthedeltafunctionca(t)=1,t<0cos(α/h),t>0;cb(t)=0,t<0-iα+αsin(α/h),t>0Obviously,|ca(t)|2+|cb(t)|2=1inbothtimeperiods.FinallyPab=b2=sin2(α/h)

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Most popular questions from this chapter

Suppose you don’t assumeH'aa=H'aa=0

(a) Findca(t)andcb(t)in first-order perturbation theory, for the case

ce(0)=1,cb(0)=0.show that |ca(1)(t)|2+|cb(1)(t)|2=1, to first order inH^' .

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

daeih0tHaac(tc)dtc0ca,dbei20tHbbc(tc)dtc0cb.

Show that

role="math" localid="1658561855290" d-a=-iheiϕH'abe-iω0tdb;db-=-iheiϕH'bae-iω0tda

where

ϕ(t)1h0l[H'aa(t')-H'bb(t')]dt'.

So the equations fordaanddbare identical in structure to Equation 11.17 (with an extra role="math" localid="1658562498216" eiϕtackedontoH^')

ca-=-ihH'abe-iω0tcb,cb-=-ihH'baeiω0tca

(c) Use the method in part (b) to obtainrole="math" localid="1658562468835" ca(t)andcb(t)in first-order
perturbation theory, and compare your answer to (a). Comment on any discrepancies.

You could derive the spontaneous emission rate (Equation 11.63) without the detour through Einstein’s A and B coefficients if you knew the ground state energy density of the electromagnetic field P0(ω)for then it would simply be a case of stimulated emission (Equation 11.54). To do this honestly would require quantum electrodynamics, but if you are prepared to believe that the ground state consists of one photon in each classical mode, then the derivation is very simple:

(a) Replace Equation 5.111by localid="1658381580036" N0=dkand deduce P0(ω) (Presumably this formula breaks down at high frequency, else the total "vacuum energy" would be infinite ... but that's a story for a different day.)

(b) Use your result, together with Equation 9.47, to obtain the spontaneous emission rate. Compare Equation 9.56.

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.

As a mechanism for downward transitions, spontaneous emission competes with thermally stimulated emission (stimulated emission for which blackbody radiation is the source). Show that at room temperature (T = 300 K) thermal stimulation dominates for frequencies well below 5×1012Hz , whereas spontaneous emission dominates for frequencies well above . Which mechanism dominates for visible light?

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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