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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).

Short Answer

Expert verified

The second order perturbation theory for the equation is

cα(2)(t)=α-ibh0tHabc(tc)e-iω0tcdtc-αh20tHabc(tc)e-iω0tc0tcHbac(tcc)eiω0tccdtccdtccb(2)(t)=b-iah0tHabc(t¢)eiω0tcdtc-bh20tHabc(t¢)eiω0tcdtc0tcHbac(tcc)e-iω0tccdtccdtc

Step by step solution

01

Concept.

Consider a time dependent potential, we can solve the Schrodinger equation for this potential in a two state system if we split the Hamiltonian into a time independent part H°and time dependent part H', that is:

H=H°+H1

This is done in the section 9.1 to get the solution.

02

Solving the given equation to second order perturbation theory

Wehave,Zeroorder:cα(0)(t)=α,cb(0)(t)=bThecoefficientsaresolutionsofthecouplesODEs,thatis:Theequation9.13isc.a=-iHab'e-iω0tcb,c.b=-iHab'e-iω0tcαFirstorder;c.a=-iHab'e-0tbcα(1)(t)=α-ib0tHab'(t)e-0tdt'c.a=-iHab'e-0tαcb(1)(t)=b-0tHab'(t)e-0tdt'Secondorder:c.a=-iHab'e-0tb-0tHab'(t)e-0tdt'cα(2)(t)=α-ibHab'(t)e-0tdt'-α20tHab'(t)e-0tdt'0tHba'(t)e-0tdt'dt'Togetcbjustswitchab(whichentailsalsochangingthesignofω0)cb(2)(t)=b-iaHba'(t')e0tdt'-b20tHab'(t')e0tdt'0tHba'(t')e-0tdt'dt'

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Most popular questions from this chapter

Close the “loophole” in Equation 9.78 by showing that ifl'=l=0thenn'l'm'|r|nlm=0

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.

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.

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.)

A particle of mass m is initially in the ground state of the (one-dimensional) infinite square well. At time t = 0 a “brick” is dropped into the well, so that the potential becomes

V(x)={V0,0xa/20,a/2<xa;,otherwise

where V0E1After a time T, the brick is removed, and the energy of the particle is measured. Find the probability (in first-order perturbation theory) that the result is nowE2 .

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