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Starting with Equation 6.80, and using Equations 6.57, 6.61, 6.64, and 6.81, derive Equation 6.82.

Short Answer

Expert verified

The equation is derived,Efs1=13.6eVn3α234n-II+1-m1msI+I+1/2I+1 .

Step by step solution

01

Definition of spin-orbit coupling.

The connection between the electron's spin and its orbital motion around the nucleus is known as spin-orbit coupling.

02

Step 2: Derivation of equation 6.82.

Write the expression for the relativistic correction of the energy levels.

Er1=En22mc24nI+1/2-3

Write the expression spin- orbit coupling energy.

Hso'=e28πε0.1m2c2r3.S.LEso1=e28πε0.1m2c2r3.S.Lr3

It is known that localid="1658141432913" S.L=ħ2m1msand 1r3=1II+1/2I+1n3a3 Substitute ħ2m1msfor S.Land1II+1/2I+1n3a3for 1r3 in the above expression.

Eso1=e28πε0.1m2c2n3a3.ħm1msII+1/2I+1

Apply the first-order perturbation theory's fine structure adjustment to energy levels.

Efs1=n/mImsHr'n/m1ms+n/mImsHso'n/m1ms=Er1+Eso1=-En22mc24nI+1/2-3+e28πε0.1m2c2n3a3.ħ2m1msII+1/2I+1

Here,a=4πε0ħ2me2.

Efs1=-α24n413.6e.V4nI+1/2-3+α4m2ħe24πε02mImsn3II+1/2I+1=-α24n413.6e.V4nI+1/2-3+α213.6eVmImsn3II+1/2I+1=13.6e.Vn3α2-1I+1/2+34n+mImsIII+1/2I+1

Write the expression for the total energy.

role="math" localid="1658144520537" Efs1=13.6eVn3α234n-II+1-m1msII+1/2I+1

Use the definition of Bohr energy.

role="math" localid="1658144104030" En=-E1n2En=-mc2α22n2-En22mc2=-α213.6eV4n4En2=E12n4

The expression becomes,

E1=-mc2α22E1n4.-mc2α22=--13.6eVmc2α22n4En22mc2=-13.6eVmc2α24n4mc2=-13.6eV4n4α2

Thus, equation 6.82 is derived, that isEfs1=-13.6eVn4α234n-II+1-m1msII+1/2I+1 .

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Most popular questions from this chapter

Two identical spin-zero bosons are placed in an infinite square well (Equation 2.19). They interact weakly with one another, via the potential

V(x1,x2)=-aV0δ(x1-x2). (2.19).

(where V0is a constant with the dimensions of energy, and a is the width of the well).

(a)First, ignoring the interaction between the particles, find the ground state and the first excited state—both the wave functions and the associated energies.

(b) Use first-order perturbation theory to estimate the effect of the particle– particle interaction on the energies of the ground state and the first excited state.

Question: In Problem 4.43you calculated the expectation value ofrsin the stateψ321. Check your answer for the special cases s = 0(trivial), s = -1(Equation 6.55), s = -2(Equation 6.56), and s = -3(Equation 6.64). Comment on the case s = -7.

If I=0, then j=s,mj=ms, and the "good" states are the same (nms)for weak and strong fields. DetermineEz1(from Equation) and the fine structure energies (Equation 6.67), and write down the general result for the I=O Zeeman Effect - regardless of the strength of the field. Show that the strong field formula (Equation 6.82) reproduces this result, provided that we interpret the indeterminate term in square brackets as.

Question: Evaluate the following commutators :

a)[L·S,L]

b)[L·S,S]

c)role="math" localid="1658226147021" [L·S,J]

d)[L·S,L2]

e)[L·S,S2]

f)[L·S,J2]

Hint: L and S satisfy the fundamental commutation relations for angular momentum (Equations 4.99 and 4.134 ), but they commute with each other.

[LX,LY]=ihLz;[Ly,Lz]=ihLx;[Lz,Lx]=ihLy.......4.99[SX,SY]=ihSz;[Sy,Sz]=ihSx;[Sz,Sx]=ihSy........4.134

Suppose the Hamiltonian H, for a particular quantum system, is a function of some parameter λlet En(λ)and ψn(λ)be the eigen values and

Eigen functions of. The Feynman-Hellmann theorem22states that

∂En∂λ=(ψn∂H∂λψn)

(Assuming either that Enis nondegenerate, or-if degenerate-that the ψn's are the "good" linear combinations of the degenerate Eigen functions).

(a) Prove the Feynman-Hellmann theorem. Hint: Use Equation 6.9.

(b) Apply it to the one-dimensional harmonic oscillator,(i)using λ=Ӭ(this yields a formula for the expectation value of V), (II)using λ=ħ(this yields (T)),and (iii)using λ=m(this yields a relation between (T)and (V)). Compare your answers to Problem 2.12, and the virial theorem predictions (Problem 3.31).

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