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Suppose we perturb the infinite cubical well (Equation 6.30) by putting a delta function “bump” at the point(a/4,a/2,3a/4):H'=a3V0δ(x-a/4)δ(y-a/2)δ(z-3a/4).

Find the first-order corrections to the energy of the ground state and the (triply degenerate) first excited states.

Short Answer

Expert verified

The first order correction to the energy of the ground state areWab=8V0sin2(π4)sin(π2)sin(π)sin(3π2)sin(3π4)=0.Wac=8V0sin(π4)sin(π2)sin2(π2)sin(3π2)sin(3π4)=8V0(12)(1)(1)(-1)(12)=-4V0.Wbc=8V0sin(π4)sin(π2)sin(π)sin(π2)sin2(3π4)=0.

Step by step solution

01

Definition of first order correction energy

The anticipated value of the perturbation in the unperturbed state is the first order adjustment to the energy.

02

Finding the first order corrections to the energy of the ground state and the first excited states

Ground state is non degenerate; Eqs. 6.9⇒

En'=ψn0H'ψn0 …(6.9).

localid="1658148464503" E1=2a3a3V0a0sin2πaxsin2πaysin2πazδx-a4δy-a2δz-3a4dxdydz.=8V0sin2π4sin2π2sin23π4=8V012(1)12=2V0

First excited states:

Waa=8V0sin2πaxsin2πaysin22πazδx-a4δy-a2δz-3a4dxdydz.=8V012(1)(1)=4V0.

Wbb=8V0sin2πaxsin22πaysin2πazδx-a4δy-a2δz-3a4dxdydz.=8V012(0)12=0.

Wcc=8V0sin22πaxsin2πaysin2πazδx-a4δy-a2δz-3a4dxdydz.=8V0(1)(1)12=4V0.

Wab=8V0sin2π4sinπ2sin(π)sin3π2sin3π4=0.

Wbc=8V0sinπ4sinπ2sin(π)sinπ2sin23π4=0.

W=4V010-1000-101=4V0D;det(D-λ)=1-λ0-10-λ0-101-λ=-λ(1-λ)2+λ=0

λ=0,or(1-λ)2=11-λ=±1λ=0.

So the first-order corrections to the energies are 0,8V0.

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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.

Van der Waals interaction. Consider two atoms a distanceapart. Because they are electrically neutral you might suppose there would be no force between them, but if they are polarizable there is in fact a weak attraction. To model this system, picture each atom as an electron (mass m , charge -e ) attached by a spring (spring constant k ) to the nucleus (charge +e ), as in Figure. We'll assume the nuclei are heavy, and essentially motionless. The Hamiltonian for the unperturbed system is

H0=12mp12+12kx12+12mp22+12kx22[6.96]

The Coulomb interaction between the atoms is

H'=14πϵ0(e2R-e2R-x1-e2R+x2+e2R-x1+x2 [6.97]

(a) Explain Equation6.97. Assuming that localid="1658203563220" |x1| and |x2|are both much less than, show that

localid="1658203513972" H'-e2x1x22πϵ0R3 [6.98]

(b) Show that the total Hamiltonian (Equationplus Equation) separates into two harmonic oscillator Hamiltonians:

H=[12mp+2+12(k-e22πϵ0R3x+2]+[+12mp-2+12(k+e22πϵ0R3x-2] [6.99]

under the change of variables

x±12(x1±x2) Which entails p±=12(p1±p2) [6.100]

(c) The ground state energy for this Hamiltonian is evidently

E=12(ω++ω-) Where ω±=k(e2/2πϵ0R3)m [6.101]

Without the Coulomb interaction it would have been E0=ħω0, where ω0=k/m. Assuming that, show that

ΔVE-E0-8m2ω03(e22πϵ0)21R6. [6.102]

Conclusion: There is an attractive potential between the atoms, proportional to the inverse sixth power of their separation. This is the van der Waals interaction between two neutral atoms.

(d) Now do the same calculation using second-order perturbation theory. Hint: The unperturbed states are of the form ψn1(x1)ψn2(x2), where ψn(x)is a one-particle oscillator wave function with mass mand spring constant k;ΔVis the second-order correction to the ground state energy, for the perturbation in Equation 6.98 (notice that the first-order correction is zero).

Calculate the wavelength, in centimeters, of the photon emitted under a hyperfine transition in the ground state (n=1) of deuterium. Deuterium is "heavy" hydrogen, with an extra neutron in the nucleus; the proton and neutron bind together to form a deuteron, with spin 1 and magnetic moment

μdl=gde2mdSd

he deuteron g-factor is 1.71.

Estimate the correction to the ground state energy of hydrogen due to the finite size of the nucleus. Treat the proton as a uniformly charged spherical shell of radius b, so the potential energy of an electron inside the shell is constant:-e2/(4πϵ0b);this isn't very realistic, but it is the simplest model, and it will give us the right order of magnitude. Expand your result in powers of the small parameter, (b / a) whereis the Bohr radius, and keep only the leading term, so your final answer takes the form ΔEE=A(b/a)n. Your business is to determine the constant Aand the power n. Finally, put in b10-15m(roughly the radius of the proton) and work out the actual number. How does it compare with fine structure and hyperfine structure?

Question: In the text I asserted that the first-order corrections to an n-fold degenerate energy are the eigen values of the Wmatrix, and I justified this claim as the "natural" generalization of the case n = 2.

Prove it, by reproducing the steps in Section 6.2.1, starting with

ψ0=j=1nαjψj0

(generalizing Equation 6.17), and ending by showing that the analog to Equation6.22 can be interpreted as the eigen value equation for the matrix W.

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