Two particles of mass mare attached to the ends of a massless rigid rod of length a. The system is free to rotate in three dimensions about the center (but the center point itself is fixed).

(a) Show that the allowed energies of this rigid rotor are

En=h2n(n+1)ma2, for n=0,1,2,...

Hint: First express the (classical) energy in terms of the total angular momentum.

(b) What are the normalized Eigen functions for this system? What is the degeneracy of thenthenergy level?

Short Answer

Expert verified
  1. It is shown that En=h2n(n+1)ma2.
  2. The Eigen functions is Ψnmθ,ϕ=Ynmθ,ϕ. The degeneracy of the nth energy level is 2n+1 .

Step by step solution

01

Step 1: Definition of Normalized eigen functions

This isaseries expansion in terms of the "full" collection of orthonormal Eigen functions for the Sturm-Lowville operator with periodic boundary conditions across the interval.

02

(a) Verification of the given equation

Consider two particles of mass are attached to the ends of a massless rigid rod of length . In the absence of potential energy, the system's energy is equal to the kinetic energy of the two particles, i.e.

E=2K=2p22m=p2m...(i)

The particles are only allowed to move in a rotating direction, and the rod's length is fixed, which implies that r is always perpendicular to p, where is the momentum of one of the masses. So,the angular momentum is expressed as follows,

|L|=2|r||p|

Here is the distance from one of the particles to the center of the rod, that is |r|=a/2.

Substitute localid="1658207215926" a2for r .

|L|=2a2p

=apL2=a2p2p2=L2a2

Substitute the above value in equation (i).

E=L2ma2

Write the eigenvalues of h2nn+1 , for n= 0,1,2,.... .

En=h2nn+1ma2

Hence, the given equation is proved.

03

(b) Determination the Normalized eigen functions

Since E is directly proportional to L2, then the Eigen functions are just the ordinary spherical harmonics, that is:

Ψnmθ,ϕ=Ynmθ,ϕ

Here, the degeneracy of the energy level is the number of m values for given n , that is 2n+1 .

Thus, the Eigen functions is determined as Ψnmθ,ϕ=Ynmθ,ϕ and also the degeneracy of the nth energy level is 2n +1 .

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Most popular questions from this chapter

a) Check that Arj1(kr)satisfies the radial equation with V(r)=0and I=1.

(b) Determine graphically the allowed energies for the infinite spherical well, when I=1. Show that for large n,En1(h2π2/2ma2)(n+1/2)2. Hint: First show that j1(x)=0x=tanx. Plot xandtanxon the same graph, and locate the points of intersection.

Work out the radial wave functions R30,R31,andR32using the recursion formula. Don’t bother to normalize them.

(a) If you measured the component of spin angular momentum along the x direction, at time t, what is the probability that you would get +h/2?

(b) Same question, but for the ycomponent.

(c) Same, for the z component.

(a) Work out the Clebsch-Gordan coefficients for the case s1=1/2,s2=anything. Hint: You're looking for the coefficients A and Bin

|sm=A|1212|s2(m-12)+B|12(-12)|s2(m+12)

such that|sm is an eigenstate of . Use the method of Equations 4.179 through 4.182. If you can't figure out whatSx(2) (for instance) does to|s2m2 , refer back to Equation 4.136 and the line before Equation 4.147. Answer:

;role="math" localid="1658209512756" A=s2+12±m2s2+1;B=±s2+12±m2s2+1

where, the signs are determined bys=s2±1/2 .

(b) Check this general result against three or four entries in Table 4.8.

Work out the normalization factor for the spherical harmonics, as follows. From Section 4.1.2we know that

Ylm=BlmeimϕPlmcosθ

the problem is to determine the factor (which I quoted, but did not derive, in Equation 4.32). Use Equations 4.120, 4.121, and 4.130to obtain a recursion

relation giving Blm+1 in terms of Blm. Solve it by induction on to get Blm up to an overall constant Cl, .Finally, use the result of Problem 4.22 to fix the constant. You may find the following formula for the derivative of an associated Legendre function useful:

1-x2dPlmdx=1-x2Plm+1-mxPlm [4.199]

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