Construct the matrixSrrepresenting the component of spin angular momentum along an arbitrary directionr. Use spherical coordinates, for which

rsinθcosΦı+sinθsinΦø+cosθk [4.154]

Find the eigenvalues and (normalized) eigen spinors ofSr. Answer:

x+(r)=(cosθ/2esinθ/2); x+(r)=(esin(θ/2)-cos(θ/2)) [4.155]

Note: You're always free to multiply by an arbitrary phase factor-say,eiϕ-so your answer may not look exactly the same as mine.

Short Answer

Expert verified

The Eigen values and Eigen spinors areabcosθ2eiΦsinθ2andab=eiΦsinθ2cosθ2

Step by step solution

01

Definition of Eigen values and Eigen spinors

Eigenvalues are a unique set of scalar values associated with a set of linear equations, most commonly found in matrix equations.

Characteristic roots are another name for eigenvectors. It's a non-zero vector that can only be altered by its scalar factor once linear transformations are applied.

In quantum physics, Eigen spinors are considered basis vectors that represent a particle's general spin state.

02

Determination of the Eigen values

Use eigenvalues |Sr-λI|=0and find the value the eigenvalues Sr,λ.

ħ2cosθ-λħ2e-iϕsinθħ2e-iϕsinθħ2cosθ-λ=0-ħ4cos2θ+λ2-ħ4sin2θ=0λ2=ħ4sin2θ+cos2θλ2=-ħ4λ=±ħ2Thus,theeigenvaluesofSris±ħ2

03

Determination of the Eigen spinors

Use the eigen-spinor as an exampleab.

S2ab=λab

For λ=ħ2,

localid="1659013250803" ħ2cosθe-iϕsinθe-iϕsinθ-cosθab=ħ2cosθe-iϕsinθe-iϕsinθ-cosθab=ab

Compare the relevant entries on both sides of the matrices.

acosθ+be-iϕsinθ=aaeiϕsinθ-bcosθ=b

Solve the above two equations.

b=a1-cosθe-iϕsinθ=e-iϕ1-cosθasinθ=e-iϕ2sin2θ22sin2θ2cosθ2a=e-iϕsinθ2cosθ2a

For abbecome commonplace,

Apply a2+b2=1.

a2+sin2θ2cos2θ2a2=1

Solve the above expression further.

a2sin2θ2cos2θ2+1=1a2sinθ2+cos2θ2cos2θ2=1a21cosθ2=1a=cosθ2

Substitute the above value in b=eiϕsinθ2cosθ2a.

b=eiϕsinθ2cosθ2cosθ2=eiϕsinθ2

Substitute the values of a, and b in ab.

ab=cosθ2eiϕsinθ2

For λ=-ħ2,

ħ2cosθe-iϕsinθe-iϕsinθ-cosθab=-ħ2abacosθ+be-iϕsinθ=-aaeiϕsinθ-bcosθ=b

Solve the above two equations.

b=-a1+cosθsinθeiϕ=-aeiϕ2cos2θ22sinθ2cosθ2=-aeiϕ2cos2θ22sinθ2cosθ2Applya2+b2

a2+cos2θ2sin2θ2a2=1a21+cos2θ2sin2θ2=1a=e-iΦsinθ2

Substitute the above value inb=-aeiϕcosθ2sinθ2.

b=-e-iΦsinθ2e-iϕcosθ2sinθ2=-eiϕcosθ2

Substitute the values of a, and b in ab.

ab=e-iΦsinθ2-cosθ2

Thus, the eigen values and the eigen spinors are role="math" localid="1659015532483" ab=cosθ2e-iΦsinθ2and

ab=e-iΦsinθ2-cosθ2.

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Most popular questions from this chapter

For the most general normalized spinor (Equation 4.139),

compute{Sx},{Sy},{Sz},{Sx2},{Sy2},and{Sx2}.checkthat{Sx2}+{Sy2}+{Sz2}={S2}.

X=(ab)=aX++bX(4.139).

(a) Prove that for a particle in a potential V(r)the rate of change of the expectation value of the orbital angular momentum L is equal to the expectation value of the torque:

ddt<L>=<N>

Where,

N=r×(VV)

(This is the rotational analog to Ehrenfest's theorem.)

(b) Show that d<L>/dt=0for any spherically symmetric potential. (This is one form of the quantum statement of conservation of angular momentum.)

Coincident spectral lines. 43According to the Rydberg formula (Equation 4.93) the wavelength of a line in the hydrogen spectrum is determined by the principal quantum numbers of the initial and final states. Find two distinct pairs{ni,nf} that yield the same λ. For example,role="math" localid="1656311200820" {6851,6409} and{15283,11687}will do it, but you're not allowed to use those!

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

Work out the spin matrices for arbitrary spin , generalizing spin (Equations 4.145 and 4.147), spin 1 (Problem 4.31), and spin (Problem 4.52). Answer:

Sz=(s0000s-10000s-200000-s)Sx=2(0bs0000bs0bs-10000bs-10bs-20000bs-200000000b-s+10000b-s+10)Sy=2(0-ibs0000ibs0-ibs-10000-ibs-10-ibs-20000-ibs-200000000-ibs+10000-ibs+10)

where,bj(s+j)(s+1-j)
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