2025-05-30
Solutions to Principles of Quantum Mechanics
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目录

Chapter 14 Spin
14.1 Introduction
14.2 What is the Nature of Spin?
14.3 Kinematics of Spin
14.4 Spin Dynamics
14.5 Return of Orbital Degrees of Freedom

Chapter 14 Spin

14.1 Introduction

14.2 What is the Nature of Spin?

14.3 Kinematics of Spin

Exercise 14.3.1 Let us verify the above corollary explicitly. Take some spinor with components α=ρ1eiϕ1\alpha=\rho_1 \mathrm{e}^{\mathrm{i} \phi_1} and β=ρ2eiϕ2\beta=\rho_2 \mathrm{e}^{\mathrm{i} \phi_2}. From χχ=1\langle\chi \mid \chi\rangle=1, deduce that we can write ρ1=cos(θ/2)\rho_1=\cos (\theta / 2) and ρ2=sin(θ/2)\rho_2=\sin (\theta / 2) for some θ\theta. Next pull out a common phase factor so that the spinor takes the form in Eq. (14.3.28a). This verifies the corollary and also fixes n^\hat{n}.

Exercise 14.3.2 (1) Show that the eigenvectors of σn^\boldsymbol{\sigma}\cdot\hat{n} are given by Eq. (14.3.28).

(2) Verify Eq. (14.3.29).

Exercise 14.3.3 Using Eqs. (14.3.32) and (14.3.33) show that the Pauli matrices are traceless.

Exercise 14.3.4 Derive Eq. (14.3.39) in two different ways.

(1) Write σ1σ2\sigma_{1}\sigma_{2} in terms of [σi,σj]+[\sigma_{i},\sigma_{j}]_{+} and [σi,σj][\sigma_{i},\sigma_{j}].

(2) Use Eqs. (14.3.42) and (14.3.43).

Exercise 14.3.5 Express the following matrix MM in terms of the Pauli matrices:

M=(αβγδ)M=\begin{pmatrix} \alpha & \beta \\ \gamma & \delta \end{pmatrix}

Exercise 14.3.6 (1) Argue that n^,+=U[R(ϕk)]U[R(θj)]sz=/2|\hat{n},+\rangle=U[R(\phi \mathbf{k})] U[R(\theta \mathbf{j})]\left|s_z=\hbar / 2\right\rangle.

(2) Verify by explicit calculation.

Exercise 14.3.7 Express the following as linear combinations of the Pauli matrices and II:

(1) (I+iσx)1/2\left(I+\mathrm{i} \sigma_x\right)^{1 / 2}. (Relate it to half a certain rotation.)

(2) (2I+σx)1\left(2 I+\sigma_x\right)^{-1}.

(3) σx1\sigma_x^{-1}.

Exercise 14.3.8 (1) Show that any matrix that commutes with σ\boldsymbol{\sigma} is a multiple of the unit matrix.

(2) Show that we cannot find a matrix that anticommutes with all three Pauli matrices. (If such a matrix exists, it must equal zero.)

14.4 Spin Dynamics

Exercise 14.4.1 Show that if H=γLBH=-\gamma \mathbf{L} \cdot \mathbf{B}, and B\mathbf{B} is position independent,

dLdt=μ×B=μ×B\frac{\mathrm{d}\langle\mathbf{L}\rangle}{\mathrm{d} t}=\langle\boldsymbol{\mu} \times \mathbf{B}\rangle=\langle\boldsymbol{\mu}\rangle \times \mathbf{B}

Exercise 14.4.2 Derive (14.4.31) by studying Fig. 14.3.

Exercise 14.4.3 We would like to study here the evolution of a state that starts out as (10)\binom{1}{0} and is subject to the B\mathbf{B} field given in Eq. (14.4.27). This state obeys

iddtψ(t)=Hψ(14.4.34)\mathrm{i} \hbar \frac{\mathrm{d}}{\mathrm{d} t}|\psi(t)\rangle=H|\psi\rangle\tag{14.4.34}

where H=γSBH=-\gamma \mathbf{S} \cdot \mathbf{B}, and B\mathbf{B} is time dependent. Since classical reasoning suggests that in a frame rotating at frequency (ωk-\omega \mathbf{k}) the Hamiltonian should be time independent and governed by Br\mathbf{B}_r [Eq. (14.4.29)], consider the ket in the rotating frame, ψr(t)\left|\psi_r(t)\right\rangle, related to ψ(t)|\psi(t)\rangle by a rotation angle ωt\omega t:

ψr(t)=eiωtSz/ψ(t)(14.4.35)\left|\psi_r(t)\right\rangle=\mathrm{e}^{-\mathrm{i} \omega t S_z / \hbar}|\psi(t)\rangle\tag{14.4.35}

Combine Eqs. (14.4.34) and (14.4.35) to derive Schrödinger's equation for ψr(t)\left|\psi_r(t)\right\rangle in the SzS_z basis and verify that the classical expectation is borne out. Solve for ψr(t)=Ur(t)ψr(0)\left|\psi_r(t)\right\rangle=U_r(t)\left|\psi_r(0)\right\rangle by computing Ur(t)U_r(t), the propagator in the rotating frame. Rotate back to the lab and show that

ψ(t)Sz basis[[cos(ωrt2)+iω0ωωrsin(ωrt2)]e+iωt/2iγBωrsin(ωrt2)eiωt/2](14.4.36)|\psi(t)\rangle \xrightarrow[S_{z}~\text{basis}]{ }\left[\begin{array}{c} {\left[\cos \left(\frac{\omega_r t}{2}\right)+\mathrm{i} \frac{\omega_0-\omega}{\omega_r} \sin \left(\frac{\omega_r t}{2}\right)\right] \mathrm{e}^{+\mathrm{i} \omega t / 2}} \\ \frac{\mathrm{i} \gamma B}{\omega_r} \sin \left(\frac{\omega_r t}{2}\right) \mathrm{e}^{-\mathrm{i} \omega t / 2} \end{array}\right]\tag{14.4.36}

Compare this to the state n^,+|\hat{\mathbf{n}},+\rangle and see what is happening to the spin for the case ω0=ω\omega_0=\omega.

Calculate μz(t)\left\langle\mu_z(t)\right\rangle and verify that it agrees with Eq. (14.4.31).

Exercise 14.4.4 At t=0t=0, an electron is in the state with sz=/2s_z=\hbar/2. A steady field B=Bi\mathbf{B}=B \mathbf{i}, B=100GB=100 \mathrm{G}, is turned on. How many seconds will it take for the spin to flip?

Exercise 14.4.5 We would like to establish the validity of Eq. (14.4.26) when ω\boldsymbol{\omega} and B0\mathbf{B}_0 are not parallel.

(1) Consider a vector V\mathbf{V} in the inertial (nonrotating) frame which changes by ΔV\Delta \mathbf{V} in a time Δt\Delta t. Argue, using the results from Exercise 12.4.3, that the change as seen in a frame rotating at an angular velocity ω\boldsymbol{\omega}, is ΔVω×VΔt\Delta \mathbf{V}-\boldsymbol{\omega} \times \mathbf{V} \Delta t. Obtain a relation between the time derivatives of V\mathbf{V} in the two frames.

(2) Apply this result to the case of l\mathbf{l} [Eq. (14.4.8)], and deduce the formula for the effective field in the rotating frame.

Exercise 14.4.6 (A Density Matrix Problem) (1) Show that the density matrix for an ensemble of spin-1/2 particles may be written as

ρ=12(I+aσ)\rho=\frac{1}{2}(I+\mathbf{a} \cdot \boldsymbol{\sigma})

where a\mathbf{a} is a cc-number vector.

(2) Show that a\mathbf{a} is the mean polarization, σ\langle\overline{\boldsymbol{\sigma}}\rangle.

(3) An ensemble of electrons in a magnetic field B=Bk\mathbf{B}=B \mathbf{k}, is in thermal equilibrium at temperature TT. Construct the density matrix for this ensemble. Calculate μ\langle\overline{\boldsymbol{\mu}}\rangle.

14.5 Return of Orbital Degrees of Freedom

Exercise 14.5.1 (1) Why is the coupling of the proton's intrinsic moment to B an order m/Mm / M correction to Eq. (14.5.4)?

(2) Why is the coupling of its orbital motion an order (m/M)2(m / M)^2 correction? (You may reason classically in both parts.)

Exercise 14.5.2 (1) Estimate the relative size of the level splitting in the n=1n=1 state to the unperturbed energy of the n=1n=1 state, when a field B=1000kG\mathbf{B}=1000 \mathrm{kG} is applied.

(2) Recall that we have been neglecting the order B2B^2 term in HH. Estimate its contribution in the n=1n=1 state relative to the linear (μB-\boldsymbol{\mu} \cdot \mathbf{B}) term we have kept, by assuming the electron moves on a classical orbit of radius a0a_0. Above what B|\mathbf{B}| does it begin to be a poor approximation?

Exercise 14.5.3 A beam of spin-1/2 particles moving along the yy axis goes through two collinear SG apparatuses, both with lower beams blocked. The first has its B field along the zz axis and the second has its B\mathbf{B} field along the xx axis (i.e., is obtained by rotating the first by an angle π/2\pi / 2 about the yy axis). What fraction of particles leaving the first will exit the second? If a third filter that transmits only spin up along the zz axis is introduced, what fraction of particles leaving the first will exit the third? If the middle filter transmits both spins up and down (no blocking) the xx axis, but the last one transmits only spin down the zz axis, what fraction of particles leaving the first will leave the last?

Exercise 14.5.4 A beam of spin-1 particles, moving along the yy axis, is incident on two collinear SG apparatuses, the first with B\mathbf{B} along the zz axis and the second with B\mathbf{B} along the zz^{\prime} axis, which lies in the xzx-z plane at an angle θ\theta relative to the zz axis. Both apparatuses transmit only the uppermost beams. What fraction leaving the first will pass the second?