Symmetries and Conservation Laws — David J. Griffiths
Physics — Quantum Mechanics · spin_rotations
Problem
Rotations on spin states are given by an expression identical to Equation 6.32, with the spin angular momentum replacing the orbital angular momentum:
Rn(φ)=exp[−iℏφn⋅S].
In this problem we will consider rotations of a spin-1/2 state.
(a) Show that
(a⋅σ)(b⋅σ)=a⋅b+i(a×b)⋅σ,
where the σi are the Pauli spin matrices and a and b are ordinary vectors. Use the result of Problem 4.29.
(b) Use your result from part (a) to show that
exp[−iℏφn⋅S]=cos(2φ)−isin(2φ)n⋅σ.
Recall that S=(ℏ/2)σ.
(c) Show that your result from part (b) becomes, in the standard basis of spin up and spin down along the z axis, the matrix
Rn=cos(2φ)(1001)−isin(2φ)(cosθsinθeiϕsinθe−iϕ−cosθ)
where θ and ϕ are the polar coordinates of the unit vector n that describes the axis of rotation.
(d) Verify that the matrix Rn in part (c) is unitary.
(e) Compute explicitly the matrix Sx′=R†SxR where R is a rotation by an angle φ about the z axis and verify that it returns the expected result. *Hint*: rewrite your result for Sx′ in terms of Sx and Sy.
(f) Construct the matrix for a π rotation about the x axis and verify that it turns an up spin into a down spin.
(g) Find the matrix describing a 2π rotation about the z axis. Why is this answer surprising?