For a spatial rotation through angle φ about an axis of rotation along a unit vector n, transformations in spinor space are represented by
U=eiφn⋅S/ℏ.
(a) Show using (9.18b) that
U=cosφ/2+i(n⋅σ)sinφ/2.
(b) Using this formula for U and again exploiting the identities for the Pauli matrices, show that
UσU†=n(n⋅σ)−n×[n×σ]cosφ+[n×σ]sinφ.
(c) Discuss the special case n=ez and consider infinitesimal rotations.
(d) Finally, calculate for an arbitrary spinor (α−α+) the transformed spinor defined by
(α+′α−′)=U(α+α−)
for n=ez.