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FOUNDATIONS OF QUANTUM MECHANICS

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III. 6. SPIN 1/2 PARTICLES 67<br />

we have<br />

⃗n · ⃗σ =<br />

( cos θ e<br />

− i ϕ )<br />

sin θ<br />

e i ϕ , (III. 131)<br />

sin θ − cos θ<br />

with eigenvectors<br />

|⃗n, +⟩ =<br />

(<br />

)<br />

e − i 2 ϕ cos 1 2 θ<br />

e i 2 ϕ sin 1 2 θ<br />

and |⃗n, −⟩ =<br />

(<br />

)<br />

− e − i 2 ϕ sin 1 2 θ<br />

e i 2 ϕ cos 1 2 θ<br />

(III. 132)<br />

for eigenvalues ±1.<br />

EXERCISE 22. Verify (III. 132)<br />

III. 6. 1<br />

SPIN 1/2 AND ROTATIONS IN SPIN SPACE<br />

A rotation over an angle α ∈ [0, π) around an axis in the direction of the unit vector ⃗m,<br />

with ⃗m ∈ R 3 , can be written as a unitary matrix<br />

U (⃗m, α) = e − i α ( ⃗m · ⃗J) , (III. 133)<br />

where the total angular momentum J ⃗ = L ⃗ + S ⃗ is the infinitesimal generator of rotations. With L ⃗ = 0<br />

and writing S i = 1 2 σ i, which is, using (III. 124), in accordance to (III. 120) and the still unfounded<br />

(III. 129), the Pauli matrices are the generators of rotations in C 2 , leading to<br />

U (⃗m, α) = e − i 2 α ( ⃗m · ⃗σ) , (III. 134)<br />

where ∥⃗m∥ is again 1. Using Taylor expansions, with (III. 128) we find for (III. 134)<br />

∞∑ (− i) k (⃗m · ⃗σ) k (<br />

U(⃗m, α) =<br />

1<br />

k!<br />

2 α) k<br />

=<br />

k=0<br />

∞∑<br />

k=0<br />

k=even<br />

(− 1) 1 2 k ( 1<br />

k!<br />

2 α) ∑<br />

k ∞ 11 + i (⃗m · ⃗σ)<br />

k=1<br />

k=odd<br />

(− 1) 1 2 (k+1) ( 1<br />

k!<br />

2 α) k<br />

= cos 1 2 α 11 − i (⃗m · ⃗σ) sin 1 2α. (III. 135)<br />

It can be verified that, under a rotation around an axis ⃗m over an angle α, with ⃗n R the unit vector<br />

in the rotated direction, the eigenstates of ⃗n · ⃗σ, (III. 132), transform into the eigenstates of ⃗n R · ⃗σ,<br />

obeying the rotational transformation rules<br />

U (⃗m, α) |⃗n, ±⟩ = |⃗n R , ±⟩. (III. 136)

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