Heisenberg Uncertainty Relation
ΔAΔB≥21E[[A^,B^]]
ΔA2ΔB2≥⟨ψ∣2j1[A^,B^]∣ψ⟩2=(2j1E[[A^,B^]])2
Proof
Consider any scalar λ∈C and any Vector ∣u⟩,∣v⟩∈Cn and we have two states ∣f⟩ and ∣g⟩.
We subtract it like so ∣f⟩−λ∣g⟩ is also a vector
Note that for QM systems, ⟨u∣u⟩=1. This is because of Born Rule where the number it represents is the total probability, which needs to sum to 1.
⟨f−λg∣f−λg⟩≥0
⇒⟨f∣f⟩−λ⟨f∣g⟩−λ∗⟨g∣f⟩+(∣λ∣)2⟨g∣g⟩≥0
We want to choose the λ that minimizes the expression.
λ=⟨g∣g⟩⟨g∣f⟩⇒λ∗=⟨g∣g⟩⟨f∣g⟩,∣λ∣2=⟨g∣g⟩2⟨f∣g⟩⟨g∣f⟩
Which makes ∣f⟩−λ∣g⟩ orthogonal to ∣g⟩.
⇒⟨f∣f⟩−⟨g∣g⟩⟨g∣f⟩⟨f∣g⟩−⟨g∣g⟩⟨f∣g⟩⟨g∣f⟩+⟨g∣g⟩2⟨f∣g⟩⟨g∣f⟩⟨g∣g⟩≥0
Note that ⟨g∣f⟩⟨f∣g⟩=∣⟨f∣g⟩∣2
⇒⟨f∣f⟩−⟨g∣g⟩∣⟨f∣g⟩∣2−⟨g∣g⟩∣⟨f∣g⟩∣2+⟨g∣g⟩∣⟨f∣g⟩∣2≥0
⇒⟨f∣f⟩−⟨g∣g⟩∣⟨f∣g⟩∣2≥0
Assuming ⟨g∣g⟩≥0
⇒⟨f∣f⟩⟨g∣g⟩≥∣⟨f∣g⟩∣2
This is Cauchy-Schwarz squared
Consider the Observable that we defined above. This can be written as
∣f⟩=(A^−E[A]I)∣ψ⟩∣g⟩=(B^−E[B]I)∣ψ⟩
Note that ΔA is the Spread of A^.
⟨f∣f⟩=⟨ψ∣(A^−E[A]I)∣ψ⟩
=⟨ψ∣(A^2−2E[A]A^+E[A]2I)∣ψ⟩
=⟨ψ∣A^2∣ψ⟩−2E[A]⟨ψ∣A^∣ψ⟩+E[A]2⟨ψ∣I∣ψ⟩
=E[A^2]−2E[A]2+E[A]2
=E[A^2]−E[A]2
=ΔA2
By symmetry
⟨g∣g⟩=ΔB2
Plug into our equation above
ΔA2ΔB2≥∣⟨f∣g⟩∣2
⇒ΔA2ΔB2≥(Im⟨f∣g⟩)2
⇒ΔA2ΔB2≥(Im(⟨ψ∣(A^−E[A]I)(B^−E[B]I)∣ψ⟩))2
⇒ΔA2ΔB2≥(Im(E[AB]−2E[A]E[B]−+E[A]E[B]))2
⇒ΔA2ΔB2≥(Im(E[AB]−E[A]E[B]))2
Note that Imz=2i1(z−z∗)
⇒ΔA2ΔB2≥(2i1(E[AB]−E[BA]))2
⇒ΔA2ΔB2≥(⟨ψ∣2i1[A^,B^]∣ψ⟩)2