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Problem set 2

These are my solutions to the problem sets assigned to me during the graduate-level quantum mechanics course.

Problem 1

1) Suppose a 2×22\times2 matrix XX (not necessarily Hermitian, nor unitary) is written as X=a0+σ⋅aX=a_{0}+\sigma\cdot\boldsymbol{a}, where a0a_{0} and a1,2,3a_{1,2,3} are numbers.

a) How are a0a_{0} and aka_{k} (k=1,2,3k=1,2,3) related to Tr(X)Tr\left(X\right) and Tr(σkX)Tr\left(\sigma_{k}X\right)?

b) Obtain a0 and ak in terms of the matrix elements Xij.

Tendo então uma matriz XX qualquer de dimensão 2×22\times2 escrita como:

X=(a0+σ→⋅a→)σ0X=\left(a_{0}+\overrightarrow{\sigma}\cdot\overrightarrow{a}\right)\sigma_{0}

Sendo σ→=(σ1,σ2,σ3)\overrightarrow{\sigma}=\left(\sigma_{1},\sigma_{2},\sigma_{3}\right) onde σk\sigma_{k} são as matrizes de Pauli e σ0\sigma_{0} a matriz identidade, e aka_{k} são números (k=0,1,2,3)\left(k=0,1,2,3\right) em que a→=(a1,a2,a3)\overrightarrow{a}=\left(a_{1},a_{2},a_{3}\right), então:

X=(a0+σ1a1+σ2a2+σ3a3)σ0=a0σ0+σ1a1σ0+σ2a2σ0+a3σ3σ0=a0σ0+σ1a1+σ2a2+a3σ3=∑k=03akσk\begin{align*} X= & \left(a_{0}+\sigma_{1}a_{1}+\sigma_{2}a_{2}+\sigma_{3}a_{3}\right)\sigma_{0}\\ = & a_{0}\sigma_{0}+\sigma_{1}a_{1}\sigma_{0}+\sigma_{2}a_{2}\sigma_{0}+a_{3}\sigma_{3}\sigma_{0}\\ = & a_{0}\sigma_{0}+\sigma_{1}a_{1}+\sigma_{2}a_{2}+a_{3}\sigma_{3}\\ = & \sum^{3}_{k=0}a_{k}\sigma_{k} \end{align*}

Pela seguinte propriedade do traçoç Tr(A+B)=Tr(A)+Tr(B)Tr\left(A+B\right)=Tr\left(A\right)+Tr\left(B\right) e Tr(cA)=cTr(A)Tr\left(cA\right)=cTr\left(A\right) onde A,BA,B são matrizes e cc um número complexo, temos que:

Tr(X)=Tr(∑k=03akσk)=∑k=03akTr(σk)\begin{align*} Tr\left(X\right)= & Tr\left(\sum^{3}_{k=0}a_{k}\sigma_{k}\right)\\ = & \sum^{3}_{k=0}a_{k}Tr\left(\sigma_{k}\right) \end{align*}

Lembrando das matrizes de Pauli:

σ0=(1001),σ1=(0110),σ2=(0−ii0),σ3=(100−1)\sigma_{0}=\left(\begin{array}{cc} 1 & 0\\ 0 & 1 \end{array}\right),\sigma_{1}=\left(\begin{array}{cc} 0 & 1\\ 1 & 0 \end{array}\right),\sigma_{2}=\left(\begin{array}{cc} 0 & -i\\ i & 0 \end{array}\right),\sigma_{3}=\left(\begin{array}{cc} 1 & 0\\ 0 & -1 \end{array}\right)

Então temos que:

Tr(σ0)=2Trk≠0(σk)=0Tr\left(\sigma_{0}\right)=2\qquad Tr_{k\neq0}\left(\sigma_{k}\right)=0

Logo:

Tr(X)=2a0Tr\left(X\right)=2a_{0}

Agora precisamos calcular primeiramente (σkX)\left(\sigma_{k}X\right). Usando a relação de produto das matrizesde Pauli: σiσj=δijσ0+iϵijkσk\sigma_{i}\sigma_{j}=\delta_{ij}\sigma_{0}+i\epsilon_{ijk}\sigma_{k}, obtemos:

σiX=σi(∑j=03ajσj)=∑j=03ajσiσj=∑j=03aj(δijσ0+iϵijkσk)=∑j=03(δijajσ0+iϵijkajσk)\begin{align*} \sigma_{i}X= & \sigma_{i}\left(\sum^{3}_{j=0}a_{j}\sigma_{j}\right)\\ = & \sum^{3}_{j=0}a_{j}\sigma_{i}\sigma_{j}\\ = & \sum^{3}_{j=0}a_{j}\left(\delta_{ij}\sigma_{0}+i\epsilon_{ijk}\sigma_{k}\right)\\ = & \sum^{3}_{j=0}\left(\delta_{ij}a_{j}\sigma_{0}+i\epsilon_{ijk}a_{j}\sigma_{k}\right) \end{align*}

De acordo com a condições propostas no enunciado temos que i=1,2,3i=1,2,3, tirando o traço então:

Tr(σiX)=∑j=03(δijajTr(σ0)+iϵijkajTr(σk))=∑j=03δij2aj=2ai\begin{align*} Tr\left(\sigma_{i}X\right)= & \sum^{3}_{j=0}\left(\delta_{ij}a_{j}Tr\left(\sigma_{0}\right)+i\epsilon_{ijk}a_{j}Tr\left(\sigma_{k}\right)\right)\\ = & \sum^{3}_{j=0}\delta_{ij}2a_{j}\\ = & 2a_{i} \end{align*}

Temos então as seguintes relações:

Tr(X)=2a0Tr(σkX)=2akTr\left(X\right)=2a_{0}\qquad Tr\left(\sigma_{k}X\right)=2a_{k}

b)

Dos resultados anteriores sabemos que:

a0=Tr(X)2ak=Tr(σkX)2a_{0}=\frac{Tr\left(X\right)}{2}\qquad a_{k}=\frac{Tr\left(\sigma_{k}X\right)}{2}

Escrevendo então XX explícitamente de forma genérica como:

X=(X11X12X21X22)X=\left(\begin{array}{cc} X_{11} & X_{12}\\ X_{21} & X_{22} \end{array}\right)

Pode-se perceber que:

a0=Tr(X)2=X11+X222a_{0}=\frac{Tr\left(X\right)}{2}=\frac{X_{11}+X_{22}}{2}

E calculando o produto das matrizes:

σ1X=(0110)(X11X12X21X22)=(X21X22X11X12)σ2X=(0−ii0)(X11X12X21X22)=(−iX21−iX22iX11iX12)σ1X=(100−1)(X11X12X21X22)=(X11X12−X21−X22)\begin{alignat}{2} \sigma_{1}X= & \left(\begin{array}{cc} 0 & 1\\ 1 & 0 \end{array}\right)\left(\begin{array}{cc} X_{11} & X_{12}\\ X_{21} & X_{22} \end{array}\right)= & \left(\begin{array}{cc} X_{21} & X_{22}\\ X_{11} & X_{12} \end{array}\right)\\ \sigma_{2}X= & \left(\begin{array}{cc} 0 & -i\\ i & 0 \end{array}\right)\left(\begin{array}{cc} X_{11} & X_{12}\\ X_{21} & X_{22} \end{array}\right)= & \left(\begin{array}{cc} -iX_{21} & -iX_{22}\\ iX_{11} & iX_{12} \end{array}\right)\\ \sigma_{1}X= & \left(\begin{array}{cc} 1 & 0\\ 0 & -1 \end{array}\right)\left(\begin{array}{cc} X_{11} & X_{12}\\ X_{21} & X_{22} \end{array}\right)= & \left(\begin{array}{cc} X_{11} & X_{12}\\ -X_{21} & -X_{22} \end{array}\right) \end{alignat}

Logo, podemos obter quase que diretamente:

a1=12Tr(σ1X)=X21+X122a2=12Tr(σ2X)=iX12−X212a3=12Tr(σ3X)=X11−X222\begin{alignat}{2} a_{1}= & \frac{1}{2}Tr\left(\sigma_{1}X\right)= & \frac{X_{21}+X_{12}}{2}\\ a_{2}= & \frac{1}{2}Tr\left(\sigma_{2}X\right)= & i\frac{X_{12}-X_{21}}{2}\\ a_{3}= & \frac{1}{2}Tr\left(\sigma_{3}X\right)= & \frac{X_{11}-X_{22}}{2} \end{alignat}

Problem 2

The Hamiltonian operator for a two-state system is given by

H=a(∣1⟩⟨1∣−∣2⟩⟨2∣+∣1⟩⟨2∣+∣2⟩⟨1∣)H=a\left(\left|1\right\rangle \left\langle 1\right|-\left|2\right\rangle \left\langle 2\right|+\left|1\right\rangle \left\langle 2\right|+\left|2\right\rangle \left\langle 1\right|\right)

where aa is a number with the dimension of energy. Find the energy eigenvalues and the corresponding energy eigenkets (as linear combinations of ∣1⟩\left|1\right\rangle and ∣2⟩\left|2\right\rangle).

Temos o seguinte hamiltoniano para um sistema de dois estados:

H=a(∣1⟩⟨1∣−∣2⟩⟨2∣+∣1⟩⟨2∣+∣2⟩⟨1∣)H=a\left(\left|1\right\rangle \left\langle 1\right|-\left|2\right\rangle \left\langle 2\right|+\left|1\right\rangle \left\langle 2\right|+\left|2\right\rangle \left\langle 1\right|\right)

Sendo ∣1⟩=(10)T\left|1\right\rangle =\left(\begin{array}{cc} 1 & 0\end{array}\right)^{T} e ∣2⟩=(01)T\left|2\right\rangle =\left(\begin{array}{cc} 0 & 1\end{array}\right)^{T}, então o hamiltoniano é representado matricialmente como:

H=a[(10)(10)−(01)(01)+(10)(01)+(01)(10)]=a[(1000)−(0001)+(0100)+(0010)]=a(111−1)\begin{align*} H= & a\left[\left(\begin{array}{c} 1\\ 0 \end{array}\right)\left(\begin{array}{cc} 1 & 0\end{array}\right)-\left(\begin{array}{c} 0\\ 1 \end{array}\right)\left(\begin{array}{cc} 0 & 1\end{array}\right)+\left(\begin{array}{c} 1\\ 0 \end{array}\right)\left(\begin{array}{cc} 0 & 1\end{array}\right)+\left(\begin{array}{c} 0\\ 1 \end{array}\right)\left(\begin{array}{cc} 1 & 0\end{array}\right)\right]\\ = & a\left[\left(\begin{array}{cc} 1 & 0\\ 0 & 0 \end{array}\right)-\left(\begin{array}{cc} 0 & 0\\ 0 & 1 \end{array}\right)+\left(\begin{array}{cc} 0 & 1\\ 0 & 0 \end{array}\right)+\left(\begin{array}{cc} 0 & 0\\ 1 & 0 \end{array}\right)\right]\\ = & a\left(\begin{array}{cc} 1 & 1\\ 1 & -1 \end{array}\right) \end{align*}

Os autovalores são então dados pela raíz do determinante:

∣H−λI∣=∣a−λaa−(a+λ)∣=00=−(a−λ)(a+λ)−a20=−(a2−λ2)−a20=−a2+λ2−a20=−2a2+λ2λ2=2a2λ=±a2\begin{align*} \left|H-\lambda\mathbb{I}\right|= & \left|\begin{array}{cc} a-\lambda & a\\ a & -\left(a+\lambda\right) \end{array}\right|=0\\ 0= & -\left(a-\lambda\right)\left(a+\lambda\right)-a^{2}\\ 0= & -\left(a^{2}-\lambda^{2}\right)-a^{2}\\ 0= & -a^{2}+\lambda^{2}-a^{2}\\ 0= & -2a^{2}+\lambda^{2}\\ \lambda^{2}= & 2a^{2}\\ \lambda & =\pm a\sqrt{2} \end{align*}

Calculando então o autovetor para λ+=a2\lambda_{+}=a\sqrt{2}, temos que:

(H−λI)∣λ+⟩=0(a(1−2)aa−a(1+2))(x1x2)=(00)\begin{align*} \left(H-\lambda\mathbb{I}\right)\left|\lambda_{+}\right\rangle & =\boldsymbol{0}\\ \left(\begin{array}{cc} a\left(1-\sqrt{2}\right) & a\\ a & -a\left(1+\sqrt{2}\right) \end{array}\right) & \left(\begin{array}{c} x_{1}\\ x_{2} \end{array}\right)=\left(\begin{array}{c} 0\\ 0 \end{array}\right) \end{align*}

Como:

−a(1+2)⋅(1−2)=−a(1−2)=a-a\left(1+\sqrt{2}\right)\cdot\left(1-\sqrt{2}\right)=-a\left(1-2\right)=a

As linhas são linearmente dependentes. Então da primeira linha podemos obter que:

0=a(1−2)x1+ax20=(1−2)x1+x2x2=(2−1)x1\begin{align*} 0 & =a\left(1-\sqrt{2}\right)x_{1}+ax_{2}\\ 0 & =\left(1-\sqrt{2}\right)x_{1}+x_{2}\\ x_{2} & =\left(\sqrt{2}-1\right)x_{1} \end{align*}

Logo o autovetor normalizado pode ser escrito:

∣λ+⟩=(x1∣1⟩+(2−1)x1∣2⟩)x12+(2−1)2x12\left|\lambda_{+}\right\rangle =\frac{\left(x_{1}\left|1\right\rangle +\left(\sqrt{2}-1\right)x_{1}\left|2\right\rangle \right)}{\sqrt{x^{2}_{1}+\left(\sqrt{2}-1\right)^{2}x^{2}_{1}}}

Escolhendo x1=1x_{1}=1:

∣λ+⟩=(∣1⟩+(2−1)∣2⟩)1+2−22+1=14−22(∣1⟩+(2−1)∣2⟩)\left|\lambda_{+}\right\rangle =\frac{\left(\left|1\right\rangle +\left(\sqrt{2}-1\right)\left|2\right\rangle \right)}{\sqrt{1+2-2\sqrt{2}+1}}=\frac{1}{\sqrt{4-2\sqrt{2}}}\left(\left|1\right\rangle +\left(\sqrt{2}-1\right)\left|2\right\rangle \right)

E para λ−=−a2\lambda_{-}=-a\sqrt{2}, temos que:

(H−λI)∣λ+⟩=0(a(1+2)aaa(2−1))(x1x2)=(00)\begin{align*} \left(H-\lambda\mathbb{I}\right)\left|\lambda_{+}\right\rangle & =\boldsymbol{0}\\ \left(\begin{array}{cc} a\left(1+\sqrt{2}\right) & a\\ a & a\left(\sqrt{2}-1\right) \end{array}\right) & \left(\begin{array}{c} x_{1}\\ x_{2} \end{array}\right)=\left(\begin{array}{c} 0\\ 0 \end{array}\right) \end{align*}

Como:

−a(1+2)⋅(1−2)=−a(1−2)=a-a\left(1+\sqrt{2}\right)\cdot\left(1-\sqrt{2}\right)=-a\left(1-2\right)=a

As linhas novamente são linearmente dependentes. De modo análogo:

0=a(1+2)x1+ax20=(1+2)x1+x2x2=−(1+2)x1\begin{align*} 0 & =a\left(1+\sqrt{2}\right)x_{1}+ax_{2}\\ 0 & =\left(1+\sqrt{2}\right)x_{1}+x_{2}\\ x_{2} & =-\left(1+\sqrt{2}\right)x_{1} \end{align*}

Logo o autovetor normalizado pode ser escrito:

∣λ−⟩=(x1∣1⟩−(1+2)x1∣2⟩)x12+(2+1)2x12\left|\lambda_{-}\right\rangle =\frac{\left(x_{1}\left|1\right\rangle -\left(1+\sqrt{2}\right)x_{1}\left|2\right\rangle \right)}{\sqrt{x^{2}_{1}+\left(\sqrt{2}+1\right)^{2}x^{2}_{1}}}

Escolhendo x1=1x_{1}=1:

∣λ−⟩=(∣1⟩−(2+1)∣2⟩)1+2+22+1=14+22(∣1⟩−(2+1)∣2⟩)\left|\lambda_{-}\right\rangle =\frac{\left(\left|1\right\rangle -\left(\sqrt{2}+1\right)\left|2\right\rangle \right)}{\sqrt{1+2+2\sqrt{2}+1}}=\frac{1}{\sqrt{4+2\sqrt{2}}}\left(\left|1\right\rangle -\left(\sqrt{2}+1\right)\left|2\right\rangle \right)

Desta forma, reescrevendo os autovetores utilizando um resultado numérico, obtemos que:

∣λ+⟩=0.92∣1⟩+0.38∣2⟩∣λ+⟩=0.38∣1⟩−0.92∣2⟩\left|\lambda_{+}\right\rangle =0.92\left|1\right\rangle +0.38\left|2\right\rangle \qquad\left|\lambda_{+}\right\rangle =0.38\left|1\right\rangle -0.92\left|2\right\rangle

Problem 3

A certain observable in quantum mechanics has a 3×33\times3 matrix representation as follows:

12(010101010)\frac{1}{\sqrt{2}}\left(\begin{array}{ccc} 0 & 1 & 0\\ 1 & 0 & 1\\ 0 & 1 & 0 \end{array}\right)

a) Find the normalized eigenvectors of this observable and the corresponding eigenvalues. Is there any degeneracy?

b) Give a physical example where all this is relevant.

Temos a seguinte matriz:

12(010101010)\frac{1}{\sqrt{2}}\left(\begin{array}{ccc} 0 & 1 & 0\\ 1 & 0 & 1\\ 0 & 1 & 0 \end{array}\right)

Calculando entao os autovalores:

∣−λ12012−λ12012−λ∣=(−λ3+λ4)=(000)\left|\begin{array}{ccc} -\lambda & \frac{1}{\sqrt{2}} & 0\\ \frac{1}{\sqrt{2}} & -\lambda & \frac{1}{\sqrt{2}}\\ 0 & \frac{1}{\sqrt{2}} & -\lambda \end{array}\right|=\left(-\lambda^{3}+\frac{\lambda}{4}\right)=\left(\begin{array}{c} 0\\ 0\\ 0 \end{array}\right)

A partir da seguinte equação de segundo grau −λ(λ2−1)=0-\lambda\left(\lambda^{2}-1\right)=0, obtemos os autovalores λ1=0\lambda_{1}=0 e λ2,3=±1\lambda_{2,3}=\pm1. Desta forma já podemos concluir que não há autovalores degenerados. Para o primeiro autovalor:

(0120120120120)(x1x2x3)=(000)\left(\begin{array}{ccc} 0 & \frac{1}{\sqrt{2}} & 0\\ \frac{1}{\sqrt{2}} & 0 & \frac{1}{\sqrt{2}}\\ 0 & \frac{1}{\sqrt{2}} & 0 \end{array}\right)\left(\begin{array}{c} x_{1}\\ x_{2}\\ x_{3} \end{array}\right)=\left(\begin{array}{c} 0\\ 0\\ 0 \end{array}\right)

Da primeira e última linha temos que x2=0x_{2}=0. E da segunda linha que x1=−x3x_{1}=-x_{3}. Então para garantir a normalização escolhendo x1=12x_{1}=\frac{1}{\sqrt{2}}:

∣λ1⟩=(−12012)T\begin{align*} \left|\lambda_{1}\right\rangle & =\left(\begin{array}{ccc} -\frac{1}{\sqrt{2}} & 0 & \frac{1}{\sqrt{2}}\end{array}\right)^{T} \end{align*}

De modo análogo para λ2=1\lambda_{2}=1:

(−112012−112012−1)(x1x2x3)=(000)\left(\begin{array}{ccc} -1 & \frac{1}{\sqrt{2}} & 0\\ \frac{1}{\sqrt{2}} & -1 & \frac{1}{\sqrt{2}}\\ 0 & \frac{1}{\sqrt{2}} & -1 \end{array}\right)\left(\begin{array}{c} x_{1}\\ x_{2}\\ x_{3} \end{array}\right)=\left(\begin{array}{c} 0\\ 0\\ 0 \end{array}\right)

Da primeira linha −x1+x22=0-x_{1}+\frac{x_{2}}{\sqrt{2}}=0 ou x1=x22x_{1}=\frac{x_{2}}{\sqrt{2}}. Fazendo análogo, da terceira linha obtemos que x22−x3=0\frac{x_{2}}{\sqrt{2}}-x_{3}=0, então x3=x22x_{3}=\frac{x_{2}}{\sqrt{2}}. Subtituindo ambos na segunda linha então:

12(x22)−x2+12(x22)=0x22−x2+x22=0(1−1)x2=0\begin{align*} \frac{1}{\sqrt{2}}\left(\frac{x_{2}}{\sqrt{2}}\right)-x_{2}+\frac{1}{\sqrt{2}}\left(\frac{x_{2}}{\sqrt{2}}\right) & =0\\ \frac{x_{2}}{2}-x_{2}+\frac{x_{2}}{2} & =0\\ \left(1-1\right)x_{2} & =0 \end{align*}

Então x2x_{2} pode ser qualquer valor. Isto é esperado uma vez que a segunda linha (L2L2) pode ser escrito como uma combinaçaõ linear das outras linhas (L2=−12(L1+L3))\left(L_{2}=-\frac{1}{\sqrt{2}}\left(L_{1}+L_{3}\right)\right). Escolhendo x2=2x_{2}=\sqrt{2} para facilitar, e normalizando, ficamos com

∣λ2⟩11+2+1(121)T∣λ2⟩=12(121)T\begin{align*} \left|\lambda_{2}\right\rangle & \frac{1}{\sqrt{1+2+1}}\left(\begin{array}{ccc} 1 & \sqrt{2} & 1\end{array}\right)^{T}\\ \left|\lambda_{2}\right\rangle & =\frac{1}{2}\left(\begin{array}{ccc} 1 & \sqrt{2} & 1\end{array}\right)^{T} \end{align*}

E por fim λ3=−1\lambda_{3}=-1:

(1120121120121)(x1x2x3)=(000)\left(\begin{array}{ccc} 1 & \frac{1}{\sqrt{2}} & 0\\ \frac{1}{\sqrt{2}} & 1 & \frac{1}{\sqrt{2}}\\ 0 & \frac{1}{\sqrt{2}} & 1 \end{array}\right)\left(\begin{array}{c} x_{1}\\ x_{2}\\ x_{3} \end{array}\right)=\left(\begin{array}{c} 0\\ 0\\ 0 \end{array}\right)

Então da primeira linha x1+x22=0x_{1}+\frac{x_{2}}{\sqrt{2}}=0 ou x1=−x22x_{1}=-\frac{x_{2}}{\sqrt{2}}. Fazendo análogo, da terceira linha obtemos que x22+x3=0\frac{x_{2}}{\sqrt{2}}+x_{3}=0, então x3=−x22x_{3}=-\frac{x_{2}}{\sqrt{2}}. Subtituindo ambos na segunda linha então:

12(−x22)+x2+12(−x22)=0−x22+x2−x22=0(1−1)x2=0\begin{align*} \frac{1}{\sqrt{2}}\left(-\frac{x_{2}}{\sqrt{2}}\right)+x_{2}+\frac{1}{\sqrt{2}}\left(-\frac{x_{2}}{\sqrt{2}}\right) & =0\\ -\frac{x_{2}}{2}+x_{2}-\frac{x_{2}}{2} & =0\\ \left(1-1\right)x_{2} & =0 \end{align*}

Em situação análoga ao caso anterior, escolhemos: x2=−2x_{2}=-\sqrt{2} para facilitar, e normalizando, temos:

∣λ3⟩11+2+1(1−21)T∣λ3⟩=12(1−21)T\begin{align*} \left|\lambda_{3}\right\rangle & \frac{1}{\sqrt{1+2+1}}\left(\begin{array}{ccc} 1 & -\sqrt{2} & 1\end{array}\right)^{T}\\ \left|\lambda_{3}\right\rangle & =\frac{1}{2}\left(\begin{array}{ccc} 1 & -\sqrt{2} & 1\end{array}\right)^{T} \end{align*}

Logo os autovetores são:

∣λ1⟩=(−120+12)∣λ2⟩=12(121)∣λ3⟩=12(1−21)\left|\lambda_{1}\right\rangle =\left(\begin{array}{c} -\frac{1}{\sqrt{2}}\\ 0\\ +\frac{1}{\sqrt{2}} \end{array}\right)\qquad\left|\lambda_{2}\right\rangle =\frac{1}{2}\left(\begin{array}{c} 1\\ \sqrt{2}\\ 1 \end{array}\right)\qquad\left|\lambda_{3}\right\rangle =\frac{1}{2}\left(\begin{array}{c} 1\\ -\sqrt{2}\\ 1 \end{array}\right)

b)

Com a diferença de uma constante, esta matriz pode ser usada para representar o momento angular com spin unitário na direção xx. Isto é possível pois junto com outras 2 ela faz parte de um grupo de objetos que satisfazem as relações de comutação para o momento angular, seja o momento angular orbital LxL_{x} ou o de spin SxS_{x}, que são as notações normalmente empregas para se referir esta matriz. A constante multiplicativa tem o único efeito de multiplicar os autovalores da matriz, mantendo os mesmos autovetores. Portanto este é um exemplo físico onde tudo desenvolvido nesta questão é relevante.

Problem 4

Find the linear combination of ∣+⟩\left|+\right\rangle and ∣−⟩\left|-\right\rangle kets that maximizes the uncertainty product

⟨(ΔSx)2⟩⟨(ΔSy)2⟩\left\langle \left(\Delta S_{x}\right)^{2}\right\rangle \left\langle \left(\Delta S_{y}\right)^{2}\right\rangle

Verify explicity that for the linear combination you found, the uncertainty relation for SxS_{x} and SyS_{y} is not violated.

Um estado qualquer formado pela combinação dos vetores ∣+⟩\left|+\right\rangle e ∣−⟩\left|-\right\rangle pode ser representado genericamente por:

∣α⟩=a∣+⟩+beiβ∣−⟩\left|\alpha\right\rangle =a\left|+\right\rangle +be^{i\beta}\left|-\right\rangle

Onde aa e bb são números reais e obedecem a condição de normalização: a2+b2=1a^{2}+b^{2}=1. Qyeremos maximizar a incerteza do produto:

⟨(ΔSx)2⟩⟨(ΔSy)2⟩\left\langle \left(\Delta S_{x}\right)^{2}\right\rangle \left\langle \left(\Delta S_{y}\right)^{2}\right\rangle

Os operadores SxS_{x}e SyS_{y} são dados por:

Sx=ℏ2(∣+⟩⟨−∣+∣−⟩⟨+∣)Sy=iℏ2(−∣+⟩⟨−∣+∣−⟩⟨+∣)S_{x}=\frac{\hbar}{2}\left(\left|+\right\rangle \left\langle -\right|+\left|-\right\rangle \left\langle +\right|\right)\qquad S_{y}=\frac{i\hbar}{2}\left(-\left|+\right\rangle \left\langle -\right|+\left|-\right\rangle \left\langle +\right|\right)

Lembrando que:

⟨(ΔSi)2⟩≡⟨Si2⟩−⟨Si⟩2⟨Si⟩=⟨α∣Si∣α⟩\left\langle \left(\Delta S_{i}\right)^{2}\right\rangle \equiv\left\langle S^{2}_{i}\right\rangle -\left\langle S_{i}\right\rangle ^{2}\qquad\left\langle S_{i}\right\rangle =\left\langle \alpha\left|S_{i}\right|\alpha\right\rangle

Começando então calculando Si2S^{2}_{i}, lembrando que I=∣+⟩⟨+∣+∣−⟩⟨−∣\mathbb{I}=\left|+\right\rangle \left\langle +\right|+\left|-\right\rangle \left\langle -\right|:

Sx2=ℏ2(∣+⟩⟨−∣+∣−⟩⟨+∣)ℏ2(∣+⟩⟨−∣+∣−⟩⟨+∣)=ℏ24(∣+⟩⟨−∣+⟩⟨−∣+∣+⟩⟨−∣−⟩⟨+∣+∣−⟩⟨+∣+⟩⟨−∣+∣−⟩⟨+∣−⟩⟨+∣)=ℏ24(∣+⟩⟨+∣+∣−⟩⟨−∣)=ℏ24\begin{align*} S^{2}_{x} & =\frac{\hbar}{2}\left(\left|+\right\rangle \left\langle -\right|+\left|-\right\rangle \left\langle +\right|\right)\frac{\hbar}{2}\left(\left|+\right\rangle \left\langle -\right|+\left|-\right\rangle \left\langle +\right|\right)\\ & =\frac{\hbar^{2}}{4}\left(\left|+\right\rangle \left\langle -|+\right\rangle \left\langle -\right|+\left|+\right\rangle \left\langle -|-\right\rangle \left\langle +\right|+\left|-\right\rangle \left\langle +|+\right\rangle \left\langle -\right|+\left|-\right\rangle \left\langle +|-\right\rangle \left\langle +\right|\right)\\ & =\frac{\hbar^{2}}{4}\left(\left|+\right\rangle \left\langle +\right|+\left|-\right\rangle \left\langle -\right|\right)\\ & =\frac{\hbar^{2}}{4} \end{align*}

E:

Sy2=iℏ2(−∣+⟩⟨−∣+∣−⟩⟨+∣)iℏ2(−∣+⟩⟨−∣+∣−⟩⟨+∣)=−ℏ24[+∣+⟩⟨−∣+⟩⟨−∣−∣+⟩⟨−∣−⟩⟨+∣−∣−⟩⟨+∣+⟩⟨−∣+∣−⟩⟨+∣−⟩⟨+∣]=−ℏ24[−∣+⟩⟨+∣−∣−⟩⟨−∣]=ℏ24[∣+⟩⟨+∣+∣−⟩⟨−∣]=ℏ24\begin{align*} S^{2}_{y} & =\frac{i\hbar}{2}\left(-\left|+\right\rangle \left\langle -\right|+\left|-\right\rangle \left\langle +\right|\right)\frac{i\hbar}{2}\left(-\left|+\right\rangle \left\langle -\right|+\left|-\right\rangle \left\langle +\right|\right)\\ & =-\frac{\hbar^{2}}{4}\left[+\left|+\right\rangle \left\langle -|+\right\rangle \left\langle -\right|-\left|+\right\rangle \left\langle -|-\right\rangle \left\langle +\right|-\left|-\right\rangle \left\langle +|+\right\rangle \left\langle -\right|+\left|-\right\rangle \left\langle +|-\right\rangle \left\langle +\right|\right]\\ & =-\frac{\hbar^{2}}{4}\left[-\left|+\right\rangle \left\langle +\right|-\left|-\right\rangle \left\langle -\right|\right]\\ & =\frac{\hbar^{2}}{4}\left[\left|+\right\rangle \left\langle +\right|+\left|-\right\rangle \left\langle -\right|\right]\\ & =\frac{\hbar^{2}}{4} \end{align*}

Logo, temos que Sx2=Sy2=ℏ24=S2S^{2}_{x}=S^{2}_{y}=\frac{\hbar^{2}}{4}=S^{2}, sendo que S=ℏ24S=\frac{\hbar^{2}}{4} é uma constante. Então para o primeiro termo da relação de dispersão, independentemente se SxS_{x} ou SyS_{y}, temos:

⟨S2⟩=⟨α∣S2∣α⟩=⟨α∣ℏ24∣α⟩=ℏ24⟨α∣α⟩=ℏ24\begin{align*} \left\langle S^{2}\right\rangle & =\left\langle \alpha\left|S^{2}\right|\alpha\right\rangle =\left\langle \alpha\left|\frac{\hbar^{2}}{4}\right|\alpha\right\rangle =\frac{\hbar^{2}}{4}\left\langle \alpha|\alpha\right\rangle =\frac{\hbar^{2}}{4} \end{align*}

E para o segundo termo:

⟨α∣Si∣α⟩=(⟨+∣a+⟨−∣be−iβ)Si(a∣+⟩+beiβ∣−⟩)=a2⟨+∣Si∣+⟩+abeiβ⟨+∣Si∣−⟩+abe−iβ⟨−∣Si∣+⟩+b2⟨−∣Si∣−⟩\begin{align*} \left\langle \alpha\left|S_{i}\right|\alpha\right\rangle & =\left(\left\langle +\right|a+\left\langle -\right|be^{-i\beta}\right)S_{i}\left(a\left|+\right\rangle +be^{i\beta}\left|-\right\rangle \right)\\ & =a^{2}\left\langle +\right|S_{i}\left|+\right\rangle +abe^{i\beta}\left\langle +\right|S_{i}\left|-\right\rangle +abe^{-i\beta}\left\langle -\right|S_{i}\left|+\right\rangle +b^{2}\left\langle -\right|S_{i}\left|-\right\rangle \end{align*}

Para SxS_{x}:

⟨α∣Sx∣α⟩=ℏ2(a2⟨+∣(∣+⟩⟨−∣+∣−⟩⟨+∣)∣+⟩+abeiβ⟨+∣(∣+⟩⟨−∣+∣−⟩⟨+∣)∣−⟩+ab⟨−∣(∣+⟩⟨−∣+∣−⟩⟨+∣)∣+⟩e−iβ+b2⟨−∣(∣+⟩⟨−∣+∣−⟩⟨+∣)∣−⟩)=ℏ2(a2(⟨+∣+⟩⟨−∣+⟩+⟨+∣−⟩⟨+∣+⟩)+abeiβ(⟨+∣+⟩⟨−∣−⟩+⟨+∣−⟩⟨+∣−⟩)+ab(⟨−∣+⟩⟨−∣+⟩+⟨−∣−⟩⟨+∣+⟩)e−iβ+b2(⟨−∣+⟩⟨−∣−⟩+⟨−∣−⟩⟨+∣−⟩))=ℏ2(abeiβ+abe−iβ)=ℏab(eiβ+e−iβ)2=ℏabcos⁡β\begin{align*} \left\langle \alpha\left|S_{x}\right|\alpha\right\rangle = & \frac{\hbar}{2}\left(a^{2}\left\langle +\right|\left(\left|+\right\rangle \left\langle -\right|+\left|-\right\rangle \left\langle +\right|\right)\left|+\right\rangle +abe^{i\beta}\left\langle +\right|\left(\left|+\right\rangle \left\langle -\right|+\left|-\right\rangle \left\langle +\right|\right)\left|-\right\rangle +\right.\\ & \left.ab\left\langle -\right|\left(\left|+\right\rangle \left\langle -\right|+\left|-\right\rangle \left\langle +\right|\right)\left|+\right\rangle e^{-i\beta}+b^{2}\left\langle -\right|\left(\left|+\right\rangle \left\langle -\right|+\left|-\right\rangle \left\langle +\right|\right)\left|-\right\rangle \right)\\ = & \frac{\hbar}{2}\left(a^{2}\left(\left\langle +|+\right\rangle \left\langle -|+\right\rangle +\left\langle +|-\right\rangle \left\langle +|+\right\rangle \right)+abe^{i\beta}\left(\left\langle +|+\right\rangle \left\langle -|-\right\rangle +\left\langle +|-\right\rangle \left\langle +|-\right\rangle \right)+\right.\\ & \left.ab\left(\left\langle -|+\right\rangle \left\langle -|+\right\rangle +\left\langle -|-\right\rangle \left\langle +|+\right\rangle \right)e^{-i\beta}+b^{2}\left(\left\langle -|+\right\rangle \left\langle -|-\right\rangle +\left\langle -|-\right\rangle \left\langle +|-\right\rangle \right)\right)\\ = & \frac{\hbar}{2}\left(abe^{i\beta}+abe^{-i\beta}\right)\\ = & \hbar ab\frac{\left(e^{i\beta}+e^{-i\beta}\right)}{2}\\ = & \hbar ab\cos\beta \end{align*}

Para SyS_{y}:

⟨α∣Sy∣α⟩=iℏ2(a2⟨+∣(−∣+⟩⟨−∣+∣−⟩⟨+∣)∣+⟩+abeiβ⟨+∣(−∣+⟩⟨−∣+∣−⟩⟨+∣)∣−⟩+ab⟨−∣(−∣+⟩⟨−∣+∣−⟩⟨+∣)∣+⟩e−iβ+b2⟨−∣(−∣+⟩⟨−∣+∣−⟩⟨+∣)∣−⟩)=iℏ2(a2(−⟨+∣+⟩⟨−∣+⟩+⟨+∣−⟩⟨+∣+⟩)+abeiβ(−⟨+∣+⟩⟨−∣−⟩+⟨+∣−⟩⟨+∣−⟩)+ab(−⟨−∣+⟩⟨−∣+⟩+⟨−∣−⟩⟨+∣+⟩)e−iβ+b2(−⟨−∣+⟩⟨−∣−⟩+⟨−∣−⟩⟨+∣−⟩))=iℏ2(−abeiβ+abe−iβ)=ℏabi(−eiβ+e−iβ)2=ℏab(eiβ−e−iβ)2i=ℏabsin⁡β\begin{align*} \left\langle \alpha\left|S_{y}\right|\alpha\right\rangle = & \frac{i\hbar}{2}\left(a^{2}\left\langle +\right|\left(-\left|+\right\rangle \left\langle -\right|+\left|-\right\rangle \left\langle +\right|\right)\left|+\right\rangle +abe^{i\beta}\left\langle +\right|\left(-\left|+\right\rangle \left\langle -\right|+\left|-\right\rangle \left\langle +\right|\right)\left|-\right\rangle +\right.\\ & \left.ab\left\langle -\right|\left(-\left|+\right\rangle \left\langle -\right|+\left|-\right\rangle \left\langle +\right|\right)\left|+\right\rangle e^{-i\beta}+b^{2}\left\langle -\right|\left(-\left|+\right\rangle \left\langle -\right|+\left|-\right\rangle \left\langle +\right|\right)\left|-\right\rangle \right)\\ = & \frac{i\hbar}{2}\left(a^{2}\left(-\left\langle +|+\right\rangle \left\langle -|+\right\rangle +\left\langle +|-\right\rangle \left\langle +|+\right\rangle \right)+abe^{i\beta}\left(-\left\langle +|+\right\rangle \left\langle -|-\right\rangle +\left\langle +|-\right\rangle \left\langle +|-\right\rangle \right)+\right.\\ & \left.ab\left(-\left\langle -|+\right\rangle \left\langle -|+\right\rangle +\left\langle -|-\right\rangle \left\langle +|+\right\rangle \right)e^{-i\beta}+b^{2}\left(-\left\langle -|+\right\rangle \left\langle -|-\right\rangle +\left\langle -|-\right\rangle \left\langle +|-\right\rangle \right)\right)\\ = & \frac{i\hbar}{2}\left(-abe^{i\beta}+abe^{-i\beta}\right)\\ = & \hbar ab\frac{i\left(-e^{i\beta}+e^{-i\beta}\right)}{2}\\ = & \hbar ab\frac{\left(e^{i\beta}-e^{-i\beta}\right)}{2i}\\ & =\hbar ab\sin\beta \end{align*}

Logo temos:

⟨Sx⟩=ℏabcos⁡β⟨Sy⟩=ℏabsin⁡β→⟨Sx⟩2=(ℏabcos⁡β)2⟨Sy⟩2=(ℏabsin⁡β)2\left\langle S_{x}\right\rangle =\hbar ab\cos\beta\qquad\left\langle S_{y}\right\rangle =\hbar ab\sin\beta\rightarrow\left\langle S_{x}\right\rangle ^{2}=\left(\hbar ab\cos\beta\right)^{2}\qquad\left\langle S_{y}\right\rangle ^{2}=\left(\hbar ab\sin\beta\right)^{2}

Substituindo então as relações de dispersão:

⟨(ΔSx)2⟩=⟨Sx2⟩−⟨Sx⟩2⟨(ΔSy)2⟩=⟨Sy2⟩−⟨Sy⟩2=ℏ24−(ℏabcos⁡β)2=ℏ24−(ℏabsin⁡β)2\begin{align*} \left\langle \left(\Delta S_{x}\right)^{2}\right\rangle = & \left\langle S^{2}_{x}\right\rangle -\left\langle S_{x}\right\rangle ^{2} & \left\langle \left(\Delta S_{y}\right)^{2}\right\rangle = & \left\langle S^{2}_{y}\right\rangle -\left\langle S_{y}\right\rangle ^{2}\\ = & \frac{\hbar^{2}}{4}-\left(\hbar ab\cos\beta\right)^{2} & = & \frac{\hbar^{2}}{4}-\left(\hbar ab\sin\beta\right)^{2} \end{align*}

Então temos o seguinte produto da incerteza:

⟨(ΔSx)2⟩⟨(ΔSy)2⟩=(ℏ24−(ℏabcos⁡β)2)(ℏ24−(ℏabsin⁡β)2)=ℏ4[116−(absin⁡β)24−(abcos⁡β)24+(abcos⁡β)2(absin⁡β)2]=ℏ4[116−(ab2)2+(ab)4(2cos⁡βsin⁡β2)2]\begin{align*} \left\langle \left(\Delta S_{x}\right)^{2}\right\rangle \left\langle \left(\Delta S_{y}\right)^{2}\right\rangle & =\left(\frac{\hbar^{2}}{4}-\left(\hbar ab\cos\beta\right)^{2}\right)\left(\frac{\hbar^{2}}{4}-\left(\hbar ab\sin\beta\right)^{2}\right)\\ & =\hbar^{4}\left[\frac{1}{16}-\frac{\left(ab\sin\beta\right)^{2}}{4}-\frac{\left(ab\cos\beta\right)^{2}}{4}+\left(ab\cos\beta\right)^{2}\left(ab\sin\beta\right)^{2}\right]\\ & =\hbar^{4}\left[\frac{1}{16}-\left(\frac{ab}{2}\right)^{2}+\left(ab\right)^{4}\left(\frac{2\cos\beta\sin\beta}{2}\right)^{2}\right] \end{align*}

E usando a identidade trigonométrica sin⁡(2x)=2sin⁡xcos⁡x\sin\left(2x\right)=2\sin x\cos x, então a incerteza é:

⟨(ΔSx)2⟩⟨(ΔSy)2⟩=ℏ4[116−(ab2)2+(ab)4(sin⁡(2β)2)2]\begin{align*} \left\langle \left(\Delta S_{x}\right)^{2}\right\rangle \left\langle \left(\Delta S_{y}\right)^{2}\right\rangle & =\hbar^{4}\left[\frac{1}{16}-\left(\frac{ab}{2}\right)^{2}+\left(ab\right)^{4}\left(\frac{\sin\left(2\beta\right)}{2}\right)^{2}\right] \end{align*}

Como os termos (ab)2\left(ab\right)^{2} são necessariamente positivos, para maximizar a incerteza é necessário que sin⁡(2β)=1\sin\left(2\beta\right)=1. Considerando −π≤β≤+π-\pi\leq\beta\leq+\pi:

2β=±π2→β=π42\beta=\pm\frac{\pi}{2}\rightarrow\beta=\frac{\pi}{4}

Nesta situação temos que:

⟨(ΔSx)2⟩⟨(ΔSy)2⟩=ℏ416+ℏ4(ab2)2[(ab)2−1]\left\langle \left(\Delta S_{x}\right)^{2}\right\rangle \left\langle \left(\Delta S_{y}\right)^{2}\right\rangle =\frac{\hbar^{4}}{16}+\hbar^{4}\left(\frac{ab}{2}\right)^{2}\left[\left(ab\right)^{2}-1\right]

Pela condição de normalização temos que b2=1−a2b^{2}=1-a^{2}, então:

⟨(ΔSx)2⟩⟨(ΔSy)2⟩=ℏ416[1+[2a2(1−a2)]2−4a2(1−a2)]=ℏ416[1−2a2(1−a2)]2\begin{align*} \left\langle \left(\Delta S_{x}\right)^{2}\right\rangle \left\langle \left(\Delta S_{y}\right)^{2}\right\rangle & =\frac{\hbar^{4}}{16}\left[1+\left[2a^{2}\left(1-a^{2}\right)\right]^{2}-4a^{2}\left(1-a^{2}\right)\right]\\ & =\frac{\hbar^{4}}{16}\left[1-2a^{2}\left(1-a^{2}\right)\right]^{2} \end{align*}

Novamente pelas condições de normalização temos que 0≤a2≤10\leq a^{2}\leq1, então (1−a2)≥0\left(1-a^{2}\right)\geq0, de forma que 2a2(1−a2)≥02a^{2}\left(1-a^{2}\right)\geq0, assim queremos que a2(1−a2)=0a^{2}\left(1-a^{2}\right)=0. Podemos observar facilmente que isso é obtido com a=±1a=\pm1 ou a=0a=0. Dessa forma temos que o máximo de incerteza dado por:

⟨(ΔSx)2⟩⟨(ΔSy)2⟩=ℏ416\left\langle \left(\Delta S_{x}\right)^{2}\right\rangle \left\langle \left(\Delta S_{y}\right)^{2}\right\rangle =\frac{\hbar^{4}}{16}

relembrando nosso estado geral:

∣α⟩=a∣+⟩+beiβ∣−⟩\left|\alpha\right\rangle =a\left|+\right\rangle +be^{i\beta}\left|-\right\rangle

Ou ainda:

∣α⟩=a∣+⟩+1−a2eiβ∣−⟩\left|\alpha\right\rangle =a\left|+\right\rangle +\sqrt{1-a^{2}}e^{i\beta}\left|-\right\rangle

Então o máximo de incerteza ocorre quando a=0a=0 e temos que β=±π4\beta=\pm\frac{\pi}{4}:

∣α1⟩=±e±π4i∣−⟩\left|\alpha_{1}\right\rangle =\pm e^{\pm\frac{\pi}{4}i}\left|-\right\rangle

Ou se a=±1a=\pm1:

∣α2⟩=±∣+⟩\left|\alpha_{2}\right\rangle =\pm\left|+\right\rangle

Por fim, só nos resta verificar explicitamente que estas combinações lineares que encontramos não violam a relação de incerteza. Isto é, uma vez que a relação de incerteza para SxS_{x}e SyS_{y} é dada por:

⟨(ΔSx)2⟩⟨(ΔSy)2⟩≥14∣⟨[Sx,Sy]⟩∣2\left\langle \left(\Delta S_{x}\right)^{2}\right\rangle \left\langle \left(\Delta S_{y}\right)^{2}\right\rangle \geq\frac{1}{4}\left|\left\langle \left[S_{x},S_{y}\right]\right\rangle \right|^{2}

Queremos demonstrar que :

ℏ416≥14∣⟨[Sx,Sy]⟩∣2\frac{\hbar^{4}}{16}\geq\frac{1}{4}\left|\left\langle \left[S_{x},S_{y}\right]\right\rangle \right|^{2}

Calculando então o comutador entre SxS_{x} e SyS_{y}:

[Sx,Sy]=SxSy−SySx=ℏ2(∣+⟩⟨−∣+∣−⟩⟨+∣)iℏ2(−∣+⟩⟨−∣+∣−⟩⟨+∣)−ℏ2iℏ2(−∣+⟩⟨−∣+∣−⟩⟨+∣)(∣+⟩⟨−∣+∣−⟩⟨+∣)=iℏ24(−∣+⟩⟨−∣+⟩⟨−∣+∣+⟩⟨−∣−⟩⟨+∣−∣−⟩⟨+∣+⟩⟨−∣+∣−⟩⟨+∣−⟩⟨+∣)−iℏ24(−∣+⟩⟨−∣+⟩⟨−∣−∣+⟩⟨−∣−⟩⟨+∣+∣−⟩⟨+∣+⟩⟨−∣+∣−⟩⟨+∣−⟩⟨+∣)=iℏ24(2∣+⟩⟨+∣−2∣−⟩⟨−∣)=iℏ[ℏ2(∣+⟩⟨+∣−∣−⟩⟨−∣)]=iℏSz\begin{align*} \left[S_{x},S_{y}\right]= & S_{x}S_{y}-S_{y}S_{x}\\ = & \frac{\hbar}{2}\left(\left|+\right\rangle \left\langle -\right|+\left|-\right\rangle \left\langle +\right|\right)\frac{i\hbar}{2}\left(-\left|+\right\rangle \left\langle -\right|+\left|-\right\rangle \left\langle +\right|\right)-\frac{\hbar}{2}\frac{i\hbar}{2}\left(-\left|+\right\rangle \left\langle -\right|+\left|-\right\rangle \left\langle +\right|\right)\left(\left|+\right\rangle \left\langle -\right|+\left|-\right\rangle \left\langle +\right|\right)\\ = & \frac{i\hbar^{2}}{4}\left(-\left|+\right\rangle \left\langle -|+\right\rangle \left\langle -\right|+\left|+\right\rangle \left\langle -|-\right\rangle \left\langle +\right|-\left|-\right\rangle \left\langle +|+\right\rangle \left\langle -\right|+\left|-\right\rangle \left\langle +|-\right\rangle \left\langle +\right|\right)-\\ & \frac{i\hbar^{2}}{4}\left(-\left|+\right\rangle \left\langle -|+\right\rangle \left\langle -\right|-\left|+\right\rangle \left\langle -|-\right\rangle \left\langle +\right|+\left|-\right\rangle \left\langle +|+\right\rangle \left\langle -\right|+\left|-\right\rangle \left\langle +|-\right\rangle \left\langle +\right|\right)\\ = & \frac{i\hbar^{2}}{4}\left(2\left|+\right\rangle \left\langle +\right|-2\left|-\right\rangle \left\langle -\right|\right)\\ = & i\hbar\left[\frac{\hbar}{2}\left(\left|+\right\rangle \left\langle +\right|-\left|-\right\rangle \left\langle -\right|\right)\right]\\ = & i\hbar S_{z} \end{align*}

Usando então ∣α1⟩\left|\alpha_{1}\right\rangle obtemos:

⟨[Sx,Sy]⟩1=⟨α1∣iℏSz∣α1⟩=iℏ22[⟨−∣e∓π4i(∣+⟩⟨+∣−∣−⟩⟨−∣)e±π4i∣−⟩]=iℏ22[(⟨−∣+⟩⟨+∣−⟩−⟨−∣−⟩⟨−∣−⟩)]=−iℏ22\begin{align*} \left\langle \left[S_{x},S_{y}\right]\right\rangle _{1}= & \left\langle \alpha_{1}\left|i\hbar S_{z}\right|\alpha_{1}\right\rangle \\ = & \frac{i\hbar^{2}}{2}\left[\left\langle -\right|e^{\mp\frac{\pi}{4}i}\left(\left|+\right\rangle \left\langle +\right|-\left|-\right\rangle \left\langle -\right|\right)e^{\pm\frac{\pi}{4}i}\left|-\right\rangle \right]\\ = & \frac{i\hbar^{2}}{2}\left[\left(\left\langle -|+\right\rangle \left\langle +|-\right\rangle -\left\langle -|-\right\rangle \left\langle -|-\right\rangle \right)\right]\\ = & -\frac{i\hbar^{2}}{2} \end{align*}

Usando então ∣α2⟩\left|\alpha_{2}\right\rangle obtemos:

⟨[Sx,Sy]⟩2=⟨α2∣iℏSz∣α2⟩=iℏ22[⟨+∣±(∣+⟩⟨+∣−∣−⟩⟨−∣)±∣+⟩]=iℏ22[(⟨+∣+⟩⟨+∣+⟩−⟨+∣−⟩⟨−∣+⟩)]=iℏ22\begin{align*} \left\langle \left[S_{x},S_{y}\right]\right\rangle _{2}= & \left\langle \alpha_{2}\left|i\hbar S_{z}\right|\alpha_{2}\right\rangle \\ = & \frac{i\hbar^{2}}{2}\left[\left\langle +\right|\pm\left(\left|+\right\rangle \left\langle +\right|-\left|-\right\rangle \left\langle -\right|\right)\pm\left|+\right\rangle \right]\\ = & \frac{i\hbar^{2}}{2}\left[\left(\left\langle +|+\right\rangle \left\langle +|+\right\rangle -\left\langle +|-\right\rangle \left\langle -|+\right\rangle \right)\right]\\ = & \frac{i\hbar^{2}}{2} \end{align*}

Então independente de qual combinação linear escolhermos, ficamos com:

∣⟨[Sx,Sy]⟩∣=ℏ22\left|\left\langle \left[S_{x},S_{y}\right]\right\rangle \right|=\frac{\hbar^{2}}{2}

Consequentemente:

∣⟨[Sx,Sy]⟩∣2=ℏ44\left|\left\langle \left[S_{x},S_{y}\right]\right\rangle \right|^{2}=\frac{\hbar^{4}}{4}

Logo a relação de incerteza é:

⟨(ΔSx)2⟩⟨(ΔSy)2⟩≥ℏ416\left\langle \left(\Delta S_{x}\right)^{2}\right\rangle \left\langle \left(\Delta S_{y}\right)^{2}\right\rangle \geq\frac{\hbar^{4}}{16}

Portanto ela não é violada, uma vez que:

ℏ416≥ℏ416\frac{\hbar^{4}}{16}\geq\frac{\hbar^{4}}{16}

É uma igualdade válida.