Minimizing angular momentum uncertainties

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mrbetadine
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Homework Statement
Consider a physical system of fixed angular momentum ##l##. The state of the system is in the subspace spanned by ##2l+1## eigenvectors ##|l,m\rangle## of ##L_z## (##-l\leq m\leq +l##). Find the state ##|\psi_0\rangle## of the system for which ##(\Delta L_x)^2+(\Delta L_y)^2+(\Delta L_z)^2## is minimal.
Relevant Equations
n/a
\begin{align*}
&(\Delta L_x)^2+(\Delta L_y)^2+(\Delta L_z)^2\\
={}&\langle L_x^2\rangle-\langle L_x \rangle^2+\langle L_y^2\rangle-\langle L_y \rangle^2+\langle L_z^2\rangle-\langle L_z \rangle^2\\
={}&\langle L_x^2+L_y^2+L_z^2 \rangle-(\langle L_x \rangle^2+\langle L_y \rangle^2+\langle L_z \rangle^2)\\
={}&l(l+1)\hbar^2-(\langle L_x \rangle^2+\langle L_y \rangle^2+\langle L_z \rangle^2).
\end{align*}
To minimize ##(\Delta L_x)^2+(\Delta L_y)^2+(\Delta L_z)^2## is equivalent to maximizing
$$ \langle L_x \rangle^2+\langle L_y \rangle^2+\langle L_z \rangle^2$$

How should I proceed?
I have also obtained an alternative expression
$$\langle L_x \rangle^2+\langle L_y \rangle^2+\langle L_z \rangle^2=\langle L_+\rangle\langle L_-\rangle+\langle L_z\rangle^2 $$
where
$$ L_\pm=L_x\pm i L_y$$
but it does not help much. It would be easy if we restrict ourselves to finding states of the form ##|l,m\rangle##.

*The hint I got indicates that ##|\psi_0\rangle## is the solution to the equations
\begin{align*}
(L_x+iL_y)|\psi_0\rangle&=0\\
L_z|\psi_0\rangle&=l\hbar|\psi_0\rangle.
\end{align*}
 
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By the hint
$$<L_x>=<L_y>=0$$
$$<L_z>=l\hbar$$
 
There may be a simple and elegant solution to the problem, but I can't see it currently. So I'll suggest a brute force approach.

Note that if ##~|\psi_0\rangle~## minimizes the uncertainty, then any state derived from it by a rotation is just as good.

Any normalized state in the ##l## subspace can be spanned as$$|\psi\rangle=\sum^l_{m=-l}\left(\alpha_m+i\beta_m\right)|l,m\rangle\quad,$$where ##~\{\alpha_m,\beta_m\}~## are ##~4l+2~## real coefficients.
As you concluded in post #1, minimizing the uncertainty is the same as maximizing$$f:=\langle L_+\rangle\langle L_-\rangle+\langle L_z\rangle^2 $$(which can now be expressed explicitly as a real function of the real ##~\{\alpha_m,\beta_m\}~##), subjected to the normalization constraint$$\chi:=\langle\psi|\psi\rangle-1=\sum\left(\alpha_m^2+\beta_m^2\right)-1=0\quad.$$The method of Lagrange multipliers is usually applicable in cases like this.
 
We wish to maximise ##\langle L_x \rangle^2 + \langle L_y \rangle^2 + \langle L_z \rangle^2##. Write

\begin{align*}
| \psi_0 \rangle = \sum_{m=-l}^l a_m |l,m\rangle
\end{align*}

I get

\begin{align*}
& | \langle L_+\rangle |^2 + \langle L_z\rangle^2 =
\nonumber \\
& = \hbar^2\, \left| \sum_{m=-l}^{l-1} a_{m+1}^* a_m \sqrt{l(l+1)-m(m+1)} \right|^2 + \hbar^2\, (\sum_{m=-l}^l |a_m|^2m)^2
\end{align*}

We want to maximise this subject to ##\sum_{m=-l}^l |a_m|^2 = 1##.

The value of the first sum is maximised when all terms have the same phase. Choose ##a_m = |a_m| e^{-i m \phi - i \phi_0}##, then

\begin{align*}
& | \langle L_+\rangle |^2 + \langle L_z\rangle^2 =
\nonumber \\
& = \hbar^2\, \left( \sum_{m=-l}^{l-1} x_{m+1} x_m \sqrt{l(l+1)-m(m+1)} \right)^2 + \hbar^2\, (\sum_{m=-l}^l x_m^2m)^2
\end{align*}

where ##x_m = |a_m|##. We want to maximise this subject to ##\sum_{m=-l}^l x_m^2 = 1##.

Let us maximise ##f(x_m) = \hbar \sqrt{S^2+M^2}##, where

\begin{align*}
S = \sum_{m=-l}^{l-1} x_{m+1} x_m \sqrt{l(l+1)-m(m+1)} , \quad M = \sum_{m=-l}^l x_m^2m
\end{align*}

Method of Lagrange multipliers gives the eigenvector equation

\begin{align*}
\frac{\partial}{\partial x_m} f (x_m) - \lambda \frac{\partial}{\partial x_m} (\sum_{m=-l}^l x_m^2 - 1) = 0
\end{align*}

Thus

\begin{align*}
\hbar\, \frac{S}{\sqrt{S^2+M^2}} \frac{\partial S}{\partial x_m} + \hbar\, \frac{M}{\sqrt{S^2+M^2}} \frac{\partial M}{\partial x_m} - \lambda 2 x_m = 0
\end{align*}

Define

\begin{align*}
\sin \alpha = \frac{S}{\sqrt{S^2+M^2}} , \quad \cos \alpha = \frac{M}{\sqrt{S^2+M^2}} ,
\end{align*}

then the eigenvector equation becomes

\begin{align*}
\hbar\, \sin \alpha \frac{\partial S}{\partial x_m} + \hbar\, \cos \alpha \frac{\partial M}{\partial x_m} - \lambda 2 x_m = 0
\end{align*}

Perform ##\frac{\partial S}{\partial x_m}## and ##\frac{\partial M}{\partial x_m}##.

Calculate ##\langle l,m | \, e^{-i \phi L_z/\hbar} L_{x} e^{i \phi L_z/\hbar} | \psi_0 \rangle##.

Use ##e^{-i \phi L_z/\hbar} L_{x} e^{i \phi L_z/\hbar} = \cos \phi L_{x} + \sin \phi L_{y}##. Substituting into the eigenvector equation, we obtain

\begin{align*}
\sin \alpha (\cos \phi L_{x} + \sin \phi L_{y}) \,|\psi_0 \rangle + \cos \alpha L_{z} \,|\psi_0 \rangle = \lambda |\psi_0 \rangle
\end{align*}

or

\begin{align*}
\vec{L} \cdot \vec{n} |\psi_0 \rangle = \lambda |\psi_0 \rangle
\end{align*}

where ##\vec{n} = (\sin \alpha \cos \phi , \sin \alpha \sin \phi, \cos \alpha)##. Without loss of generality, you can consider

\begin{align*}
L_z |\psi_0 \rangle = \lambda |\psi_0 \rangle
\end{align*}

and find the eigenvector and eigenvalue that maximises ##\langle L_x \rangle^2 + \langle L_y \rangle^2 + \langle L_z \rangle^2##. For eigenstates of ##L_{z}##, ##\langle l,m |L_x | l,m \rangle = \langle l,m | L_y | l,m \rangle = 0## and ##\langle l,m | L_z | l,m \rangle^2 = m^2##. Obviously the states ##| l,l \rangle## and ##| l,-l \rangle## maximises ##\langle L_x \rangle^2 + \langle L_y \rangle^2 + \langle L_z \rangle^2##.

States that also maximises ##\langle L_x \rangle^2 + \langle L_y \rangle^2 + \langle L_z \rangle^2##, are obtained from the state ##| l,l \rangle## by rotation.
 
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Very nice. Thanks, @julian.

Actually, it is easier to show by variation that ##~|l,l\rangle~## (or its rotations) yield a maximum for$$f:=\langle L_+\rangle\langle L_-\rangle+\langle L_z\rangle^2\quad.$$The shortcoming of this variation approach is that we still have to prove that this maximum is global.

Consider the variation$$|\psi\rangle=\left(1-\varepsilon^2\sum^{l-1}_{m=-l}\left|a_m\right|^2\right)^{1/2}|l,l\rangle+\varepsilon\sum^{l-1}_{m=-l}a_m|l,m\rangle\quad,$$where ##~\varepsilon\ll 1~##. Then
1. The lowest order correction to ##f## is proportional to ##~\varepsilon^2~##.
2. The contribution of the left term of ##f## to the ##~a_{l-1}##-dependence of the ##~\varepsilon^2~## correction, is canceled by the contribution of the right term.
3. For ##~m\le l-2~##, only the (diagonal) right term of ##f## contributes to the ##~\varepsilon^2~## correction, and these contributions are either zero (rotation) or negative.
 
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