I'm looking for a way to derive a closed form expression for $\omega$, which is the solution of the following maximization problem: $$\max_{w} \omega^{T}\mu$$ $$\textrm{st.}\hspace{0.5cm} \omega^{T}\Sigma\omega=\sigma^2$$ $$ \omega^{T}\textbf{1}=1 $$ In particular I'm struggeling at the point where i try to solve for the lagrange multipliers given the second FOC: $$\frac{d{L(\dots)}}{d{\omega}}=\mu-2\lambda_{1}\Sigma\omega-\lambda_{2}\textbf{1}=0$$ $$\frac{d{L(\dots)}}{d{\lambda_{1}}}=\sigma^{2}-\omega^{T}\Sigma\omega=0$$ $$\frac{d{L(\dots)}}{d{\lambda_{2}}}=1-\omega^{T}\textbf{1}=0$$
Here, $\mu$ is a (1xn)-vector nx1 of some constants, $\omega$ the (1xn)-vector of interest, $\Sigma$ some (nxn)-matrix, $\lambda_{1}$ and $\lambda_{2}$ the lagrange multipliers for constraints 1 and 2 and $\sigma^2$ is some (1x1)-variable.
The problem here (at least for me) is that the first derivative for the lagrange multipliers of the constraints includes two $\omega$-vectors and thus yields a quadratic expression, for which i can't easily solve the second FOC for the needed lagrange multipliers.. I'm not sure whether i'm on the right track and if yes, how to solve for the analytical expression of $\omega$ from here.
If an analytical solution / expression for $\omega$ does exist, how can I explicitly derive this solution step-by-step?

Here's another solution that doesn't reduce the order of the problem.
We have the following three equations (as described in the question)
$ \mu - 2 \lambda_1 \Sigma \omega - \lambda_2 \mathbf{1} = \mathbf{0} $
$ \omega^T \Sigma \omega = \sigma^2 $
$ \omega^T \mathbf{1} = 1 $
From the first equation,
$ \omega = \dfrac{1}{2 \lambda_1} \Sigma^{-1} ( \mu - \lambda_2 \mathbf{1} ) $
substituting this into the next two equations, gives us,
$\dfrac{1}{(2 \lambda_1)^2} ( \mu - \lambda_2 \mathbf{1} )^T \Sigma^{-1} ( \mu - \lambda_2 \mathbf{1} ) = \sigma^2 $
and
$\dfrac{1}{2 \lambda_1} \mathbf{1}^T \Sigma^{-1} ( \mu - \lambda_2 \mathbf{1} ) = 1 $
Combining the two equations by eliminating $(2 \lambda_1)$,
$ ( \mu - \lambda_2 \mathbf{1} )^T \Sigma^{-1} ( \mu - \lambda_2 \mathbf{1} ) = \sigma^2 ( \mathbf{1}^T \Sigma^{-1} ( \mu - \lambda_2 \mathbf{1} ) )^2 $
This is a quadratic equation in $\lambda_2$ that can be solved for $2$ values of $\lambda_2$. Corresponding to each value of $\lambda_2$ we then solve for $\lambda_1$, and $\omega$ follows.
I will now expand the above quadratic equation and put it in the standard quadratic equation format.
$ \lambda_2^2 (\mathbf{1}^T \Sigma^{-1} \mathbf{1} ) - 2 \lambda_2 (\mu^T \Sigma^{-1} \mathbf{1} ) + \mu^T \Sigma^{-1} \mu = \sigma^2 ( \mu^T \Sigma^{-1} \mathbf{1} - \lambda_2 (\mathbf{1}^T \Sigma^{-1} \mathbf{1} ) )^2 $
Define,
$ a = \mathbf{1}^T \Sigma^{-1} \mathbf{1} $
$ b = \mu^T \Sigma^{-1} \mathbf{1} $
$ c = \mu^T \Sigma^{-1} \mu $
Then our equation in $\lambda_2$ becomes
$ a \lambda_2^2 - 2 b \lambda_2 + c = \sigma^2 ( b - a \lambda_2 )^2 $
Expanding the squared term on the right hand side and re-grouping,
$ (a - a^2 \sigma^2 ) \lambda_2^2 + ( 2 a b \sigma^2 - 2 b ) \lambda_2 + (c - b^2 \sigma^2) = 0 $
Divide through by $ (1 - a \sigma^2 ) $,
$ a \lambda_2^2 - 2 b \lambda_2 + \bigg(\dfrac{ c - b^2 \sigma^2}{1- a \sigma^2 } \bigg) = 0 $
Complete the square,
$ a ( \lambda - \dfrac{b}{a} )^2 + \bigg(\dfrac{ c - b^2 \sigma^2}{1- a \sigma^2 } \bigg) - \dfrac{b^2}{a} = 0 $
The constant term simplifies to
$ \dfrac{ a (c - b^2 \sigma^2 ) - b^2 (1 - a \sigma^2 ) }{a (1 - a \sigma^2)} = \dfrac{ ac - b^2 }{ a (1 - a \sigma^2) } $
Divide through by $a$, then
$ ( \lambda - \dfrac{b}{a} )^2 = \dfrac{ b^2 - a c }{ a^2 (1 - a \sigma^2)} $
Hence, the solutions are
$ \lambda_2 = \dfrac{b}{a} \pm \sqrt{ \dfrac{ b^2 - a c }{a^2 (1 - a \sigma^2) } } $
Note that $a$ and $c$ are positive. To have a real solution, we require that
$ \dfrac{ b^2 - a c }{a^2 (1 - a \sigma^2) } \ge 0 $
Now, for the tangent plane to the ellipsoid $ \omega^T \Sigma \omega = \sigma^2 $ to have a normal vector along $\mathbf{1}$, we have
$ \Sigma \omega = \alpha \mathbf{1} $
Substituting in the ellipsoid equation, we get
$ \alpha = \sqrt{\dfrac{ \sigma^2 }{ \mathbf{1}^T \Sigma^{-1} \mathbf{1} } } = \sqrt{\dfrac{ \sigma^2 }{a} } $
So that tangency point is
$ \omega_1 = \dfrac{ \Sigma^{-1} \mathbf{1} \sqrt{ \sigma^2} }{ \sqrt{a} } $
The distance between the origin and the tangent plane is
$ d_1 = \sqrt{\sigma^2} \dfrac{ \mathbf{1}^T \Sigma^{-1} \mathbf{1} } { \sqrt{a} \sqrt{\mathbf{1}^T \mathbf{1} } } = \dfrac{ \sqrt{a \sigma^2} }{\sqrt{n}} $
On the other hand, the distance between the origin and the hyperplane $ \omega^T \mathbf{1} = 1 $ is given by
$ d_2 = \dfrac{1}{\sqrt{ n } } $
Hence, there will be an intersection between the ellipsoid and the hyperplane if and only if $d_1 \gt d_2 $, which is equivalent to
$ a \sigma^2 \gt 1 $
Using this in the inequality for real solutions of the quadratic in $\lambda_2$ above, we deduce that the condition is now
$ b^2 - a c \le 0 $
i.e
$ a c \ge b^2 $
Careful examination of the definitions of $a,b, c$, and the use of the Cauchy-Schwartz inequality, leads to the conclusion that we always have,
$ a c \ge b^2 $
Therefore, in conclusion, the necessary and sufficient condition that the quadratic equation has real solutions is that
$ a \sigma^2 \ge 1 $
And this inequality is satisfied if and only if the hyperplane $\omega^T \mathbf{1} = 1$ intersects the ellipsoid $\omega^T \Sigma \omega = \sigma^2$.
The two values of $\lambda_2 $ are given by
$ \lambda_2 = \dfrac{1}{a} \bigg( b \pm \sqrt{ \dfrac{ ac - b^2 }{ a \sigma^2 - 1 } } \bigg) $
One solution is for the minimum and the other the maximum of the given objective function.
From the value of $\lambda_2$ (there is obviously two of them), we can calculate the corresponding $\lambda_1$ from
$\dfrac{1}{2 \lambda_1} \mathbf{1}^T \Sigma^{-1} ( \mu - \lambda_2 \mathbf{1} ) = 1 $
which is stated above in the derivation, and from which, we have
$ \lambda_1 = \dfrac{1}{2} \mathbf{1}^T \Sigma^{-1} (\mu - \lambda_2 \mathbf{1} ) = \dfrac{1}{2} ( b - a \lambda_2 ) $
And finally, from $\lambda_1, \lambda_2 $ we can compute $\omega$.
This is given by,
$ \omega = \dfrac{1}{2 \lambda_1} \Sigma^{-1} ( \mu - \lambda_2 \mathbf{1} ) $
Now
$ f(\omega) = \mu^T \omega = \dfrac{1}{2 \lambda_1} ( c - \lambda_2 b ) $
Substituting the above expression for $\lambda_1$, we get
$ f = \dfrac{ c - b \lambda_2 }{ b - a \lambda_2 } $