Okay, I checked and you got it mostly right, except the factor $\mu(u)$ in front of the power of $u$ at the very end, in the main equation. Let's simplify slightly your notations and write $R(\Omega, u)$ and $R(\Omega, u + \varphi)$ for the Rayleigh quotients. I do not compute using a real parameter ; rather, I perform some generalized Taylor exapnsions to get the full derivative of the quotient, which means that $\varphi$ is to be thought of as small itself. Denote by $\|u\|_q^2$ the denominator of $R$. The numerator of $R(\Omega, u + \varphi)$ expands as \begin{equation} \int_{\Omega} |\nabla u |^2 + \alpha \int_{\partial \Omega} |u|^2 + 2 \int_{\Omega} \nabla u \cdot \nabla \varphi + 2 \alpha \int_{\partial \Omega} u \varphi + \mathcal{O}(\varphi^2). \end{equation} Its denominator writes \begin{align} & \|u\|_q^2 \left( 1 + \frac{q}{\|u\|_q^q} \int_{\Omega} |u|^{q-2} u \varphi + \mathcal{O}(\varphi^2) \right)^{\frac{2}{q}} \\ & = \|u\|_q^2 \left( 1 + \frac{2}{\|u\|_q^q} \int_{\Omega} |u|^{q-2} u \varphi + \mathcal{O}(\varphi^2) \right) . \end{align} Thanks to the usual $(1+x)^{-1} = 1-x + \mathcal{O}(x^2)$, we get : \begin{equation} R(\Omega, u + \varphi) = R(\Omega, u) - \frac{2}{\|u\|_q^q} R(\Omega,u) \int_{\Omega} |u|^{q-2} u \varphi + \frac{2}{\|u\|_q^2} \left( \int_{\Omega} \nabla u \cdot \nabla \varphi + \alpha \int_{\Omega} u \varphi \right) + \mathcal{O}(\varphi^2). \end{equation} Using integration by parts, this rewrites \begin{equation} R(\Omega, u + \varphi) = \lambda - \frac{2}{\|u\|_q^q} \lambda \int_{\Omega} |u|^{q-2}u \varphi + \frac{2}{\|u\|_q^2} \left( - \int_{\Omega} \Delta u \varphi + \int_{\partial \Omega} (\partial_{\nu} u + \alpha u) \varphi\right). \end{equation} Finally we are done. The boundary condition that you got was the right one, whereas the main equation is now \begin{equation} - \frac{\Delta u}{\|u\|_q^2} = \lambda \frac{|u|^{q-2}u}{\|u\|_q^q}, \end{equation} i.e. \begin{equation} - {\Delta u} = \lambda \frac{|u|^{q-2}u}{\|u\|_q^{q-2}}. \end{equation} Notice that if we set $q=2$ and $\alpha = 0$, we indeed get back to the usual eigenvalue problem for the Neumann laplacian, which is your first case.