I'm working through Pinchover and Rubinstein's "Introduction to Partial Differential Equations" and am trying to understand the motivation for studying Sturm Liouville problems. To this end, I am following the process of taking a general parabolic PDE:
$$u_{t}-\frac{1}{r\left(x\right)m\left(t\right)}\left(\left(p\left(x\right)u_{x}\right)_{x}+q\left(x\right)u\right) = 0, \ x\in\left(a,b\right),t\in\left(0,\infty\right)$$ with boundary conditions $$B_{a}\left[u\right]:=\alpha u\left(a,t,\right)+\beta u_{x}\left(a,t\right) = 0, \ t\in\left[0,\infty\right)$$ $$B_{b}\left[u\right]:=\gamma u\left(b,t\right)+\delta u_{x}\left(b,t\right) = 0, \ t\in\left[0,\infty\right)$$ and initial condition $$u\left(x,0\right) = f\left(x\right), \ x\in\left[a,b\right].$$
Let us consider the parabolic problem in more detail. Just as in the case for the heat equation, we seek non-trivial solutions of the form \begin{equation} u\left(x,t\right)=X\left(x\right)T\left(t\right). \end{equation}
Differentiating and substituting, noting that $\left(pX_{x}T\right)_{x}=T\left(pX_{x}\right)$, \begin{eqnarray} XT_{t}-\frac{1}{rm}\left(\left(pX_{x}T\right)_{x}+qXT\right) & = & 0\\ \frac{T_{t}m}{T} & = & \frac{\left(pX_{x}\right)_{x}+qX}{rX} \end{eqnarray} where the LHS is a function only of $t$ and the RHS a function only of $x$, so that $$ \frac{T_{t}m}{T}=\frac{\left(pX_{x}\right)_{x}+qX}{rX}=-\lambda. $$ Hence, we have the system of ordinary differential equations
\begin{array}{cccc} \frac{d}{dx}\left(pX\right)+qX+\lambda rX & = & 0, & x\in\left(a,b\right),\\ m\frac{dT}{dt}+\lambda T & = & 0, & t\in\left(0,\infty\right). \end{array}
All fine so far by me. However, the authors then go on to say that since $u$ satisfies the boundary conditions $B_a [u]$ and $B_b [u]$, it follows that
$$B_a [X] = 0, \ B_b [X] =0.$$
I'm afraid I don't see why this is. Can anybody explain?