One loop corrections for gravity usually includes non-local terms in the action such as $R\log(\frac{-\Box}{\mu^2})R$, where $\Box=g^{\mu\nu}\nabla_\mu\nabla_\nu$ is the D'Alembert operator, $R$ is the scalar curvature and $\mu$ is just some constant. My problem concerns how to interpret the log of an operator. In http://arxiv.org/pdf/1507.07829.pdf, the definition goes like (see equation 4.2 in pg 9)
$ \log(\frac{-\Box}{\mu^2})=\int_0^\infty ds \left(\frac{1}{\mu^2+s}+\frac{1}{-\Box+s}\right). $
Besides this definition be quite arbitrary to me, again a function of $\Box$ shows up and I end up with the same problem. So how should I interpret a function like $f(\Box)$? Is it to be seen as a Taylor expansion in the same way that is usually defined in quantum mechanics, i.e.
$ f(\Box)=\sum_n\frac{f^{(n)}(0)}{n!}\Box^n \quad? $