Integrate
$$I=\int_{0}^{\infty}{1\over x}\cdot{1-e^{-\phi{x}}\over 1+e^{\phi{x}}}\,dx=\ln\left({\pi\over 2}\right)\tag1,$$
where $\phi={1+\sqrt5\over 2}$.
Recall
$\tanh y=-{1-e^{2y}\over 1+e^{2y}}$, setting $y={\phi{x}\over 2}$ we have
$$\tanh\left({\phi{x}\over 2}\right)=-{1-e^{x\phi}\over 1+e^{x\phi}}\tag2.$$
Sub $(2)$ into $(1)\rightarrow (3)$
$$I=-\int_{0}^{\infty}{\tanh\left({x\phi\over 2}\right)\over x}\,dx\tag4.$$
Recall
$$\tanh x=\sum_{n=1}^{\infty}{(-1)^{n-1}2^{2n}(2^{2n}-1)B_nx^{2n-1}\over (2n)!}\tag5$$
Sub $(5)$ into $(4)\rightarrow (6)$
$$I=\sum_{n=1}^{\infty}{(-1)^{n-1}2^{2n}(2^{2n}-1)B_nx^{2n-1}\over (2n)!}\int_{0}^{\infty}{\left({x\phi\over 2}\right)^{2n-1}\over x}\,dx\tag6.$$
The problem is that
$$\int_{0}^{\infty}{\left({x\phi\over 2}\right)^{2n-1}\over x}dx$$ diverges. I went wrong somewhere, can anyone help please?
$\newcommand{\angles}[1]{\left\langle\, #1 \,\right\rangle} \newcommand{\braces}[1]{\left\lbrace\, #1 \,\right\rbrace} \newcommand{\bracks}[1]{\left\lbrack\, #1 \,\right\rbrack} \newcommand{\dd}{\mathrm{d}} \newcommand{\ds}[1]{\displaystyle{#1}} \newcommand{\expo}[1]{\,\mathrm{e}^{#1}\,} \newcommand{\half}{{1 \over 2}} \newcommand{\ic}{\mathrm{i}} \newcommand{\iff}{\Leftrightarrow} \newcommand{\imp}{\Longrightarrow} \newcommand{\ol}[1]{\overline{#1}} \newcommand{\pars}[1]{\left(\, #1 \,\right)} \newcommand{\partiald}[3][]{\frac{\partial^{#1} #2}{\partial #3^{#1}}} \newcommand{\root}[2][]{\,\sqrt[#1]{\, #2 \,}\,} \newcommand{\totald}[3][]{\frac{\mathrm{d}^{#1} #2}{\mathrm{d} #3^{#1}}} \newcommand{\verts}[1]{\left\vert\, #1 \,\right\vert}$ It's clear that the integral is $\ds{\phi}$-independent. ${\phi \equiv {1 + \root{5} \over 2} > 0}$.
Namely, $\ds{\int_{0}^{\infty}{1 - \expo{-\phi x} \over 1 + \expo{\phi x}} \,{\dd x \over x}\ \stackrel{\phi x\ \to\ x}{=}\ \int_{0}^{\infty}{1 - \expo{-x} \over 1 + \expo{x}}\,{\dd x \over x}}$
\begin{align} \int_{0}^{\infty}{1 - \expo{-x} \over 1 + \expo{x}}\,{\dd x \over x} & = \int_{0}^{\infty}{1 - \expo{-x} \over 1 + \expo{-x}}\,\expo{-x}\,{\dd x \over x} \ \stackrel{\expo{-x}\ =\ t}{=}\ -\int_{0}^{1}{1 - t \over 1 + t}\,{\dd t \over \ln\pars{t}} \\[3mm] & = \int_{0}^{1}{1 - t \over 1 + t}\ \overbrace{\int_{0}^{\infty}t^{\mu}\,\dd\mu}^{\ds{-\,{1 \over \ln\pars{t}}}}\ \,\dd t = \int_{0}^{\infty}\int_{0}^{1}{t^{\mu} - t^{\mu + 1} \over 1 + t}\,\dd\mu\,\dd t \\[3mm] & = \int_{0}^{\infty}\bracks{% 2\int_{0}^{1}{t^{\mu} - t^{\mu + 1} \over 1 - t^{2}}\,\dd\mu - \int_{0}^{1}{t^{\mu} - t^{\mu + 1} \over 1 - t}\,\dd\mu} \\[3mm] & = \int_{0}^{\infty}\bracks{% \int_{0}^{1}{t^{\mu/2 - 1/2} - t^{\mu/2} \over 1 - t}\,\dd\mu - \int_{0}^{1}{t^{\mu} - t^{\mu + 1} \over 1 - t}\,\dd\mu} \\[8mm] & = \int_{0}^{\infty}\left\lbrack% \int_{0}^{1}{1 - t^{\mu/2} \over 1 - t}\,\dd\mu - \int_{0}^{1}{1 - t^{\mu/2 - 1/2} \over 1 - t}\,\dd\mu\right. \\[3mm] & \left.\mbox{} + \int_{0}^{1}{1 - t^{\mu} \over 1 - t}\,\dd\mu - \int_{0}^{1}{1 - t^{\mu + 1} \over 1 - t}\,\dd\mu\right\rbrack \\[8mm] & = \int_{0}^{\infty}\bracks{% \Psi\pars{1 + {\mu \over 2}} - \Psi\pars{\half + {\mu \over 2}} + \Psi\pars{1 + \mu} - \Psi\pars{2 + \mu}}\,\dd\mu \\[3mm] & = \left.% \ln\pars{\Gamma^{2}\pars{1 + \mu/2}\Gamma\pars{1 + \mu} \over \Gamma^{2}\pars{1/2 + \mu/2}\Gamma\pars{2 + \mu}} \right\vert_{\ 0}^{\ \infty} \\[3mm] & = \underbrace{% \lim_{\mu \to \infty}\ln\pars{\Gamma^{2}\pars{1 + \mu/2} \over \Gamma^{2}\pars{1/2 + \mu/2}\pars{1 + \mu}}}_{\ds{-\ln\pars{2}}}\ -\ \underbrace{\ln\pars{\Gamma^{2}\pars{1}\Gamma\pars{1} \over \Gamma^{2}\pars{1/2}\Gamma\pars{2}}}_{\ds{-\ln\pars{\pi}}}\ =\ \color{#f00}{\ln\pars{\pi \over 2}} \end{align}
where $\Psi$ is the Digamma function and, by definition, $\ds{\Psi\pars{z} = \totald{\ln\pars{\Gamma\pars{z}}}{z}}$. In the above calculation we used the well known identities ( $\gamma$ is the Euler-Mascheroni constant ): \begin{align} \Psi\pars{z} + \gamma & = \int_{0}^{1}{1 - t^{z - 1} \over 1 - t}\,\dd t\,,\qquad\Re\pars{z} > 0 \\[3mm] \Gamma\pars{1} & = \Gamma\pars{2} = 1\,,\quad\Gamma\pars{\half} = \root{\pi} \,,\quad\Gamma\pars{z + 1} = z\,\Gamma\pars{z} \end{align}
The last $\ds{\mu \to \infty}$ limit can be evaluated with Stirling Asymptotic Formula.