In the Random Energy Model, the Hamiltonian of a spin system $S_{N} = \{ -1,+1 \} ^N$ is defined as $H_{N}(\sigma) = -\sqrt{N}X_{\sigma}$, where the $X_{\sigma}$ are i.i.d normally distributed. We are interested in the behaviour of the expectation of $\Phi$, which is defined as: \begin{equation*} \Phi_{\beta, N} = \frac{1}{N} ln Z_{\beta, N} \end{equation*} With Z the partition function: \begin{equation*} Z_{\beta, N} = \frac{1}{2^N} \sum\limits_{\sigma \in S_{N}}^{} e^{\beta \sqrt{N} X_{\sigma}} \end{equation*}
In this formulation of the model, the expectation of $\Phi$ has a very interesting property: it turns out that the law of large numbers holds up to a certain level of $\beta$ which we call the critical value $\beta_{c}$. Thus, up to this point it holds that $Z_{\beta, N} \sim E(Z_{\beta, N})$ and for $\beta > \beta_{c}$ a breakdown of the law of large numbers occurs. For a system of normally distributed $X_\sigma$ we have the following ground-state energy : \begin{equation} \lim_{N\to\infty} max_{\sigma \in S_{N}} \frac{X_{\sigma}}{\sqrt{N}} = \sqrt{2ln(2)}, a.s. \end{equation} We want to follow the proof of Anton Bovier (Statistical Mechanics of Disordered Systems, Theorem 9.1.2) that the expectation of $\Phi$ now behaves in the following way: $ \lim_{N\to\infty} E(\Phi_{\beta,N}) = \begin{cases} \frac{\beta^{2}}{2}, & \beta \leq \beta_{c} \\ \frac{\beta^{2}}{2} + (\beta - \beta_{c})\beta{c} ,&\beta \geq \beta_{c} \\ \end{cases} $
From the previous we can derive that $E(\frac{d}{d\beta})\Phi \leq N^{-1/2} E(max_{\sigma \in S_{N}}X_{\sigma})$. Bovier now concludes the follwing two things:
1) $E(\frac{d}{d\beta})\Phi \leq N^{-1/2} E(max_{\sigma \in S_{N}}X_{\sigma}) \leq \beta \sqrt{2ln2} (1+C/N)$ with C a constant.
2) $E(\Phi) \leq \frac{\beta_{0}^2}{2} + (\beta - \beta_{0})\sqrt{2ln2}(1+C/N) = ln{2} + (\beta - \sqrt{2ln2})\sqrt{2ln2}(1+C/N)$
I have no idea of how the $\beta$ and the constant $C$ pop up in the first equation, nor how the second expression follows from the first. Do you have any ideas?