content_image/316624.jpg content_image/316622.jpg content_image/316623.jpg content_image/316625.jpg content_image/316626.jpg content_image/316620.jpg content_image/316621.jpg
As we are considering the time of the end of primordial inflation, | m$_{φ,}$$_{eff}$ | ∼ g T$_{end,inf}$ , as given by Eq. (4.99). Therefore we have 

So, we now have 

<img src='content_image/316624.jpg'>

<img src='content_image/316622.jpg'>

<img src='content_image/316623.jpg'>

where A is a constant of integration. We can obtain A by equating Eq. (A.30) with Eq. (A.14) and setting κ = τ =0 . We obtain 

<img src='content_image/316625.jpg'>

<img src='content_image/316626.jpg'>

Given that | m$_{φ,}$$_{eff}$ | ∼ g T$_{end,inf}$ , we have κ = g . Therefore Eq. (A.30) becomes 

For all values of g , i.e. g ≤ 1 , we have 

<img src='content_image/316620.jpg'>

<img src='content_image/316621.jpg'>

