by ˙ φ$_{i}$ . If ˙ φ 2 i > 2 V ( φ$_{i}$ ), the kinetic dominance prevails. In principle the inflaton will overshoot the point of inflection only if it begins very close to φ$_{0}$ and has a large negative velocity initially. It is interesting to note that φ can end up above the point of inflection even if φ$_{i}$ < φ$_{0}$ , provided that ˙ φ$_{i}$ > 3 H$_{false}$ ( φ$_{0}$ − φ$_{i}$ ). The most important regime is (3) the slow-roll regime: which we will discuss below. Once an initial phase of oscillations or kinetic energy dominance ends, φ starts a slow-roll motion towards the inflection point, φ$_{0}$ . The equation of motion in this regime is 3 H$_{false}$ ˙ φ + V ′ ( φ ) ≈ 0. Initially the field is under the influence of the non-renormalizable potential, i.e. V ( φ ) ∝ φ $^{10}$, see Eq. (317), however, as φ moves toward φ$_{0}$ , the φ 10 term becomes increasingly smaller. Eventually, for φ ≈ φ$_{0}$ , we have V ′ ( φ ) = V ′ ( φ$_{0}$ ) + V ′′′ ( φ$_{0}$ )( φ − φ$_{0}$ ) $^{2}$/ 2. It happens that this is the longest part of φ journey. It is desirable to find how long does it take for φ to reach the edge of the plateau in Eq. (324). Outside the plateau, V ′ ( φ$_{0}$ ) is subdominant, see Eqs. (322, 323), and hence: This results in for large t . Therefore the inflection point acts as an attractor for the classical equation of motion. After using Eq. (324), t$_{slow}$ > ∼ 10 10 e-foldings of false vacuum inflation (note that φ$_{0}$ ∼ 10 14 GeV, and H$_{false}$ > m$_{φ}$ ∼ O (100) GeV). After this time φ is settled within the plateau in the bulk of the inflating space. This implies that the bubbles which nucleate henceforth have the right initial conditions for a subsequent stage of MSSM inflation. Let us consider the bubbles that have the right initial conditions for MSSM inflation, i.e. φ has settled in the plateau around a point of inflection according to Eq. (324). The initial size of the bubble is r$_{0}$ $_{< H}$− 1 $_{false}$. Inside of an expanding bubble has the same geometry as an open FRW universe. The Hubble rate inside the bubble is therefore given by [284] 3. Inflating the MSSM bubble ˙ φ = − 32 m 2 $_{φ}$( φ − φ$_{0}$ ) 2 3 H$_{false}$φ$_{0}$ . (363) ( φ − φ$_{0}$ ) ≈ 3 H$_{false}$φ$_{0}$ 32 m 2 $_{φ}$t , (364) H 2 = V$_{φ}$ + V$_{ϕ}$ 3 M 2 P + 1 a $_{2}$, (365) 168