A Geometric Origin for the Duration of Inflation Why the Number $6\pi^2$ Appears Inflation is usually described dynamically: a scalar field rolls, spacetime expands quasi-exponentially, and the universe accumulates roughly $N_e \sim 50\text{--}60$ e-folds. But there is a striking geometric number sitting right in that range: $$6\pi^2 \approx 59.22.$$ The point of this note is not to claim that inflation is explained by geometry alone. The claim is narrower: the number $6\pi^2$ arises naturally as an exact self-dual $SU(2)$-invariant closure measure on the $S^3$ slice of Euclidean de Sitter space. With one further physical ingredient — a conserved bulk flow matched to a boundary closure charge — that same invariant becomes an inflationary e-fold count. 1. The Boundary Gives $4\pi$ Take the observer screen to be a closed two-sphere, $\Sigma_2 \simeq S^2$. Its intrinsic-curvature closure is fixed by Gauss–Bonnet: $$I_c \equiv \int_{\Sigma_2} K,dA = 2\pi \chi(\Sigma_2).$$ ...
Yes! Also, it is not the 'Planck Power' (despite what you might have read in Misner, Thorne and Wheeler, P.980). The existence of black hole horizons implies a maximum luminosity (power) limit in General Relativity. Not even gravitational waves can escape a black hole . Consider an (almost) black hole made of light (this is called a Kugelblitz ) sphere of radius \begin{equation} \notag R \geq \frac{2Gp}{c^3} \end{equation} which is filled with photons with a total mass-energy of momentum $p$ times speed of light $c$ \begin{equation} \notag E=p \ c \end{equation} that leave after a time \begin{equation} \notag t=R/c \end{equation} with average power (luminosity) \begin{equation} \notag P_{max} = \frac{E}{t}=\frac{p \ c^2}{R}=\frac{c^5}{2G} \approx 1.8\times10^{52} \ W \end{equation} This is maximum power in GR , regardless of the nature of the system. You might be tempted to call this half a 'Planck Power' but there is no $\h...