The APDE seminar on Monday, 3/9, will be given by Jesús Oliver (Cal State East Bay) in-person in Evans 736, and will also be broadcasted online via Zoom from 4:10pm to 5:00pm PST. To participate, please email Adam Black (adamblack@berkeley.edu).
Title: Global existence for a Fritz John equation in expanding FLRW spacetimes
Abstract: We study the semilinear wave equation
\[\square_{\mathbf g_p}\phi = (\partial_t \phi)^2\]
on expanding FLRW spacetimes with spatial slices $\mathbb{R}^3$ and power-law scale factor $a(t)=t^p$, where $0 < p \le 1$. This equation extends the classical Fritz John blow-up model on Minkowski space (the case $p=0$) to a non-stationary cosmological background.
In Minkowski space, nontrivial solutions arising from smooth, compactly supported data blow up in finite time. In contrast, we prove that for $0 < p \le 1$, sufficiently small, smooth, compactly supported initial data generate global-in-time solutions toward the future.
Earlier joint work with Costa and Franzen treated the accelerated regime $p>1$, where global existence follows from the integrability of the inverse scale factor. In the present setting, this mechanism is unavailable. Instead, we develop a vector field method adapted to FLRW geometry that exploits the interaction between dispersion and spacetime expansion to suppress the nonlinear blow-up mechanism. The argument relies on commuting the Laplace–Beltrami operator with a boosts-free subset of the Poincaré algebra and establishing Klainerman–Sideris type estimates adapted to the non-stationary background.
The approach provides a robust framework for quantifying the regularizing effect of cosmological expansion and is expected to extend to a broader class of nonlinear wave equations.