Non-self similar blowup solutions to the higher dimensional Yang-Mills heat flows
A. Bensouilah, G. K. Duong, T. E. Ghoul
TL;DR
This work constructs non-self-similar (Type II) blow-up solutions for the higher-dimensional Yang-Mills heat flow in dimensions $d\ge 11$ under an $SO(d)$-equivariant symmetry. It develops a time-dependent spectral framework around a moving ground state $Q_b$, introducing blow-up variables and a dynamic operator $\mathscr{L}_b$, and proves both stable and unstable blow-up regimes via a shrinking-set bootstrap, finite-dimensional reduction, and maximum-principle techniques. Central to the approach is the precise diagonalisation of $\mathscr{L}_b$ through matched inner/outer eigenfunctions, yielding blow-up speeds $\lambda_ℓ(t) = C(u_0)(T-t)^{\frac{2ℓ}{\alpha}}$ with stability properties: stable for $\ell=1$ and codimension $\ell-1$ for $\ell\ge 2$. The results also establish the existence and properties of the ground state $Q$ and provide a robust analytical framework that combines spectral analysis with parabolic maximum principles, applicable to other nonlinear parabolic PDEs with Type II blow-up.
Abstract
In this paper, we consider the Yang-Mills heat flow on $\mathbb R^d \times SO(d)$ with $d \ge 11$. Under a certain symmetry preserved by the flow, the Yang-Mills equation can be reduced to: $$ \partial_t u =\partial_r^2 u +\frac{d+1}{r} \partial_r u -3(d-2) u^2 - (d-2) r^2 u^3, \text{ and } (r,t) \in \mathbb R_+ \times \mathbb R_+. $$ We are interested in describing the singularity formation of this parabolic equation. We construct non-self-similar blowup solutions for $d \ge 11$ and prove that the asymptotic of the solution is of the form $$ u(r,t) \sim \frac{1}{λ_\ell(t)} \mathcal{Q} \left( \frac{r}{\sqrt{λ_\ell (t)}} \right), \text{ as } t \to T ,$$ where $\mathcal{Q}$ is the ground state with boundary conditions $\mathcal{Q}(0)=-1, \mathcal{Q}'(0)=0$ and the blowup speed $λ_\ell$ verifies $$λ_\ell (t) = \left( C(u_0) +o_{t\to T}(1) \right) (T-t)^{\frac{2\ell }α} \text{ as } t \to T,~~ \ell \in \mathbb{N}^*_+, ~~α>1.$$ In particular, when $\ell = 1$, this asymptotic is stable whereas for $ \ell \ge 2$ it becomes stable on a space of codimension $\ell-1$. Our approach here is not based on energy estimates but on a careful construction of time dependent eigenvectors and eigenvalues combined with maximum principle and semigroup pointwise estimates.
