We prove the boundedness of global classical solutions for the semilinear
heat equation ut−Δu=∣u∣p−1u in the whole space Rn, with n≥3 and supercritical power p>(n+2)/(n−2). This is proved {\rmb without any
radial symmetry or sign assumptions}, unlike in all the previously known
results for the Cauchy problem, and under spatial decay assumptions on the
initial data that are essentially optimal in view of the known
counter-examples. Moreover, we show that any global classical solution has to
decay in time faster than t−1/(p−1), which is also optimal and in contrast
with the subcritical case.
The proof relies on nontrivial modifications of techniques developed by Chou,
Du and Zheng [Calc. Var. PDE 2007] and by Blatt and Struwe [IMRN, 2015] for the
case of convex bounded domains. They are based on weighted energy estimates of
Giga-Kohn type, combined with an analysis of the equation in a suitable Morrey
space. We in particular simplify the approach of Blatt and Struwe by
establishing and using a result on global existence and decay for small initial
data in the critical Morrey space M2,4/(p−1)(Rn), rather than
\eps-regularity in a parabolic Morrey space. This method actually works for
any convex, bounded or unbounded, smooth domain, but at the same time captures
some of the specific behaviors associated with the case of the whole space
Rn.
As a consequence we also prove that the set of initial data producing global
solutions is open in suitable topologies, and we show that the so-called
"borderline" global weak solutions blow up in finite time and then become
classical again and decay as t→∞. All these results put into light the
key role played by the Morrey space M2,4/(p−1) in the understanding of the
structure of the set of global solutions for p>pS.Comment: 29 page