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Oscillatory behavior of solutions to the critical Fujita equation in 6D

Junichi Harada

TL;DR

The article analyzes the long-time dynamics of the energy-critical Fujita equation in 6 dimensions, constructing three classes of global radially symmetric solutions with a leading Aubin–Talenti profile $u(x,t)\approx\lambda(t)^{-(n-2)/2}Q(x/\lambda(t))$ and a vanishing error in $\dot H^1$. It uses an inner-outer gluing framework and matched asymptotics to manipulate a modulation parameter $\lambda(t)$, producing both monotone and oscillatory behaviors; in particular, the oscillatory solution exhibits $\liminf_{t\to\infty}\lambda(t)=0$ and $\limsup_{t\to\infty}\lambda(t)=\infty$. The construction relies on a careful analysis of the linearized operator around the ground state, tail decay via the linear heat equation, and a fixed-point argument that couples the inner core with an outer tail. This work highlights a novel dynamic regime in which $\dot H^1$ dynamics can diverge significantly from $H^1$ behavior, revealing intricate, nonstatic evolution near the energy-critical ground state in the 6D setting.

Abstract

Long time dynamics of solutions to the 6D energy critical heat equation $u_t=Δu+|u|^{p-1}u$ on $\R^6\times(0,\infty)$ is investigated. It is shown that there exists a radially symmetric global solution $u(x,t)\in C([0,\infty);\dot H^1(\R^6))$ of the form \begin{align*} u(x,t) = λ(t)^{-\frac{n-2}{2}} {\sf Q}(\tfrac{x}{λ(t)}) + \text{error} (x,t), \end{align*} where the function \( λ(t) \) satisfies: \begin{itemize} \item $\dis\lim_{t\to\infty}\|\text{error}(\cdot,t)\|_{\dot H_x^1(\R^6)}=0$, \item $\dis\liminf_{t\to\infty}λ(t)=0$, \item $\dis\limsup_{t\to\infty}λ(t)=\infty$. \end{itemize} The solutions constructed here demonstrate that the dynamical behavior in \( \dot H^1(\mathbb{R}^n) \) can differ significantly from the behavior in \( H^1(\mathbb{R}^n) \).

Oscillatory behavior of solutions to the critical Fujita equation in 6D

TL;DR

The article analyzes the long-time dynamics of the energy-critical Fujita equation in 6 dimensions, constructing three classes of global radially symmetric solutions with a leading Aubin–Talenti profile and a vanishing error in . It uses an inner-outer gluing framework and matched asymptotics to manipulate a modulation parameter , producing both monotone and oscillatory behaviors; in particular, the oscillatory solution exhibits and . The construction relies on a careful analysis of the linearized operator around the ground state, tail decay via the linear heat equation, and a fixed-point argument that couples the inner core with an outer tail. This work highlights a novel dynamic regime in which dynamics can diverge significantly from behavior, revealing intricate, nonstatic evolution near the energy-critical ground state in the 6D setting.

Abstract

Long time dynamics of solutions to the 6D energy critical heat equation on is investigated. It is shown that there exists a radially symmetric global solution of the form \begin{align*} u(x,t) = λ(t)^{-\frac{n-2}{2}} {\sf Q}(\tfrac{x}{λ(t)}) + \text{error} (x,t), \end{align*} where the function \( λ(t) \) satisfies: \begin{itemize} \item , \item , \item . \end{itemize} The solutions constructed here demonstrate that the dynamical behavior in \( \dot H^1(\mathbb{R}^n) \) can differ significantly from the behavior in \( H^1(\mathbb{R}^n) \).

Paper Structure

This paper contains 28 sections, 22 theorems, 322 equations, 1 table.

Key Result

Theorem 1

Let $n=6$ and $p=\frac{n+2}{n-2}$. For any $\beta\in(\frac{1}{2},1)$, there exist a constant $t_I>0$ and a global, positive, radially symmetric solution solution $u_\beta(x,t)$ satisfying (c1) - (c3), such that where $\lambda_\beta(t)$, $\chi_1$ and $\text{\rm error}_1(x,t)$ are given as follows:

Theorems & Definitions (40)

  • Theorem 1: Positive $\dot H^1$-Solution
  • Theorem 2: Sign-Changing $\dot H^1$-Solution
  • Theorem 3: Oscillatory $\dot H^1$-Solution
  • Remark 2.1
  • Remark 2.2
  • Remark 2.3
  • Remark 2.4
  • Lemma 3.1
  • Lemma 3.2: Lemma 3.1-Lemma 3.2 Harada_5D p. 312
  • Lemma 3.3: Lemma 7.2 Cortazar-delPino-Musso, Lemma 3.3 Harada_5D p. 313
  • ...and 30 more