Abstract:We show that the finite time type II blow up solutions for the energy critical nonlinear wave equation u "´u 5 on R 3`1 constructed in [28], [27] are stable along a co-dimension three manifold of radial data perturbations in a suitable topology, provided the scaling parameter λptq " t´1´ν is sufficiently close to the self-similar rate, i. e. ν ą 0 is sufficiently small. Our method is based on Fourier techniques adapted to time dependent wave operators of the forḿfor suitable monotone scaling parameters λptq an… Show more
“…In the energy critical case, u T is the unique self-similar solution and it can be used to construct blowup solutions that diverge in the scale invariant norṁ H 1 × L 2 (R 3 ), cf. for example [30]. This behavior is referred to as type I and contrasted by type II blowup, where solutions stay bounded in the critical norm.…”
We consider semilinear wave equations with focusing power nonlinearities in odd space dimensions d ≥ 5. We prove that for every p > d+3 d−1 there exists an open set of radial initial data in Hsuch that the corresponding solution exists in a backward lightcone and approaches the ODE blowup profile. The result covers the entire range of energy supercritical nonlinearities and extends our previous work for the three-dimensional radial wave equation to higher space dimensions.
1(1.5)By setting Ψ T (τ ) := (ψ T 1 (τ, ·), ψ T 2 (τ, ·)) this can be written aswhere L 0 represents the linear part of the right hand side of Eq. (1.5). To formulate the following statement we define for k ∈ N 0 H k rad (B d ) := {u ∈ H k (B d ) : u is radial}.
“…In the energy critical case, u T is the unique self-similar solution and it can be used to construct blowup solutions that diverge in the scale invariant norṁ H 1 × L 2 (R 3 ), cf. for example [30]. This behavior is referred to as type I and contrasted by type II blowup, where solutions stay bounded in the critical norm.…”
We consider semilinear wave equations with focusing power nonlinearities in odd space dimensions d ≥ 5. We prove that for every p > d+3 d−1 there exists an open set of radial initial data in Hsuch that the corresponding solution exists in a backward lightcone and approaches the ODE blowup profile. The result covers the entire range of energy supercritical nonlinearities and extends our previous work for the three-dimensional radial wave equation to higher space dimensions.
1(1.5)By setting Ψ T (τ ) := (ψ T 1 (τ, ·), ψ T 2 (τ, ·)) this can be written aswhere L 0 represents the linear part of the right hand side of Eq. (1.5). To formulate the following statement we define for k ∈ N 0 H k rad (B d ) := {u ∈ H k (B d ) : u is radial}.
“…Many recent works focus on energy-critical equations where type II blowup solutions are studied that emerge from a dynamical rescaling of a soliton, e.g. [29,41,12,11,39,18,21,23,24,17,20,19,27], see also [42,38,36,37].…”
Section: Related Workmentioning
confidence: 99%
“…• The topology in which we consider the problem is optimal in the class of Sobolev spaces H k × H [29,41,12,11,39,18,21,23,24,17,20,19,27], see also [42,38,36,37]. In the supercritical case, blowup is typically self-similar.…”
We study the blowup behavior for the focusing energysupercritical semilinear wave equation in 3 space dimensions without symmetry assumptions on the data. We prove the stability in H 2 × H 1 of the ODE blowup profile.
“…The author and Schörkhuber [16,18,17] proved the asymptotic stability of the ODE blowup profile, but in the stronger topology H 2 × H 1 . We also mention the recent paper by Krieger and Wong [44] on continuation beyond type II singularities. Unfortunately, the impressive machinery [48,49,50,51,53,52] developed by Merle and Zaag for studying type I blowup is confined to energy-subcritical equations and does not apply here.…”
Abstract. We establish Strichartz estimates in similarity coordinates for the radial wave equation in three spatial dimensions with a (time-dependent) self-similar potential. As an application we consider the critical wave equation and prove the asymptotic stability of the ODE blowup profile in the energy space.
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