The local characterizations of the singularity formation for the MHD equations
Abstract
This paper characterizes the possible blow-up of solutions for the 3D magneto-hydrodynamics (MHD for short) equations. We first establish some ε-regularity criteria in Lq,∞ spaces for suitable weak solutions, and then together with an embedding theorem from Lp,∞ space into a Morrey type space to characterize the local behaviors of solutions near a potential singular point. More precisely, we show that if z0=(t0, x0) is a singular point, then for any r>0 it holds that t → t0-(\|u(t, x)-u(t)x0, r\|L3, ∞(Br(x0))+\|b(t, x)-b(t)x0, r\|L3, ∞(Br(x0)))>δ*; t → t0-(t0-t)1μ r2-3p\|(u,b)(t)\|Lp, ∞(Br(x0))>δ* for 1μ+1=12,\,2 ≤ ≤ 2 p3,\, 3<p≤∞; t → t0-(t0-t)1μ r2-3p+1\|(∇ u,∇ b)(t)\|Lp(Br(x0))>δ* for 1μ+1=12,\, ∈\arrayll [2, ∞], & p≥ 3 [2, 2p3-p], & 32≤ p<3 array. where δ* is a positive constant independent on and p.
Turn this paper into a lesson
ArcXiv compiles a structured reading guide from this paper's metadata: plain-English importance, contributions, prerequisite concepts, which sections to read first, flashcards, and a quiz. Grounded in the abstract, never invented.