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Collapse vs. blow up and global existence in the generalized Constantin-Lax-Majda equation

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arxiv 2010.01201 v2 pith:FRMZIUHR submitted 2020-10-02 nlin.PS nlin.SIphysics.flu-dyn

classification nlin.PSnlin.SIphysics.flu-dyn
keywords solutionfindsingularitysolutionsblow-upcollapsingexistencetime
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abstract

The question of finite time singularity formation vs. global existence for solutions to the generalized Constantin-Lax-Majda equation is studied, with particular emphasis on the influence of a parameter $a$ which controls the strength of advection. For solutions on the infinite domain we find a new critical value $a_c=0.6890665337007457\ldots$ below which there is finite time singularity formation % if we write a=a_c=0.6890665337007457\ldots here then \ldots doesn't fit into the line that has a form of self-similar collapse, with the spatial extent of blow-up shrinking to zero. We find a new exact analytical collapsing solution at $a=1/2$ as well as prove the existence of a leading order complex singularity for general values of $a$ in the analytical continuation of the solution from the real spatial coordinate into the complex plane. This singularity controls the leading order behaviour of the collapsing solution. For $a_c<a\leq1$, we find a blow-up solution in which the spatial extent of the blow-up region expands infinitely fast at the singularity time. For $a \gtrsim 1.3$, we find that the solution exists globally with exponential-like growth of the solution amplitude in time. We also consider the case of periodic boundary conditions. We identify collapsing solutions for $a<a_c$ which are similar to the real line case. For $a_c<a\le0.95$, we find new blow-up solutions which are neither expanding nor collapsing. For $ a\ge 1,$ we identify a global existence of solutions.

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  1. The spectral picture of self-similar collapse in the Constantin-Lax-Majda equation

    physics.flu-dyn 2026-07 conditional novelty 7.0 of 10

    On the origin-H2 realization, the CLM collapse linearization has essential spectrum Re λ = -1/2 and point spectrum {0,1}, hence a spectral gap 1/2; weaker L2 realizations fill the whole strip.

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