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Nailya Manatova

Publications and source records attributed to Nailya Manatova.

2 recordsLinked to original sources

Slowly travelling infinite point blow-up for the critical generalized KdV equation

We study the finite time blow up phenomenon for the quintic, mass critical gKdV equation. We prove the existence of a class of solutions $U$ with infinite point, finite time blow up behavior, at the particular blow up rate $$\|\partial_x U(t)\|_{L^2} \sim (T-t)^{-ν}\quad \text{as} \quad t \uparrow T,$$ where $ν= \frac 12$, $T$ is the blow up time and where the travel speed of the blow up bubble is logarithmic. Therefore, we call this behaviour slowly travelling infinite point blow up. The special blow up rate $ν=\frac 12$ is a threshold which separates finite and infinite point bubbling. In a previous work arXiv:2511.13538, the author constructed other infinite point blow up solutions for the continuum of rates $ν\in(\frac 12,1)$, using polynomial tails in the space variable and extending the results in arXiv:1209.2510, restricted to $ν> \frac{11}{13}$. However, that work suggested a change of the tail for the threshold case. In the present paper, we consider an exponentially decaying tail on the right in space. As in arXiv:2511.13538, the initial data can be taken arbitrarily close to the ground state in $H^1$. From a technical perspective, in addition to the change of tail, we have to adapt the energy-virial functional to the presence of the exponential tail, by modifying a scaling term used to control the right-hand side of the blow up solution.

math.AP↗

Full range of infinite point blow-up exponents for the critical generalized KdV equation

For the quintic, mass critical generalized Korteweg-de Vries equation, for any $ν\in (\frac{1}{2}, 1)$, we prove the existence of solutions in the energy space that blow up in finite time $T>0$ with the blow-up rate $\|\partial_x u(t)\|_{L^2} \sim (T-t)^{-ν}$ (infinite point blow-up). These solutions are constructed arbitrarily close to the family of solitons and correspond to the concentration of a soliton traveling at $+\infty$ in space as $t\uparrow T$. This complements the previous results obtained in the work of Martel, Merle, Raphaël in 2015 on infinite point exotic blow-up, which were valid under the technical restriction $ν>\frac {11}{13}$. The value $ν=\frac 12$ corresponds to a critical case to be treated elsewhere. At the technical level, we implement a modification of the virial-energy functional, to allow all $ν> \frac 12$ and simplify the proof of energy estimates.

math.AP↗