DUT Differential Equations Seminar (DDES)

The attractor is an important concept in dynamical systems, which can be used to characterize the long time asymptotic behavior of systems. In this talk, we will discuss random attractors for McKean-Vlasov stochastic differential equations (in short, MVSDEs). A difficulty arises from the distribution dependence in MVSDEs, which breaks the flow property of solutions. To address this, we consider the random attractor on product space $H\times \mathcal{P}(H)$, where $H$ is a separable Hilbert space and $\mathcal{P}(H)$ denotes the space of probability measures on $H$. This is based on a joint work with Xianjin Cheng and Zhenxin Liu.

This talk primarily presents singularity criteria for solutions to the compressible Navier-Stokes equations. It further extends a previously proven conjecture of Nash. Another part establishes the global existence of solutions for the MHD equations where the viscosity coefficients depend on the density. In this case, the initial density can be arbitrarily large.

As is well-known, the solution of the Patlak-Keller-Segel system in 3D will blow up in finite time regardless of any initial cell mass. In this talk, we are interested in the suppression of blow-up for the 3D Patlak-Keller-Segel-Navier-Stokes system via the stabilizing effect of the moving fluid. We prove that if the Couette flow is sufficiently strong, then the solutions for the system are global in time. This is a joint work with Shikun Cui, Wendong Wang and Juncheng Wei.

In this talk, we study the spectral stability of the standing periodic waves in the massive Thirring model. The Massive Thirring Model is complete integrable, the spectral stability of the standing periodic waves can be studied by using their Lax spectrum. We show analytically that each family of standing periodic waves is distinguished by the location of eight eigenvalues which coincide with the end points of the spectral bands of the Lax spectrum. The standing periodic waves are proven to be spectrally stable if the eight eigenvalues are located either on the imaginary axis or along the diagonals of the complex plane. By computing the Lax spectrum numerically, we show that this stability criterion is satisfied for some standing periodic waves. This is joint work with Prof. Dmitry Pelinovsky.

This report is about the traveling wave solutions to the pseudo-parabolic equation, a kind of non-classical diffusion equation characterized by the mixed third-order derivative term. We demonstrate that the ratio of the mixed third-order derivative coefficient to the diffusion coefficient $\frac{\tau}{D}$ can serve as a bifurcation parameter. In detail, when $\frac{\tau}{D}\leq1$, the equation possesses monotone traveling waves; when $\frac{\tau}{D}>1$, traveling waves are not monotonic and oscillate around the steady state $u=1$. The precise form of the minimal wave speed $c^*(\tau,D)$ is also derived, exhibiting a monotonic increase with respect to $\tau$ and converging to $2\sqrt{D}$ as $\tau$ approaches 0. Numerical simulations confirm and support our theoretical results. They further show that the larger the value of $\tau$ is, the more non-monotonic the traveling waves become. Our findings regarding oscillating traveling waves predict saturation overshoot—a behavior that contradicts classical diffusion-like behavior yet is widely observed in unsaturated porous media. Mathematically, the threshold value of $\frac{\tau}{D}$ reveals the essential role of the dynamic capillary effect in the fundamental overshoot mechanism.

We propose a first-order, time-discrete stochastic consensus model for global optimization. The model draws on interaction-based mechanisms to incorporate objective-function information and handles non-convex, non-differentiable, and even discontinuous functions. It is motivated by the Consensus-Based Optimization (CBO) paradigm, which promotes consensus among agents toward a global optimum through simple stochastic dynamics amenable to rigorous mathematical analysis. Despite these promises, the actual behavior of agents in its time-discrete implementation remains largely unknown. We address this issue by the novel observation that the consensus point governs the entire ensemble. We further demonstrate competitive performance across various problems.

Mean motion resonance (MMR), a phenomenon occurring when two celestial bodies have orbital periods in a commensurable ratio, plays a pivotal role in both stabilizing and destabilizing orbital motions within the Solar System. For highly eccentric orbits, the risk of close encounters introduces significant complexity. When such eccentric orbits are trapped in resonance, perturbations can induce chaotic motions, leading to rapid changes in orbital elements and transitions of different dynamical states. In this talk, we will numerically demonstrate the limits of application of canonical perturbation theory, specifically the validity of the normal form approximations, for the study of MMRs of the circular restricted three-body problem in the domain of orbits which cross, or are close to cross, the orbit of the secondary body. The external 1:2 and 5:6 MMRs for values of the mass ratios representing the Sun-Jupiter and Sun-Neptune cases will be used as model examples.

Yang-Mills theory is fundamental for both mathematics and theoretical physics. It underlies electrodynamics with the first unitary group U(1) as gauge group or quantum chromodynamics with the third special unitary group SU(3) as gauge group. It has also lead to a deeper understanding of four-dimensional manifolds, for example the Fields Medal winning proof of Donaldson’s theorem. All applications are based on the study of the Yang-Mills equations, which are partial differential equations of second order as well as linear for an abelian gauge group and non-linear for a non-abelian gauge group. Since the formulation of the Yang-Mills equations connects differential forms with Lie algebras, a differential and algebraic perspective are inseparable in Yang-Mills theory.

In this talk, I will introduce some uniqueness of inverse source scattering and inverse obstacle scattering problems with multi-frequency data. I will also present some direct sampling methods for inverse source scattering problems. With sparse data, these numerical methods can reconstruct the support of source. The stability estimation based on dense data are also provided. Additionally, I will propose some direct sampling methods for the simultaneous reconstruction of both the obstacle shape and the impedance value in the context of inverse acoustic scattering problems, backscattering data are used in this problem.

Assume $n\geq3$ and $u\in \dot{H}^1(\mathbb{R}^n)$. Recently, Piccione, Yang and Zhao [JDE, 2025] established a nonlocal version of Struwe's decomposition, i.e., if $\Gamma(u):=\left\|\Delta u+D_{n,\alpha}\int_{\mathbb{R}^{n}}\frac{|u|^{p_{\alpha}}(y) }{|x-y|^{\alpha}}\mathrm{d}y |u|^{p_{\alpha}-2}u\right\|_{H^{-1}}\rightarrow0$ and $u\geq 0$, then $dist(u,\mathcal{T})\to 0$, where $dist(u,\mathcal{T})$ denotes the $\dot{H}^1(\mathbb{R}^n)$-distance of $u$ from the manifold of sums of Talenti bubbles. In this paper, we establish the nonlocal version of the quantitative estimates of Struwe's decomposition in Ciraolo, Figalli and Maggi [IMRN, 2018] for one bubble and $n\geq3$, Figalli and Glaudo [Arma, 2021] for $3\leq n\leq5$ and Deng, Sun and Wei [Duke, 2025] for $n\geq6$ and two or more bubbles. We prove that for $n\geq 3$, $\alpha\le n$ and $0\le \alpha\leq 4$, $$ dist (u,\mathcal{T})\leq C\begin{cases} \Gamma(u)\left|\log \Gamma(u)\right|^{\frac{1}{2}}\quad&\text{if } \,\, n=6 \,\, \text{and} \,\, \alpha=4,\\ \Gamma(u) \quad&\text{for any other cases.}\end{cases} $$ Furthermore, we show that this inequality is sharp for $n=6$ and $\alpha=4$.

In this talk, we focus on the life span estimates of solutions to semilinear heat equations with inner and initial sources. We first prove that solutions blow up in finite time when only a single inner source non-rarefied at infinity, and derive the optimal upper and lower bounds on the life span. In recent work, we find only a single source dominates the asymptotic life span in this model with non-trivial non-negataive scaled sources, and establish sharp asymptotic estimates of life span on blow-up solutions.

Seiberg-Witten theory is fundamental for both mathematics and theoretical physics. It was derived from N = 2 supersymmetric Yang-Mills theory and then effectively applied to the study of four-dimensional manifolds. This was a remarkable instance of mathematics gaining from theoretical physics instead of the usual other way around. Seiberg-Witten invariants, based on the Seiberg-Witten equations with the abelian gauge group U(1), also both extended and simplified calculations of Donaldson invariants, based on the Yang-Mills equations with the non-abelian gauge group SU(2), which also concerns the study of four-dimensional manifolds. This was another remarkable aspect since an abelian theory is in many aspects simpler than a non-abelian theory. Seiberg-Witten theory is in particular able to distinguish smooth structures on four-dimensional manifolds, based on the fact that they are encoded in partial differential equations on it like the Seiberg-Witten equations. But the smooth Poincaré conjecture about smooth structures on the four-dimensional sphere is still open, so research continues to find other partial differential equations to encode the necessary information, which could come from physics again.

In 2004, Dombrowski et al. demonstrated that suspensions of aerobic bacteria often generate fluid flows through the interplay of chemotaxis and buoyancy, described by the chemotaxis-Navier-Stokes model, and observed self-concentration manifesting as turbulence characterized by transient, self-reconstituting, high-speed jets that entrain nearby fluid to form paired, oppositely signed vortices. Investigating the properties of these vortices (singular points) is of significant interest, and one approach is to follow the partial regularity theory of Caffarelli-Kohn-Nirenberg in studying the singularity properties of suitable weak solutions. In this paper, we first establish the existence of suitable weak solutions for the three-dimensional chemotaxis-Navier-Stokes equations, where the primary difficulty lies in deriving an appropriate local energy inequality of weak type. Moreover, we derive a new a priori estimate for the linear chemotaxis-Stokes model and present several $\varepsilon$-regularity criteria.

Scalar balance laws are advection-reaction equations, that appear either in biology or physic when one mesures the variation of a quantity over time. In this presentation, we will focus on specific solutions of these equations, namely propagated waves that connect two distinct constant states. A large variety of such waves can be constructed, and we will discuss the stability of some of them. It is a joint work with L. M. Rodrigues.

The Klein-Gordon equation is a wave equation with an additional mass damping term. In this presentation, I will review some literature about the dynamic of such equation when settled on an unbounded one-dimensional spatial domain. I will further present some new results regarding the global existence and long time behaviour of solutions that are initialy close to constant or periodic equilibria. Most notably, I will talk about a viscous approximation of this equation, as well as describe how uniformly local orbital stability can be obtained from polar decomposition. This is joint work with Björn de Rijk and Emile Bukieda.

We introduce the NLS hierarchy and discuss its well-posedness with a nonzero boundary condition. Here the main difficulty is local well-posedness, since good conserved energies have already been constructed by H. Koch and X. Liao. We adopt a perturbative formulation and determine its structure sufficiently in order to apply techniques for general dispersive nonlinear PDE.

We consider long-wave solutions to the NLS hierarchy with nonzero boundary condition. Rewriting the conserved energies and momenta in hydrodynamic variables, we find that they are approximated by the conserved energies of the KdV hierarchy. Combining this with a similar approximation of the symplectic structures yields a formal approximation result for tthe hierarchies. We quantify this using energy estimates and previously established well-posedness results.

We shall discuss the global nonlinear stability of vortex sheets for the Navier-Stokes equations. When the Mach number is small, we allow both the amplitude and the initial vorticity of the vortex sheets to be large. We introduce an auxiliary flow and reformulate the problem as a new vortex sheet with small vorticity but subjected to a large perturbation. Based on the decomposition of frequency, the largeness of the perturbation is encoded in the zero modes of the tangential velocity. We find an essential cancellation property that there are no nonlinear interactions among these large zero modes in the zero-mode perturbed system. This cancellation is owing to the shear structure inherent in the vortex sheets. These observations enable us to derive the global estimates for strong solutions that are uniform with respect to the Mach number. As a byproduct, we can justify the incompressible limit.

Einstein's Field Equations describe gravity as the curvature of spacetime. Following the discovery of the equivalence of energy and mass, an expansion of Newton's theory of gravity became necessary. Since it doesn't treat the motion or rotation of celestial bodies as a source of gravity, although these carry kinetic and rotational energy, a contradiction appears. Fixing it requires an expansion to combine all these information. In particular the new prospect that then even gravity becomes its own source, since gravitational waves also carry energy, leads to a non-linear formulation and the precise partial differential equations were in development for an entire decade. By now, their unique structure has been studied for over a century. Countless strange solutions, for example allowing time travel, have already been found.

We consider quasilinear partially dissipative hyperbolic systems with time-dependent damping in the whole space $R^d$, with $d \ge 1$. Using an approach similar to that developed by Crin-Barat and Danchin, we establish the global existence of small-amplitude solutions for systems endowed with a damping term of the form $-\frac{K z}{(1+t)^{\alpha}}, \quad 0 < \alpha \le 1.$ We assume that the linearized system satisfies the Shizuta--Kawashima (SK) condition, which ensures that the dissipation acts on all characteristic components through coupling. The key idea is to construct a Lyapunov-type functional that compensates for the lack of full dissipation. Such a functional was first introduced by Beauchard and Zuazua in the framework of control theory.

In this talk, I will present recent work on numerical approximations of the stochastic Allen–Cahn equation driven by multiplicative trace-class noise. We consider a fully discrete scheme combining a drift-implicit Euler method in time with a spectral Galerkin approximation in space.
The main focus is on weak convergence analysis. I will explain how the spatial weak convergence rate improves upon the corresponding strong rate—by nearly one order in dimensions $d =1,2$ and by nearly one-half order in dimension $d=3$. For the temporal discretization, we obtain weak convergence rates close to order one in $d=1,2$ and close to $3/4$in $d=3$.
A key ingredient of the analysis is the derivation of suitable a priori estimates for the Kolmogorov equations associated with the spectral Galerkin semi-discretization. In addition, I will introduce techniques for handling operator traces involving stochastic integrals in the temporal weak error analysis.