Asymptotic behavior of gradient-like dynamical systems involving inertia and multiscale aspects

In a Hilbert space $\mathcal H$, we study the asymptotic behaviour, as time variable $t$ goes to $+\infty$, of nonautonomous gradient-like dynamical systems involving inertia and multiscale features. Given $\mathcal H$ a general Hilbert space, $\Phi: \mathcal H \rightarrow \mathbb R$ and $\Psi: \mathcal H \rightarrow \mathbb R$ two convex differentiable functions, $\gamma$ a positive damping parameter, and $\epsilon (t)$ a function of $t$ which tends to zero as $t$ goes to $+\infty$, we consider the second-order differential equation $$\ddot{x}(t) + \gamma \dot{x}(t) + \nabla \Phi (x(t)) + \epsilon (t) \nabla \Psi (x(t)) = 0.$$ This system models the emergence of various collective behaviors in game theory, as well as the asymptotic control of coupled nonlinear oscillators. Assuming that $\epsilon(t)$ tends to zero moderately slowly as $t$ goes to infinity, we show that the trajectories converge weakly in $\mathcal H$. The limiting equilibria are solutions of the hierarchical minimization problem which consists in minimizing $\Psi$ over the set $C$ of minimizers of $\Phi$. As key assumptions, we suppose that $\int_{0}^{+\infty}\epsilon (t) dt = + \infty$ and that, for every $p$ belonging to a convex cone $\mathcal C$ depending on the data $\Phi$ and $\Psi$ $$\int_{0}^{+\infty} \left[\Phi^* \left(\epsilon (t)p\right) -\sigma_C \left(\epsilon (t)p\right)\right]dt < + \infty$$ where $\Phi^*$ is the Fenchel conjugate of $\Phi$, and $\sigma_C$ is the support function of $C$. An application is given to coupled oscillators

A minimization problem for the lapse and the initial-boundary value problem for Einstein's field equations

We discuss the initial-boundary value problem of General Relativity. Previous considerations for a toy model problem in electrodynamics motivate the introduction of a variational principle for the lapse with several attractive properties. In particular, it is argued that the resulting elliptic gauge condition for the lapse together with a suitable condition for the shift and constraint-preserving boundary conditions controlling the Weyl scalar Psi_0 are expected to yield a well posed initial-boundary value problem for metric formulations of Einstein's field equations which are commonly used in numerical relativity. To present a simple and explicit example we consider the 3+1 decomposition introduced by York of the field equations on a cubic domain with two periodic directions and prove in the weak field limit that our gauge condition for the lapse and our boundary conditions lead to a well posed problem. The method discussed here is quite general and should also yield well posed problems for different ways of writing the evolution equations, including first order symmetric hyperbolic or mixed first-order second-order formulations. Well posed initial-boundary value formulations for the linearization about arbitrary stationary configurations will be presented elsewhere.Comment: 34 pages, no figure