Limit profiles for singularly perturbed Choquard equations with local repulsion

preprint2022arXivOpen access

Abstract

We study Choquard type equation of the form −Δu+εu−(Iα∗∣u∣p)∣u∣p−2u+∣u∣q−2u=0inRN,(Pε)-Δu +\varepsilon u-(I_α*|u|^p)|u|^{p-2}u+|u|^{q-2}u=0\quad in \quad {\mathbb R}^N,\qquad\qquad(P_\varepsilon) where N≥3N\geq3, IαI_α is the Riesz potential with α∈(0,N)α\in(0,N), p>1p>1, q>2q>2 and ε≥0\varepsilon\ge 0. Equations of this type describe collective behaviour of self-interacting many-body systems. The nonlocal nonlinear term represents long-range attraction while the local nonlinear term represents short-range repulsion. In the first part of the paper for a nearly optimal range of parameters we prove the existence and study regularity and qualitative properties of positive groundstates of (P0)(P_0) and of (Pε)(P_\varepsilon) with ε>0\varepsilon>0. We also study the existence of a compactly supported groundstate for an integral Thomas-Fermi type equation associated to (Pε)(P_\varepsilon). In the second part of the paper, for ε→0\varepsilon\to 0 we identify six different asymptotic regimes and provide a characterisation of the limit profiles of the groundstates of (Pε)(P_\varepsilon) in each of the regimes. We also outline three different asymptotic regimes in the case ε→∞\varepsilon\to\infty. In one of the asymptotic regimes positive groundstates of (Pε)(P_\varepsilon) converge to a compactly supported Thomas-Fermi limit profile. This is a new and purely nonlocal phenomenon that can not be observed in the local prototype case of (Pε)(P_\varepsilon) with α=0α=0. In particular, this provides a justification for the Thomas-Fermi approximation in astrophysical models of self-gravitating Bose-Einstein condensate.

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