On Singularity formation for the L^2-critical Boson star equation

preprint2011arXivOpen access

Abstract

We prove a general, non-perturbative result about finite-time blowup solutions for the L2L^2-critical boson star equation i∂tu=−Δ+m2 u−(∣x∣−1∗∣u∣2)ui\partial_t u = \sqrt{-Δ+m^2} \, u - (|x|^{-1} \ast |u|^2) u in 3 space dimensions. Under the sole assumption that the solution blows up in H1/2H^{1/2} at finite time, we show that u(t)u(t) has a unique weak limit in L2L^2 and that ∣u(t)∣2|u(t)|^2 has a unique weak limit in the sense of measures. Moreover, we prove that the limiting measure exhibits minimal mass concentration. A central ingredient used in the proof is a "finite speed of propagation" property, which puts a strong rigidity on the blowup behavior of uu. As the second main result, we prove that any radial finite-time blowup solution uu converges strongly in L2L^2 away from the origin. For radial solutions, this result establishes a large data blowup conjecture for the L2L^2-critical boson star equation, similar to a conjecture which was originally formulated by F. Merle and P. Raphael for the L2L^2-critical nonlinear Schrödinger equation in [CMP 253 (2005), 675-704]. We also discuss some extensions of our results to other L2L^2-critical theories of gravitational collapse, in particular to critical Hartree-type equations.

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