Cauchy data for multiple collapsing boson stars
Elena Giorgi, Dawei Shen, Jingbo Wan
TL;DR
The paper constructs asymptotically flat Cauchy initial data for the Einstein-Maxwell-Klein-Gordon system describing N well-separated charged boson stars, arranged so that their futures contain N causally independent trapped surfaces. The authors develop a six-part strategy combining a short-pulse mechanism, a stability-enabled transition region, a multi-centered charged Brill-Lindquist exterior, and a localized Klein-Gordon star region, culminating in an electrovacuum gluing that preserves charges. This extends previous vacuum N-body collapse results to a matter-coupled setting, providing a rigorous, fully geometric realization of dynamical multi-body boson-star collapse with controlled interaction. The construction yields initial data free of trapped surfaces that evolve to form multiple disjoint trapped surfaces in finite time, highlighting the rich and intricate dynamics of EMKG systems in general relativity and contributing to the broader understanding of N-body gravitational interactions in nonlinear field theories.
Abstract
We construct Cauchy initial data for the Einstein-Maxwell-Klein-Gordon (EMKG) system, which evolves in finite time into spacetimes containing multiple trapped surfaces. From a physical perspective, this corresponds to preparing multiple well-separated boson stars, each of which collapses to form a spacelike black hole region. In particular, this extends the result of the second and third named authors on the formation of multiple trapped surfaces in vacuum to the EMKG system.
