Piercing of a boson star by a black hole
Vítor Cardoso, Taishi Ikeda, Zhen Zhong, Zillao, Miguel
Abstract
New light fundamental fields are natural candidates for all or a fraction of dark matter. Self-gravitating structures of such fields might be common objects in the universe, and could comprise even galactic halos. These structures would interact gravitationally with black holes, a process of the utmost importance since it dictates their lifetime, the black hole motion, and possible gravitational radiation emission. Here, we study the dynamics of a black hole piercing through a much larger fully relativistic boson star, made of a complex minimally coupled massive scalar without self-interactions. As the black hole pierces through the bosonic structure, it is slowed down by accretion and dynamical friction, giving rise to gravitational-wave emission. Since we are interested in studying the interaction with large and heavy scalar structures, we consider mass ratios up to $q\ensuremath{\sim}10$ and length ratios $\mathcal{L}\ensuremath{\sim}62$. Somewhat surprisingly, for all our simulations, the black hole accretes more than 95% of the boson star material, even if an initially small black hole collides with large velocity. This is a consequence of an extreme ``tidal capture'' process, which binds the black hole and the boson star together, for these mass ratios. We find evidence of a ``gravitational atom'' left behind as a product of the process.