Head-on collisions of $\ell$-boson stars
V\'ictor Jaramillo, Nicolas Sanchis-Gual, Juan Barranco, Argelia, Bernal, Juan Carlos Degollado, Carlos Herdeiro, Miguel Megevand, Dar\'io, N\'u\~nez

TL;DR
This study uses numerical simulations to analyze head-on collisions of $ ext{l}$-boson stars, revealing conditions for black hole formation, bound states, and deviations from spherical symmetry, contributing to understanding multi-field boson star dynamics.
Contribution
First detailed numerical analysis of head-on collisions of $ ext{l}$-boson stars, exploring outcomes and end states in various collision scenarios.
Findings
Collisions of sufficiently massive stars produce black holes.
Below a mass threshold, stars form stable bound states.
Post-collision states are generally non-spherical and deviate from initial symmetry.
Abstract
Fully non-linear numerical evolutions of the Einstein-(multi)--Klein-Gordon equations are performed to study head-on collisions of -boson stars. Despite being spherically symmetric, -boson stars have a (hidden) frame of reference, used in defining their individual multipolar fields. To assess the impact of their relative orientation, we perform simulations with different angles between the axes of the two colliding stars. Additionally, two scenarios are considered for the colliding stars: that they are composites of either the same or different scalar fields. Despite some model-specific behaviours, the simulations generically indicate that: 1) the collision of two sufficiently (and equally) massive stars leads to black hole formation; 2) below a certain mass threshold the end result of the evolution is a bound state of the composite scalar fields, that neither disperses nor…
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Taxonomy
TopicsPulsars and Gravitational Waves Research · Astrophysical Phenomena and Observations · Black Holes and Theoretical Physics
