GW190521 as a Merger of Proca Stars: A Potential New Vector Boson of 8.7 x 10 -13 eV

Abstract

Advanced LIGO-Virgo have reported a short gravitational-wave signal (GW190521) interpreted as a quasicircular merger of black holes, one at least populating the pair-instability supernova gap, that formed a remnant black hole of 𝑀𝑓 ∼142 𝑀⊙ at a luminosity distance of 𝑑𝐿 ∼5.3 Gpc. With barely visible pre-merger emission, however, GW190521 merits further investigation of the pre-merger dynamics and even of the very nature of the colliding objects. We show that GW190521 is consistent with numerically simulated signals from head-on collisions of two (equal mass and spin) horizonless vector boson stars (aka Proca stars), forming a final black hole with 𝑀𝑓 =23⁢1+13−17 𝑀⊙, located at a distance of 𝑑𝐿 =57⁢1+348−181 Mpc. This provides the first demonstration of close degeneracy between these two theoretical models, for a real gravitational-wave event. The favored mass for the ultralight vector boson constituent of the Proca stars is 𝜇V =8.7⁢2+0.73−0.82 ×10−13 eV. Confirmation of the Proca star interpretation, which we find statistically slightly preferred, would provide the first evidence for a long sought dark matter particle.