Polarimetry imprints of exotic compact objects: Solitonic boson stars
Phys. Rev. D 111, 124036 – Published 20 June, 2025
DOI: https://doi.org/10.1103/h8ln-psjr
Abstract
In this work we analyze the polarization observational properties of solitonic boson stars orbited by spherical hot spots emitting synchrotron radiation from a thermal distribution of electrons. We consider three boson star configurations with different compactnesses ranging from a dilute model with a large radius to an ultracompact model capable of holding null bound orbits. We observe that the polarimetric imprints of the primary images for all models are comparable to those of the Schwarzschild spacetime, and thus any potentially distinguishable differences must arise from the additional structure of secondary and plunge-through images. For low inclination (20°) observations, we find that the two QU loops of the least compact model are in contradiction with the current ALMA and GRAVITY observations and effectively exclude the possibility of Sgr A* being a dilute solitonic boson star. For high inclination (80°) observations, both the electric vector position angle and the QU loops present large qualitative deviations from the Schwarzschild black hole for all models analyzed. Our results emphasize the suitability of polarimetry as a framework to test the nature of supermassive compact objects with future observations, especially at high inclination.
