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The Invisible at the Galaxy's Heart: Black Hole or Ghost Star?

Original: "Bayesian Analysis of Massive Boson Star Models for Sagittarius A* Using Near-Infrared Astrometry Data"
arXiv:2605.09521v1 · 2026-05-10 · CC BY · ⏱ 1 min · High Energy General Relativity
The center of the Milky Way might not be an abyss but a giant invisible ball of dark matter.
Abstract

Scientists tested whether the motion of hot spots near Sagittarius A* can distinguish a black hole from a boson star—a clump of ultralight particles. It turned out that with current data, both are equally probable. It’s like trying to guess from a shadow whether it’s a rock or a ball.

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In the center of our galaxy, as in many others, lies an active nucleus — a massive object holding stars in their orbits. It's conventionally thought to be a black hole, a bottomless pit from which not even light escapes. However, the data allows for another option: it could be an invisible, ultra-dense ball.

Two heavy balls of equal mass, one solid and one hollow, are indistinguishable to a light ribbon circling around them. Similarly, the orbits of hot spots of light do not reveal the nature of the central body. Computer simulations showed: the image of a spot around a black hole and around a boson star — a superdense clump of particles moving as one — match the telescope data in brightness and polarization. These star-balls, akin to neutron stars (stellar remnants compressed to city size), may consist of axions — particles that likely make up dark matter, the invisible scaffolding of the universe.

Future detectors of gravitational waves, ripples in spacetime, may solve the mystery. For now, we can only guess: perhaps at the heart of the Milky Way hides not an abyss, but a ball that, with a mass of millions of suns, would fit inside Mercury's orbit — almost like a black hole, but made of substance.

🎯 A boson star with a mass of millions of suns would be so compact that its radius would exceed the critical size of a black hole by only three times — essentially, it would fit inside Mercury's orbit.

ds^2 = -A(r) dt^2 + B(r)^{-1} dr^2 + r^2 (d\theta^2 + \sin^2\theta d\phi^2)
Unlike a black hole, there is no event horizon here — the metric functions A and B are finite everywhere.
Z = \int_{\Omega_\Theta} \mathcal{L}(\Theta) \pi(\Theta) d\Theta
Integral of likelihood over prior distribution, a quantitative measure of how well the model explains the data.
Scientists
Stephen HawkingJacob BekensteinAlbert EinsteinFritz ZwickyVera RubinBernhard Riemann
Tags
black hole dark matter axion Bose-Einstein condensate numerical simulation gravitational waves neutron star active galactic nucleus galaxy polarimetry photometry
Laws
Hawking radiationgravitational lensingBekenstein-Hawking entropyEinstein field equationsStefan–Boltzmann lawFermi–Dirac statistics
Original: arXiv:2605.09521v1 · CC BY · bridge42worlds