can watch Virtual bridges Which connects distant regions of space (and time) in one way or another, like various black holes, meaning it’s possible these legendary monsters have already been seen, according to RT.
But fortunately, if the new model proposed by a small team of physicists at Sofia University in Bulgaria is accurate, it is still possible to tell them apart.
And playing a lot with Einstein’s general theory of relativity, navigating and penetrating into it, it can be shown how the spatio-temporal background (time and space) in the universe can form not only deep gravitational pits where nothing escapes, but can also form Impossible mountain tops that can’t be climbed. And these hills of light would have moved away from anything that came close, which would have led to streams of particles and radiation that had no hope of flowing back.
Aside from the obvious possibility that the Big Bang appears to be one of these “white holes,” nothing like it has ever been observed. Nonetheless, it remains an interesting concept for exploring the limits of one of the greatest theories in physics.
In the 1930s a colleague of Einstein’s, Nathan Rosen, showed that there was nothing to say that the deeply curved space-time of a black hole couldn’t connect to the steep peaks of a white hole to form a kind of bridge.
And in this corner of physics, our day-to-day predictions of distance and time go out the window, meaning such a theoretical link could span large swathes of the universe.
Under the right conditions, it might even be possible for matter to enter this cosmic tube and exit the other end with its information more or less intact.
Then, to determine what this black hole might look like to observatories such as the Event Horizon Telescope, the Sofia University team developed a simplified model of the wormhole’s “throat” as a ring of magnetized liquid, and made various hypotheses about the origin of matter.
Particles trapped in this raging storm will produce powerful electromagnetic fields that will tumble and crack in predictable patterns, polarizing any light emitted by the hot material with a distinct signature. And it was tracking of polarized radio waves that gave us the first incredible images of M87* in 2019 and Sagittarius A* earlier this year.
It turns out that the wormhole’s hot edges are hard to distinguish from the polarized light emitted by the chaos disk surrounding the black hole.
According to this logic, M87* could be a wormhole. In fact, wormholes could be lurking at the ends of black holes anywhere, and we wouldn’t have an easy way to find out.
That doesn’t mean there’s no way to know.
And if we piece together a picture of a candidate wormhole seen indirectly through a decent gravitational lens, the subtle features that distinguish wormholes from black holes may become apparent.
This would require a mass conveniently placed between us and the wormhole to distort its light enough to amplify the small differences, of course, but at least it would give us a means of detecting dark spots in space that have a back exit.
Another medium also requires a fair amount of wealth. And if we detect a wormhole at an ideal angle, the light traveling through its dividing entrance towards us will further enhance its signature, giving us a clearer indication of a portal through the stars and beyond.
Further modeling could reveal other properties of light waves that help separate wormholes from the night sky without the need for a lens or ideal angles, a possibility researchers are now turning their attention to.
Imposing more constraints on wormhole physics could open up new ways to probe not only general relativity, but also the physics that describes the behavior of waves and particles.
