can watch Virtual bridges Which somehow connects faraway regions of space (and time), such as various black holes, which means it’s possible that these legendary monsters have already been sighted, according to RT.
But fortunately, if the new model proposed by a small team of physicists at Sofia University in Bulgaria is accurate, they can still be distinguished.
And by playing a lot with Einstein’s general theory of relativity, going through and hacking it, it is possible to show how the space-time background in the universe can not only create deep gravitational wells from which nothing escapes – it can also form impossible mountain peaks that cannot be climbed. And these glowing mounds will deflect anything that comes near them, producing streams of particles and radiation that have no hope of returning.
Aside from the obvious possibility that the Big Bang appears to be one of these “white holes”, nothing of the kind has ever been observed. Nevertheless, it remains an interesting concept for probing the edges of one of physics’ greatest theories.
In the 1930s, Einstein’s colleague Nathan Rosen showed that it was impossible to say that the deeply curved space-time of a black hole could not connect to the steep peaks of a white hole to form a kind of bridge.
And in this corner of physics, our everyday predictions about distance and time go out the window, implying that such a theoretical correlation could traverse vast expanses of the universe.
Under the right conditions, it might be possible for matter to fly into this cosmic tube and exit the other end with its information more or less intact.
So to determine what this black hole might look like in observatories such as the Event Horizon Telescope, the Sophia University team developed a simplified model of the wormhole’s “throat” as a magnetized ring of liquid and made various assumptions about how matter formed.
Particles caught in this raging storm will create powerful electromagnetic fields that roll and bounce in predictable patterns, polarizing any light that is emitted from the hot material with a distinctive signature. And it was the tracking of polarized radio waves that gave us the first stunning images of M87* in 2019 and Sagittarius A* earlier this year.
It turns out that the hot edges of the wormhole are hard to distinguish from the polarized light emitted from the chaotic disk surrounding the black hole.
By that logic, M87* could be a wormhole. In fact, wormholes could be lurking at the end of black holes everywhere, and we have no easy way of knowing.
This does not mean that there is no way to find out.
And if we put together an image of a candidate wormhole as seen indirectly through decent gravitational lensing, the subtle characteristics that distinguish wormholes from black holes might emerge.
Of course, this would require matter being properly positioned between us and the wormhole to distort its light enough to magnify the small differences, but it would at least give us a way to detect dark spots in space that have a back exit.
Another means that also requires a fair amount of wealth. And if we spot a wormhole at the perfect angle, the light passing through its divisive entrance towards us will enhance its signature even further, giving us a clearer indication of the portal through the stars and beyond.
Further modeling could reveal other properties of light waves that help sort wormholes from the night sky without the need for a perfect lens or angles, a possibility that researchers are now turning their attention to.
Placing more constraints on the physics of wormholes could reveal new avenues for research not only in general relativity, but also in the physics that describes the behavior of waves and particles.