Explain the formation of Warm Hole...??
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In 1935, Albert Einstein and his colleague Nathan Rosen showed that black holes can theoretically be connected via ‘wormholes’ – shortcuts through space and time that could link up black holes light-years apart.
To create a wormhole on Earth, we’d first need a black hole. This is problematic: creating a black hole just a centimetre across would require crushing a mass roughly equal to that of the Earth down to this tiny size. Plus, in the 1960s theorists showed that wormholes would be incredibly unstable.
It could be possible to stabilise the wormhole using so-called ‘exotic matter’, whose existence is predicted by quantum theory. This weird stuff is expected to have an antigravitational effect, which could stop the wormhole collapsing. But no one has a clue how to do any of this. And even if they did, it might all be pointless: theorists now suspect that travelling via wormholes would actually take longer than simply taking the conventional route through space.
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Explain the formation of Warmhole?
Earlier this year, physicists proposed an answer in the form of “wormholes,” or gravitational tunnels. The group showed that by creating two entangled black holes, then pulling them apart, they formed a wormhole— essentially a “shortcut” through the universe — connecting the distant black holes.
A wormhole (or Einstein–Rosen bridge or Einstein–Rosen wormhole) is a speculative structure linking disparate points in spacetime, and is based on a special solution of the Einstein field equations. A wormhole can be visualized as a tunnel with two ends at separate points in spacetime (i.e., different locations, or different points in time, or both).
Wormholes are consistent with the general theory of relativity, but whether wormholes actually exist remains to be seen. Many scientists postulate wormholes are merely a projection of a fourth spatial dimension, analogous to how a two-dimensional (2D) being could experience only part of a three-dimensional (3D) object.
A wormhole could connect extremely long distances such as a billion light years or more, short distances such as a few meters, different universes, or different points in time.