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http://proza.ru/2024/12/17/1107
must be constructed at distances larger than
. Alternatively, a fast black hole can leave a narrow tunnel in a solid object while passing through it. For example, a
g black hole should leave a tunnel with a radius of 0.
, which is large enough to be seen by an optical microscope. We could look for such micro-tunnels here on Earth in very old rocks, or even glass or other solid structures in very old buildings. While our estimate gives a very small probability of finding such tunnels, looking for them does not require expensive equipment and long preparation, and the payoff might be significant.
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