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How do you go through a black hole?

Updated: 8/18/2019
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13y ago

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You don't go through it. You fall into it, get destroyed, and the matter stays right there.

Answer:

Black hole, in astronomy, is a celestial object of such extremely intense gravity that it attracts everything near it and in some instances prevents everything, including light, from escaping.

Types of Black Holes:

A stellar black hole is a black hole formed by the gravitational collapse of a massive star (more massive than about 20 solar masses) at the end of its lifetime.

A primordial black hole is a hypothetical type of black hole that is formed not by the gravitational collapse of a large star but by the extreme density of matter present during the universe's early expansion.

A Schwarzschild black hole has no charge and no angular momentum.

A Reissner-Nordstrom black hole has charge but no angular momentum.

A Kerr black hole has angular momentum but no charge.

A Kerr-Newman black hole has charge and angular momentum.

As for the question, an observer falling into a Schwarzschild black hole (i.e. non-rotating and no charges) cannot avoid the singularity. Any attempt to do so will only shorten the time taken to get there. When they reach the singularity, they are crushed to infinite density and their mass is added to the total of the black hole. Before that happens, they will have been torn apart by the growing tidal forces in a process sometimes referred to as spaghettification or the noodle effect.

While, in the case of a charged (Reissner-Nordström) or rotating (Kerr) black hole it is possible to avoid the singularity. Extending these solutions as far as possible reveals the hypothetical possibility of exiting the black hole into a different spacetime with the black hole acting as a worm hole. The possibility of travelling to another universe is however only theoretical, since any perturbation will destroy this possibility. It also appears to be possible to follow closed timelike curves (going back to one's own past) around the Kerr singularity, which lead to problems with causality like the grandfather paradox. It is expected that none of these peculiar effects would survive in a proper quantum mechanical treatment of rotating and charged black holes.

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