Do black holes stop

Answer 1

Most likely on the other side of a black hole is nothing,

It is probably like a blender and would destroy you as you entered.

chris: the concept of the movie black hole where its a wall that you could walk through and be in a different universe or time isn't true. it comes from a collapsed star so it is more sperecal. the question isn't whats on the other side but whats in the center. to answer that....no one knows but we think its full of things its sucked in but everything is crushed down by the impossibly high gravity.

Answer 2

We will never know, but science theorizes that it does not. Answer

Steven Hawking has theorized that Black Holes emit "Hawking Radiation" and that the rate of emission is proportional to the cube of the hole's mass. Thus implies that they are evaporating and will, at some point in time, disappear. Large black holes (mass greater than the sun) will essentially last forever, this falls to 2 to 3 billion years for masses of 1011 kg. To get down to a black hole with a life span of 1 second, the hole would have to have a mass of about 2.28 × 105 kg. The recently constructed LHC in Europe was supposed to have the potential of creating mini-black holes, but these would evaporate almost as soon as they were created.

Answer 3

At one end is an open hole (aperture) with a diagonal mirror that reflects light to your eye. At the other end is a parabolic mirror that collects and concentrates light from a distant source.

Answer 4

A black hole is a region of space from which nothing, including light, can escape. It is the result of the deformation of spacetime caused by a very compact mass, thus the 'end' of a black hole is the very massive object.

Answer 5

There are at least two things. Gravity is one; lots and lots of gravity. This expenditure of gravity waves actually serves to very slowly reduce the mass of black holes. This is more than compensated for by the absorption of background radiation.

The other thing is indirect. Mass that is approaching and falling into the event horizon gives off large amounts of radiation, allowing us to see 'where a black hole is', even if we can't technically see the black hole itself.

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For "smaller" black holes, it is possible for mass itself to "escape" from the black hole, through a process known as Hawking Radiation, theorized by Stephen Hawking. Here's how it works.

In the VERY close vicinity of the black hole's event horizon, the energy density is astronomical. Basic relativity tells us that mass and energy are interchangeable, and quantum theory predicts that in a high-energy environment, particle pairs will be produced; from the energy, an electron and a positron will suddenly come into existence where neither was before. The particle pair will travel some very short distance and annihilate themselves, releasing as much energy as was consumed in the pair production. We suspect that this happens all the time.

IF one of those particles hits the event horizon AND THE OTHER ONE DOESN'T, then the particle cannot meet its antiparticle "twin", and will "appear" to have been emitted from the black hole.

So, theorizes Hawking, "small" black holes can evaporate by emitting radiation which can (at least theoretically) carry away mass from the black hole. Hawking has calculated the maximum mass at which this can occur, and these small - called "quantum black holes" - will dissipate over time.

Answer 6

To the best of our knowledge, at the end of the life-span of a black hole there might be an explosion marked by a gamma burst. This is consistent with theoretical work proposed by Stephen Hawking which posits that black holes interact thermodynamically with the universe such that they have a finite temperature and can emit particles and thereby lose energy through emissions (Hawking radiation) which causes a gradual reduction in the mass of the black hole. Since the rate of radiation is inversely proportional to the mass, this effect would increase as the black hole becomes smaller and eventually disappears; a process sometimes called black hole evaporation. This presumes that conditions allow for this evaporation, i.e., that the amount of infalling matter or absorbed energy is less than the amount of mass lost through this mechanism.

One space telescope has been launched with the goal of detecting this anticipated gamma-ray flash.

Answer 7

No. A black hole cannot stop attracting things by the force of gravity. It even can bend light.

really black holes can stop they start eating for a wile but then they go to sleep like a snake when it eats it goes to sleep the black hole in our galaxy joust woke up

Answer 8

Because human exploration and observation has not reached that point, we don't know for sure. Some of the ideas hypothesised are that there is nothing at all beyond it, that there may a bubble-like skin separating our universe from the next, and that there simply isn't an end (although there is evidence against this idea).

Answer 9

Black holes can 'disappear' by 'evaporation'. Some of their energy is radiated off as 'Hawking radiation' (named for the handicapped but brilliant theoretical physicist). This is a quantum effect. It has never been observed directly, but the rate of shrinkage would be dependent on the size of the black hole, and any new mass being added to the singularity.

Answer 10

Nobody knows what is on the other side of a black hole. Because if we were to go into one, we would die. And we haven't been able to get close enough to one to really study it's potential. they could possibly be another world on the other side, we can't say for sure.